Pith. sign in

REVIEW 1 major objections 2 minor 1 cited by

The magnetic field of the Milky Way: an observational perspective

T0 review · 1 major / 2 minor · reviewed 2026-06-28 · grok-4.3

Challenge this review Re-run · record.json Download PDF Read on arXiv ↗

Pith's one-line read The Milky Way's magnetic field roughly follows the spiral arms in the disk with an additional perpendicular component in the halo.

desk verdict This is a straightforward review that organizes existing observations on the Milky Way magnetic field without adding new data or analysis. read the letter →

arxiv 2606.02149 v1 pith:T5ZI73O3 submitted 2026-06-01 astro-ph.GA

Marijke Haverkorn This is my paper · ORCID
classification astro-ph.GA
keywords magneticfieldsMilkyWayFaradayrotationGalactichalospiralarmsinterstellarmediumdynamomodesturbulentfield
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

This review compiles observational data to describe the large-scale magnetic field structure of the Milky Way. It shows that the field aligns with spiral arms in the Galactic disk and has a vertical component away from the plane in the halo, with a different overall configuration in the disk versus the gaseous halo that matches expectations from distinct dynamo modes. These conclusions rest on measurements of Faraday rotation, synchrotron emission, and polarization. The field structure affects gas dynamics, star formation, and cosmic ray propagation across the Galaxy. Smaller-scale turbulence in the field appears anisotropic and intermittent, with orientations linked to multi-phase gas and dust.

What carries the argument

Large-scale magnetic field geometry and strength mapped through Faraday rotation measures, synchrotron polarization, and optical starlight polarization from diffuse interstellar media.

What would settle it

A new comprehensive rotation measure grid or polarization survey that shows the large-scale field neither follows the spiral arms nor exhibits the perpendicular halo component would falsify the described configuration.

Watch

Extended reading notes

Core claim

On Galaxy-wide scales, the magnetic field roughly follows the spiral arms in the Galactic disk, and includes an additional component perpendicular to the disk away from the Galactic plane. The field configuration is different in the Galactic disk and the Galactic gaseous halo, qualitatively consistent with different dominating dynamo modes. Deviations from this idealized model are ubiquitously observed and include anomalously high Faraday rotation, variable magnetic field orientations and field reversals on kiloparsec scales. On smaller scales, the magnetic field is turbulent, anisotropic and intermittent.

Load-bearing premise

The body of cited observational results from Faraday rotation, polarization, and synchrotron emission accurately trace the true magnetic field geometry and strength with limited systematic contamination from other interstellar effects.

Editorial extensions

If this is right

  • The field influences turbulent gas dynamics, star formation, energy household, evolution of interstellar objects, and cosmic-ray propagation.
  • Deviations such as kiloparsec-scale field reversals and anomalously high Faraday rotation occur throughout the Galaxy.
  • On smaller scales the turbulent field is anisotropic and intermittent, with orientations correlated to cold and warm gas phases and dust distribution.
  • Increased data from rotation measure grids, Faraday tomography, and optical polarization measurements will allow refined mapping in coming years.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • The disk-halo difference in field structure could be tested by mapping dynamo signatures against independent measures of gas density and turbulence in each region.
  • Correlations between field orientation and multi-phase gas may indicate that magnetic fields help regulate the distribution of interstellar matter across phases.
  • Field reversals on kiloparsec scales might reflect local dynamical processes such as spiral arm interactions that overlay the global pattern.
Share X Bluesky LinkedIn Reddit HN

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit.

Referee Report

1 major / 2 minor

Summary. This review paper summarizes observational constraints on the magnetic field of the Milky Way from Faraday rotation measures, synchrotron emission, and polarization data. It claims that the large-scale magnetic field in the Galactic disk roughly follows the spiral arms with an additional perpendicular component away from the plane, while the configuration differs in the gaseous halo, qualitatively consistent with different dynamo modes. The paper also discusses ubiquitous deviations such as kpc-scale reversals and high RM values, and describes the small-scale field as turbulent, anisotropic, and correlated with multi-phase ISM and dust. Future prospects from RM grids, Faraday tomography, and optical polarization are highlighted.

Significance. If the cited observational results hold, this synthesis provides a valuable overview of the current state of knowledge on Galactic magnetic fields, highlighting the distinction between disk and halo fields and pointing to the potential of upcoming large datasets from RM grids and optical polarization measurements to advance the field.

major comments (1)
  1. [Abstract] Abstract: The central synthesis that the large-scale field configuration is qualitatively consistent with different dominating dynamo modes in disk versus halo rests on the assumption that RM, synchrotron, and polarization tracers accurately reflect global geometry with limited local contamination. The abstract itself flags kpc-scale reversals and anomalously high RM values as ubiquitous deviations, but does not quantify how these are separated from global properties versus arising from unaccounted local structures or multi-phase effects; this assumption is load-bearing for the dynamo interpretation.
minor comments (2)
  1. The review could add a short dedicated subsection (perhaps in the large-scale field discussion) explicitly addressing the error budget and potential systematics across the key cited studies, to make the robustness of the consensus clearer.
  2. Terms such as 'Faraday Tomography' and specific higher-order statistics for turbulence could include one-sentence definitions or references on first use for accessibility.

Simulated Author's Rebuttal

1 responses · 0 unresolved

We thank the referee for their thoughtful and constructive comment on our review. We address the major comment below and propose a targeted revision to the abstract.

read point-by-point responses

  1. Referee: [Abstract] Abstract: The central synthesis that the large-scale field configuration is qualitatively consistent with different dominating dynamo modes in disk versus halo rests on the assumption that RM, synchrotron, and polarization tracers accurately reflect global geometry with limited local contamination. The abstract itself flags kpc-scale reversals and anomalously high RM values as ubiquitous deviations, but does not quantify how these are separated from global properties versus arising from unaccounted local structures or multi-phase effects; this assumption is load-bearing for the dynamo interpretation.

    Authors: The abstract condenses the observational synthesis presented throughout the review, where multiple sections examine the evidence from RM, synchrotron, and polarization data while explicitly discussing kpc-scale reversals, high RM values, and the difficulties of isolating global patterns from local or multi-phase contributions. The dynamo-mode statement is already qualified as 'qualitatively consistent' rather than definitive. We acknowledge that the abstract could better flag the separation challenge for readers. We will therefore add a short qualifying clause to the abstract to make this limitation explicit. revision: partial

Circularity Check

0 steps flagged · score 0.0 of 10

No circularity: observational review with no derivations or self-referential predictions

full rationale

This is a review paper summarizing external observational results on Galactic magnetic fields from tracers such as Faraday rotation, synchrotron emission, and polarization. The abstract and structure present no new equations, fitted parameters, predictions, or derivations that could reduce to the paper's own inputs by construction. All claims cite external literature without self-citation load-bearing on uniqueness theorems or ansatzes, and no internal model is fitted or renamed as a prediction. The derivation chain is therefore self-contained against external benchmarks.

Assumptions & free parameters 0 free parameters · 0 assumptions · 0 invented entities

No new free parameters, axioms, or invented entities are introduced; the paper aggregates existing observational constraints from the literature.

how reviews work

0 comments
Cite this review

Pith. "Pith review of The magnetic field of the Milky Way: an observational perspective." pith.science (2026). https://pith.science/paper/T5ZI73O3

@misc{pith2026260602149,
  author       = {Pith},
  title        = {Pith review of: The magnetic field of the Milky Way: an observational perspective},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/T5ZI73O3}},
  note         = {Machine review of arXiv:2606.02149}
}
read the original abstract

Magnetic fields are an important and enigmatic component of the Milky Way's ecosystem. Mostly frozen into interstellar plasma, they play key roles in (turbulent) gas dynamics, star formation, energy household, evolution of interstellar objects, and cosmic-ray propagation. This paper reviews recent progress on measuring and characterizing these Galactic magnetic fields, limited to the larger-scale fields in mostly diffuse media, and to an observational perspective. On Galaxy-wide scales, the magnetic field roughly follows the spiral arms in the Galactic disk, and includes an additional component perpendicular to the disk away from the Galactic plane. The field configuration is different in the Galactic disk and the Galactic gaseous halo, qualitatively consistent with different dominating dynamo modes. Deviations from this idealized model are ubiquitously observed and include anomalously high Faraday rotation, variable magnetic field orientations and field reversals on kiloparsec scales. On smaller scales, the magnetic field is turbulent, anisotropic and intermittent. Much used descriptions of the turbulent magnetic field such as power laws and Gaussianity are being replaced by higher-order statistics that better capture the complexities of the field. Magnetic field orientations and possibly strength are correlated with both cold and warm components of the multi-phase interstellar gas, and with the interstellar dust distribution. The near future will bring a large increase in observational data in rotation measure grids, Faraday Tomography data and measurements of interstellar polarization of optical starlight, promising exciting developments in characterizing and understanding magnetic fields in the Milky Way in the next few years.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Transition from Diffusion to Drift-Dominated Cosmic Ray Transport and the Origin of the Knee

    astro-ph.HE 2026-06 unverdicted novelty 4.0 of 10

    Simulations show that drift dominance over diffusion can create a knee at PeV energies if parallel diffusion becomes energy-independent above 1 TeV, though some setups fail to match observed grammage.

Reference graph

Works this paper leans on

300 extracted references · 282 canonical work pages · cited by 1 Pith paper

  1. [1]

    Nature Astronomy , keywords =

    Constraints on the magnetic field in the Galactic halo from globular cluster pulsars. Nature Astronomy , keywords =. doi:10.1038/s41550-020-1030-6 , archivePrefix =. 2003.02867 , primaryClass =

    work page doi:10.1038/s41550-020-1030-6 2003

  2. [2]

    Faraday Rotation Measure due to the Intergalactic Magnetic Field

    Faraday Rotation Measure Due to the Intergalactic Magnetic Field. , keywords =. doi:10.1088/0004-637X/723/1/476 , archivePrefix =. 1009.0570 , primaryClass =

    work page Pith review arXiv doi:10.1088/0004-637x/723/1/476

  3. [3]

    Cosmic Magnetism in Centimeter and Meter Wavelength Radio Astronomy

    Cosmic magnetism in centimeter- and meter-wavelength radio astronomy. , keywords =. doi:10.1093/pasj/psx123 , archivePrefix =. 1709.02072 , primaryClass =

    work page Pith review arXiv doi:10.1093/pasj/psx123

  4. [4]

    Faraday Tomography with Sparse Modeling

    Faraday Tomography with Sparse Modeling. arXiv e-prints , keywords =. doi:10.48550/arXiv.1811.10610 , archivePrefix =. 1811.10610 , primaryClass =

    work page Pith review arXiv doi:10.48550/arxiv.1811.10610

  5. [5]

    , keywords =

    The RWST, a comprehensive statistical description of the non-Gaussian structures in the ISM. , keywords =. doi:10.1051/0004-6361/201834975 , archivePrefix =. 1905.01372 , primaryClass =

    work page doi:10.1051/0004-6361/201834975 1905

  6. [6]

    The Local Bubble: a magnetic veil to our Galaxy

    The Local Bubble: a magnetic veil to our Galaxy. , keywords =. doi:10.1051/0004-6361/201832637 , archivePrefix =. 1803.05251 , primaryClass =

    work page Pith review arXiv doi:10.1051/0004-6361/201832637

  7. [7]

    Monthly Notices of the Royal Astronomical Society , volume =

    Probing the magnetized gas distribution in galaxy groups and the cosmic web with POSSUM Faraday rotation measures. , keywords =. doi:10.1093/mnras/stae1954 , archivePrefix =. 2407.20325 , primaryClass =

    work page doi:10.1093/mnras/stae1954

  8. [8]

    , keywords =

    The Magnetic Field Strength in the Wall of the Local Bubble toward l, b -0.5ex 300 , 0. , keywords =. doi:10.1086/503199 , adsurl =

    work page doi:10.1086/503199

Show all 300 references
  1. [9]

    , keywords =

    Sparse Faraday Rotation Measure Synthesis. , keywords =. doi:10.1088/0004-6256/143/2/33 , archivePrefix =. 1111.4167 , primaryClass =

    doi arXiv

  2. [10]

    Interstellar Polarization Survey. V. Galactic magnetic field tomography in the spiral arms using optical and near-infrared starlight polarization. arXiv e-prints , keywords =. doi:10.48550/arXiv.2506.01564 , archivePrefix =. 2506.01564 , primaryClass =

    doi

  3. [11]

    Interstellar Polarization Survey. IV. Characterizing the Magnetic Field Strength and Turbulent Dispersion Using Optical Starlight Polarization in the Diffuse Interstellar Medium. , keywords =. doi:10.3847/1538-3881/ad4b14 , archivePrefix =. 2405.07347 , primaryClass =

    doi

  4. [12]

    A Powerful Local Shear Instability in Weakly Magnetized Disks. I. Linear Analysis. , keywords =. doi:10.1086/170270 , adsurl =

    doi

  5. [13]

    , keywords =

    Magnetic fields as an alternative explanation for the rotation curves of spiral galaxies. , keywords =. doi:10.1038/360652a0 , adsurl =

    doi

  6. [14]

    Nature Astronomy , keywords =

    The spectrum of magnetized turbulence in the interstellar medium. Nature Astronomy , keywords =. doi:10.1038/s41550-025-02551-5 , archivePrefix =. 2504.07136 , primaryClass =

    doi

  7. [15]

    , keywords =

    Galactic and Extragalactic Magnetic Fields. , keywords =. doi:10.1023/A:1013805401252 , archivePrefix =. astro-ph/0012402 , primaryClass =

    doi

  8. [16]

    Cosmic Magnetic Fields , year = 2005, editor =

    Magnetic Fields in Galaxies. Cosmic Magnetic Fields , year = 2005, editor =. doi:10.1007/3540313966_3 , adsurl =

    2005 doi

  9. [17]

    , keywords =

    Magnetic fields in the nearby spiral galaxy IC 342: A multi-frequency radio polarization study. , keywords =. doi:10.1051/0004-6361/201425572 , archivePrefix =. 1502.05439 , primaryClass =

    doi arXiv

  10. [18]

    , keywords =

    Systematic bias in interstellar magnetic field estimates. , keywords =. doi:10.1051/0004-6361:20031101 , archivePrefix =. astro-ph/0307330 , primaryClass =

    doi arXiv

  11. [19]

    , keywords =

    New constraints on modelling the random magnetic field of the MW. , keywords =. doi:10.1088/1475-7516/2016/05/056 , archivePrefix =. 1409.5120 , primaryClass =

    2016 doi arXiv

  12. [20]

    Planets, Stars and Stellar Systems

    Magnetic Fields in Galaxies. Planets, Stars and Stellar Systems. Volume 5: Galactic Structure and Stellar Populations , year = 2013, editor =. doi:10.1007/978-94-007-5612-0_13 , archivePrefix =. 1302.5663 , primaryClass =

    2013 doi

  13. [21]

    , keywords =

    Polarized synchrotron data and the structure of the Galactic magnetic field. , keywords =. doi:10.1103/PhysRevD.111.063057 , archivePrefix =. 2408.02554 , primaryClass =

    doi

  14. [22]

    , keywords =

    Improved CLEAN reconstructions for rotation measure synthesis with maximum likelihood estimation. , keywords =. doi:10.1051/0004-6361/201220771 , archivePrefix =. 1211.5105 , primaryClass =

    doi arXiv

  15. [23]

    The synergy of aperture and rotation measure synthesis

    Faraday synthesis. The synergy of aperture and rotation measure synthesis. , keywords =. doi:10.1051/0004-6361/201118672 , archivePrefix =. 1112.4175 , primaryClass =

    doi arXiv

  16. [24]

    , keywords =

    Contribution of neutral gas to Faraday tomographic data at low frequencies: A first extensive comparison between real and synthetic data. , keywords =. doi:10.1051/0004-6361/202557351 , archivePrefix =. 2602.08839 , primaryClass =

    doi arXiv

  17. [25]

    Interstellar polarization at high galactic latitudes from distant stars. V. First results for the South Galactic Pole. , keywords =. doi:10.1051/0004-6361:20010202-1 , adsurl =

    doi

  18. [26]

    Interstellar polarization at high galactic latitudes from distant stars. VII. A complete map for southern latitudes b < -70^. , keywords =. doi:10.1051/0004-6361:20040308 , adsurl =

    doi

  19. [27]

    , keywords =

    Magnetic fields in the disk and halo of M 51. , keywords =. doi:10.48550/arXiv.astro-ph/9610182 , archivePrefix =. astro-ph/9610182 , primaryClass =

    doi arXiv

  20. [28]

    , keywords =

    Strong magnetic fields in normal galaxies at high redshift. , keywords =. doi:10.1038/nature07105 , archivePrefix =. 0807.3347 , primaryClass =

    doi arXiv

  21. [29]

    U ber den Ursprung der Magnetfelder auf Sternen und im interstellaren Raum (mit einem Anhang von A. Schl \

    Biermann, Ludwig , journal=. \"U ber den Ursprung der Magnetfelder auf Sternen und im interstellaren Raum (mit einem Anhang von A. Schl \"u ter)

  22. [30]

    , keywords =

    A Three-dimensional Model for the Reversal in the Local Large-scale Interstellar Magnetic Field. , keywords =. doi:10.3847/1538-4357/ae28d1 , archivePrefix =. 2512.03332 , primaryClass =

    doi

  23. [31]

    , keywords =

    Associating LOFAR Galactic Faraday structures with the warm neutral medium. , keywords =. doi:10.1051/0004-6361/202348953 , archivePrefix =. 2404.19002 , primaryClass =

    doi

  24. [32]

    , keywords =

    IMAGINE: a comprehensive view of the interstellar medium, Galactic magnetic fields and cosmic rays. , keywords =. doi:10.1088/1475-7516/2018/08/049 , archivePrefix =. 1805.02496 , primaryClass =

    2018 doi arXiv

  25. [33]

    , keywords =

    Galactic Hydrostatic Equilibrium with Magnetic Tension and Cosmic-Ray Diffusion. , keywords =. doi:10.1086/169509 , adsurl =

    doi

  26. [34]

    arXiv e-prints , keywords =

    The multiphase interstellar medium as a common origin for magnetic misalignment and TB parity violation. arXiv e-prints , keywords =. doi:10.48550/arXiv.2512.11656 , archivePrefix =. 2512.11656 , primaryClass =

    doi arXiv

  27. [35]

    , keywords =

    The multiphase and magnetized neutral hydrogen seen by LOFAR. , keywords =. doi:10.1051/0004-6361/202039283 , archivePrefix =. 2011.05647 , primaryClass =

    2011 doi

  28. [36]

    , keywords =

    Link between E-B polarization modes and gas column density from interstellar dust emission. , keywords =. doi:10.1051/0004-6361/201935951 , archivePrefix =. 1905.10471 , primaryClass =

    1905 doi

  29. [37]

    doi:10.1146/annurev-astro-071221-052807 , year = 2023, month =

    Axel Brandenburg and Evangelia Ntormousi , title =. doi:10.1146/annurev-astro-071221-052807 , year = 2023, month =

    2023 doi

  30. [38]

    , keywords =

    Faraday rotation measure synthesis. , keywords =. doi:10.1051/0004-6361:20052990 , archivePrefix =. astro-ph/0507349 , primaryClass =

    doi arXiv

  31. [39]

    , keywords =

    Classifying complex Faraday spectra with convolutional neural networks. , keywords =. doi:10.1093/mnras/sty2908 , archivePrefix =. 1711.03252 , primaryClass =

    doi arXiv

  32. [40]

    , keywords =

    Rotation Measures of Extragalactic Sources behind the Southern Galactic Plane: New Insights into the Large-Scale Magnetic Field of the Inner Milky Way. , keywords =. doi:10.1086/518499 , archivePrefix =. 0704.0458 , primaryClass =

    doi arXiv

  33. [41]

    , keywords =

    Rotation Measures of Compact Sources in the Canadian Galactic Plane Survey. , keywords =. doi:10.1086/346082 , adsurl =

    doi

  34. [42]

    , keywords =

    Properties of Interstellar Turbulence from Gradients of Linear Polarization Maps. , keywords =. doi:10.1088/0004-637X/749/2/145 , archivePrefix =. 1111.3544 , primaryClass =

    doi arXiv

  35. [43]

    , keywords =

    Density Studies of MHD Interstellar Turbulence: Statistical Moments, Correlations and Bispectrum. , keywords =. doi:10.1088/0004-637X/693/1/250 , archivePrefix =. 0811.0822 , primaryClass =

    doi arXiv

  36. [44]

    , keywords =

    In Situ Observations of Magnetic Turbulence in the Local Interstellar Medium. , keywords =. doi:10.1088/2041-8205/804/2/L31 , adsurl =

    doi

  37. [45]

    , year = 1966, month = jan, volume =

    On the depolarization of discrete radio sources by Faraday dispersion. , year = 1966, month = jan, volume =. doi:10.1093/mnras/133.1.67 , adsurl =

    1966 doi

  38. [46]

    , keywords =

    Anomalous persistence of bisymmetric magnetic structures in spiral galaxies. , keywords =. doi:10.1093/mnras/292.1.1 , adsurl =

    doi

  39. [47]

    Soviet Astronomy Letters , year = 1985, month = mar, volume =

    Shock Generation of Turbulence and Cosmic-Ray Diffusion in the Interstellar Medium. Soviet Astronomy Letters , year = 1985, month = mar, volume =

    1985

  40. [48]

    , keywords =

    A Comparison of Multiphase Magnetic Field Tracers in a High Galactic Latitude Region of the Filamentary Interstellar Medium. , keywords =. doi:10.3847/1538-4357/ac400d , archivePrefix =. 2112.03247 , primaryClass =

    doi

  41. [49]

    arXiv e-prints , keywords =

    Stable Signal Recovery from Incomplete and Inaccurate Measurements. arXiv e-prints , keywords =. doi:10.48550/arXiv.math/0503066 , archivePrefix =. math/0503066 , primaryClass =

    doi arXiv

  42. [50]

    , keywords =

    CS-ROMER: a novel compressed sensing framework for Faraday depth reconstruction. , keywords =. doi:10.1093/mnras/stac3031 , archivePrefix =. 2205.01413 , primaryClass =

    doi

  43. [51]

    , keywords =

    The nature of LOFAR rotation measures and new constraints on magnetic fields in cosmic filaments and on magnetogenesis scenarios. , keywords =. doi:10.1051/0004-6361/202451333 , archivePrefix =. 2411.13499 , primaryClass =

    doi

  44. [52]

    , keywords =

    Magnetic field strength in cosmic web filaments. , keywords =. doi:10.1093/mnras/stac384 , archivePrefix =. 2202.04607 , primaryClass =

    doi

  45. [53]

    , keywords =

    S-band Polarization All-Sky Survey (S-PASS): survey description and maps. , keywords =. doi:10.1093/mnras/stz806 , archivePrefix =. 1903.09420 , primaryClass =

    1903 doi

  46. [54]

    , keywords =

    Giant magnetized outflows from the centre of the Milky Way. , keywords =. doi:10.1038/nature11734 , archivePrefix =. 1301.0512 , primaryClass =

    doi arXiv

  47. [55]

    , keywords =

    Non-linear Galactic Dynamos and the Magnetic Pitch Angle. , keywords =. doi:10.1088/0004-637X/808/1/28 , archivePrefix =. 1506.03245 , primaryClass =

    doi arXiv

  48. [56]

    , keywords =

    The effect of magnetic field on the inner Galactic rotation curve. , keywords =. doi:10.1093/mnrasl/slac091 , archivePrefix =. 2208.06098 , primaryClass =

    doi

  49. [57]

    , year = 1953, month = jul, volume =

    Magnetic Fields in Spiral Arms. , year = 1953, month = jul, volume =. doi:10.1086/145731 , adsurl =

    1953 doi

  50. [58]

    , keywords =

    A measurement of Galactic synchrotron emission using MWA drift scan observations. , keywords =. doi:10.1017/pasa.2025.10065 , archivePrefix =. 2506.14310 , primaryClass =

    2025 doi

  51. [59]

    , keywords =

    The First CHIME/FRB Fast Radio Burst Catalog. , keywords =. doi:10.3847/1538-4365/ac33ab , archivePrefix =. 2106.04352 , primaryClass =

    doi

  52. [60]

    , keywords =

    A Technique for Constraining the Driving Scale of Turbulence and a Modified Chandrasekhar-Fermi Method. , keywords =. doi:10.3847/0004-637X/821/1/21 , archivePrefix =. 1603.08537 , primaryClass =

    doi arXiv

  53. [61]

    , year = 2009, month = mar, volume =

    The Spitzer/GLIMPSE Surveys: A New View of the Milky Way. , year = 2009, month = mar, volume =. doi:10.1086/597811 , adsurl =

    2009 doi

  54. [62]

    , keywords =

    The Origin of Parity Violation in Polarized Dust Emission and Implications for Cosmic Birefringence. , keywords =. doi:10.3847/1538-4357/ac0e35 , archivePrefix =. 2105.00120 , primaryClass =

    doi

  55. [63]

    , keywords =

    Mapping the Magnetic Interstellar Medium in Three Dimensions over the Full Sky with Neutral Hydrogen. , keywords =. doi:10.3847/1538-4357/ab5803 , archivePrefix =. 1909.11673 , primaryClass =

    1909 doi

  56. [64]

    , keywords =

    A New Probe of Line-of-sight Magnetic Field Tangling. , keywords =. doi:10.3847/2041-8213/aabb54 , archivePrefix =. 1802.00011 , primaryClass =

    doi arXiv

  57. [65]

    , keywords =

    Neutral Hydrogen Structures Trace Dust Polarization Angle: Implications for Cosmic Microwave Background Foregrounds. , keywords =. doi:10.1103/PhysRevLett.115.241302 , archivePrefix =. 1508.07005 , primaryClass =

    doi arXiv

  58. [66]

    , keywords =

    Magnetically Aligned H I Fibers and the Rolling Hough Transform. , keywords =. doi:10.1088/0004-637X/789/1/82 , archivePrefix =. 1312.1338 , primaryClass =

    doi arXiv

  59. [67]

    , keywords =

    The Galactic Plane Infrared Polarization Survey (GPIPS): Data Release 4. , keywords =. doi:10.3847/1538-4365/ab9f30 , archivePrefix =. 2006.15203 , primaryClass =

    2006 doi

  60. [68]

    , keywords =

    An iterative reconstruction algorithm for Faraday tomography. , keywords =. doi:10.1093/mnras/staa3580 , archivePrefix =. 2011.10840 , primaryClass =

    2011 doi

  61. [69]

    , keywords =

    The local interstellar medium. , keywords =. doi:10.1146/annurev.aa.25.090187.001511 , adsurl =

    doi

  62. [70]

    , year = 2012, month = sep, volume =

    Magnetic Fields in Molecular Clouds. , year = 2012, month = sep, volume =. doi:10.1146/annurev-astro-081811-125514 , adsurl =

    2012 doi

  63. [71]

    , keywords =

    Magnetic Fields in Interstellar Clouds from Zeeman Observations: Inference of Total Field Strengths by Bayesian Analysis. , keywords =. doi:10.1088/0004-637X/725/1/466 , adsurl =

    doi

  64. [72]

    Turbulence and Magnetic Fields in Astrophysics , year = 2003, editor =

    Observations of Interstellar Magnetic Fields. Turbulence and Magnetic Fields in Astrophysics , year = 2003, editor =

    2003

  65. [73]

    , keywords =

    Magnetic Misalignment of Interstellar Dust Filaments. , keywords =. doi:10.3847/1538-4357/acb0c4 , archivePrefix =. 2208.07382 , primaryClass =

    doi

  66. [74]

    , keywords =

    Determining the Magnetic Field in the Galactic Plane from New Arecibo Pulsar Faraday Rotation Measurements. , keywords =. doi:10.3847/1538-4357/ad7b15 , archivePrefix =. 2410.07967 , primaryClass =

    doi

  67. [75]

    The Strength of Interstellar Magnetic Fields , author =. Phys. Rev. , volume =. 1951 , month =

    1951

  68. [76]

    , year = 1951, month = sep, volume =

    The Polarization of Starlight by Aligned Dust Grains. , year = 1951, month = sep, volume =. doi:10.1086/145464 , adsurl =

    1951 doi

  69. [77]

    , keywords =

    Probing the magneto-ionic medium of the Milky Way using pulsars. , keywords =. doi:10.1093/mnras/staf1816 , archivePrefix =. 2510.12991 , primaryClass =

    doi

  70. [78]

    , keywords =

    Structure in the Magnetic Field of the Milky Way Disk and Halo Traced by Faraday Rotation. , keywords =. doi:10.3847/1538-4357/ac94ce , archivePrefix =. 2209.10819 , primaryClass =

    doi

  71. [79]

    , keywords =

    The Galactic Magneto-ionic Medium Survey: Moments of the Faraday Spectra. , keywords =. doi:10.3847/1538-4357/aaf85f , archivePrefix =. 1812.05399 , primaryClass =

    doi arXiv

  72. [80]

    , keywords =

    A Faraday rotation template for the Galactic sky. , keywords =. doi:10.1111/j.1365-2966.2005.09331.x , archivePrefix =. astro-ph/0410636 , primaryClass =

    2005 doi

  73. [81]

    , keywords =

    Magnetic field evolution and reversals in spiral galaxies. , keywords =. doi:10.1093/mnras/stw1625 , archivePrefix =. 1607.05532 , primaryClass =

    doi arXiv

  74. [82]

    , journal=

    Donoho, D.L. , journal=. Compressed sensing , year=

  75. [83]

    , keywords =

    Tomographic Imaging of the Sagittarius Spiral Arm's Magnetic Field Structure. , keywords =. doi:10.3847/1538-4357/ad0fe2 , archivePrefix =. 2311.13054 , primaryClass =

    doi

  76. [84]

    , keywords =

    Two-component Magnetic Field along the Line of Sight to the Perseus Molecular Cloud: Contribution of the Foreground Taurus Molecular Cloud. , keywords =. doi:10.3847/1538-4357/abfcc5 , archivePrefix =. 2104.11932 , primaryClass =

    doi

  77. [85]

    , keywords =

    A parsec-scale Galactic 3D dust map out to 1.25 kpc from the Sun. , keywords =. doi:10.1051/0004-6361/202347628 , archivePrefix =. 2308.01295 , primaryClass =

    doi

  78. [86]

    Faraday tomography of LoTSS-DR2 data. II. Multi-tracer analysis in the high-latitude outer Galaxy. , keywords =. doi:10.1051/0004-6361/202348586 , archivePrefix =. 2404.19068 , primaryClass =

    doi

  79. [87]

    Faraday tomography of LoTSS-DR2 data. III. Revealing the Local Bubble and the complex of local interstellar clouds in the high-latitude inner Galaxy. , keywords =. doi:10.1051/0004-6361/202450082 , archivePrefix =. 2406.14679 , primaryClass =

    doi

  80. [88]

    Faraday tomography of LoTSS-DR2 data. I. Faraday moments in the high-latitude outer Galaxy and revealing Loop III in polarisation. , keywords =. doi:10.1051/0004-6361/202142244 , archivePrefix =. 2203.01351 , primaryClass =

    doi

  81. [89]

    , keywords =

    Velocity Centroids as Tracers of the Turbulent Velocity Statistics. , keywords =. doi:10.1086/432458 , archivePrefix =. astro-ph/0401603 , primaryClass =

    doi arXiv

  82. [90]

    , keywords =

    Studies of Regular and Random Magnetic Fields in the ISM: Statistics of Polarization Vectors and the Chandrasekhar-Fermi Technique. , keywords =. doi:10.1086/587479 , archivePrefix =. 0801.0279 , primaryClass =

    doi arXiv

  83. [91]

    , keywords =

    Intermittency of interstellar turbulence: extreme velocity-shears and CO emission on milliparsec scale. , keywords =. doi:10.1051/0004-6361/200810963 , archivePrefix =. 0910.1766 , primaryClass =

    doi arXiv

  84. [92]

    , keywords =

    CN Zeeman measurements in star formation regions. , keywords =. doi:10.1051/0004-6361:200809577 , adsurl =

    doi

  85. [93]

    Nature Astronomy , keywords =

    A three-dimensional map of the hot Local Bubble using diffuse interstellar bands. Nature Astronomy , keywords =. doi:10.1038/s41550-019-0814-z , archivePrefix =. 1907.07429 , primaryClass =

    1907 doi arXiv

  86. [94]

    , keywords =

    Integrated Polarization of Sources at -0.5ex 1 m and New Rotation Measure Ambiguities. , keywords =. doi:10.1088/0004-6256/141/6/191 , archivePrefix =. 1103.4149 , primaryClass =

    doi arXiv

  87. [95]

    , keywords =

    Deflections of UHECRs in the Galactic magnetic field. , keywords =. doi:10.1088/1475-7516/2019/05/004 , archivePrefix =. 1711.02730 , primaryClass =

    2019 doi arXiv

  88. [96]

    , keywords =

    Joint 3D modelling of the polarized Galactic synchrotron and thermal dust foreground diffuse emission. , keywords =. doi:10.1051/0004-6361/201014492 , archivePrefix =. 1003.4450 , primaryClass =

    doi arXiv

  89. [97]

    Physical Review , year = 1949, month = apr, volume =

    On the Origin of the Cosmic Radiation. Physical Review , year = 1949, month = apr, volume =. doi:10.1103/PhysRev.75.1169 , adsurl =

    1949 doi

  90. [98]

    , keywords =

    A three-dimensional reconstruction of the interstellar magnetic field toward a star-forming region. , keywords =. doi:10.1051/0004-6361/202451034 , archivePrefix =. 2510.25879 , primaryClass =

    doi

  91. [99]

    Plasma Physics and Controlled Fusion , keywords =

    Plasma turbulence in the interstellar medium. Plasma Physics and Controlled Fusion , keywords =. doi:10.1088/1361-6587/ab49eb , archivePrefix =. 1912.08237 , primaryClass =

    1912 doi

  92. [100]

    Highlights of Astronomy , keywords =

    Theoretical understanding of Galactic magnetic fields. Highlights of Astronomy , keywords =. doi:10.1017/S174392131401165X , adsurl =

    doi

  93. [101]

    The Galactic Center: a Window to the Nuclear Environment of Disk Galaxies , year = 2011, editor =

    Magnetic Fields in the Galactic Center. The Galactic Center: a Window to the Nuclear Environment of Disk Galaxies , year = 2011, editor =

    2011

  94. [102]

    Reviews of Modern Physics , keywords =

    The interstellar environment of our galaxy. Reviews of Modern Physics , keywords =. doi:10.1103/RevModPhys.73.1031 , archivePrefix =. astro-ph/0106359 , primaryClass =

    doi arXiv

  95. [103]

    , keywords =

    Numerical models of the galactic dynamo driven by supernovae and superbubbles. , keywords =

  96. [104]

    , keywords =

    Analytical models of X-shape magnetic fields in galactic halos. , keywords =. doi:10.1051/0004-6361/201322966 , archivePrefix =. 1312.1974 , primaryClass =

    1974 doi arXiv

  97. [105]

    , keywords =

    Expansion of a Superbubble in a Uniform Magnetic Field. , keywords =. doi:10.1086/170185 , adsurl =

    doi

  98. [106]

    , year = 1968, month = dec, volume =

    The Distribution of Interstellar Reddening Material. , year = 1968, month = dec, volume =. doi:10.1086/110757 , adsurl =

    1968 doi

  99. [107]

    The Dynamic Interstellar Medium: A Celebration of the Canadian Galactic Plane Survey , year = 2010, editor =

    Magnetic Fields in Nearby Galaxies. The Dynamic Interstellar Medium: A Celebration of the Canadian Galactic Plane Survey , year = 2010, editor =. doi:10.48550/arXiv.1104.2427 , archivePrefix =. 1104.2427 , primaryClass =

    2010 doi arXiv

  100. [108]

    , keywords =

    Hydrostatic equilibrium in a magnetized, warped Galactic disc. , keywords =. doi:10.1046/j.1365-8711.2001.04418.x , archivePrefix =. astro-ph/0101387 , primaryClass =

    2001 doi

  101. [109]

    , keywords =

    Statistical Properties of Galactic Starlight Polarization. , keywords =. doi:10.1086/324297 , archivePrefix =. astro-ph/0105023 , primaryClass =

    doi arXiv

  102. [110]

    , keywords =

    Magnetic Turbulence Spectra and Intermittency in the Heliosheath and in the Local Interstellar Medium. , keywords =. doi:10.3847/1538-4357/aafd30 , archivePrefix =. 1906.06927 , primaryClass =

    1906 doi arXiv

  103. [111]

    , keywords =

    Faraday rotation measure synthesis for magnetic fields of galaxies. , keywords =. doi:10.1111/j.1365-2966.2011.18571.x , archivePrefix =. 1102.4316 , primaryClass =

    2011 doi

  104. [112]

    , keywords =

    Wavelet-based Faraday rotation measure synthesis. , keywords =. doi:10.1111/j.1745-3933.2009.00778.x , archivePrefix =. 0911.0261 , primaryClass =

    2009 doi

  105. [113]

    , keywords =

    Charting the Interstellar Magnetic Field causing the Interstellar Boundary Explorer (IBEX) Ribbon of Energetic Neutral Atoms. , keywords =. doi:10.1088/0004-637X/814/2/112 , archivePrefix =. 1510.04679 , primaryClass =

    doi arXiv

  106. [114]

    The Interstellar Magnetic Field Close to the Sun. II. , keywords =. doi:10.1088/0004-637X/760/2/106 , archivePrefix =. 1206.1273 , primaryClass =

    doi arXiv

  107. [115]

    , keywords =

    The Local Bubble and Interstellar Material Near the Sun. , keywords =. doi:10.1007/s11214-007-9209-z , archivePrefix =. astro-ph/0702596 , primaryClass =

    doi arXiv

  108. [116]

    arXiv e-prints , keywords =

    The Polarisation Sky Survey of the Universe's Magnetism (POSSUM): Science Goals and Survey Description. arXiv e-prints , keywords =

  109. [117]

    , keywords =

    Low-Mach-number turbulence in interstellar gas revealed by radio polarization gradients. , keywords =. doi:10.1038/nature10446 , archivePrefix =. 1110.2896 , primaryClass =

    doi arXiv

  110. [118]

    , keywords =

    Radio Polarization from the Inner Galaxy at Arcminute Resolution. , keywords =. doi:10.1086/319468 , archivePrefix =. astro-ph/0010518 , primaryClass =

    doi arXiv

  111. [119]

    Summary of the content and survey properties

    Gaia Data Release 3. Summary of the content and survey properties. , keywords =. doi:10.1051/0004-6361/202243940 , archivePrefix =. 2208.00211 , primaryClass =

    doi

  112. [120]

    , keywords =

    The Gaia mission. , keywords =. doi:10.1051/0004-6361/201629272 , archivePrefix =. 1609.04153 , primaryClass =

    doi arXiv

  113. [121]

    Science , keywords =

    Magnetic Fields in the Formation of Sun-Like Stars. Science , keywords =. doi:10.1126/science.1129093 , archivePrefix =. astro-ph/0609177 , primaryClass =

    doi arXiv

  114. [122]

    , keywords =

    Detection of Polarized CO Emission from the Molecular Outflow in NGC 1333 IRAS 4A. , keywords =. doi:10.1086/312345 , adsurl =

    doi

  115. [123]

    , keywords =

    Linear polarization of radio frequency lines in molecular clouds and circumstellar envelopes. , keywords =. doi:10.1086/159663 , adsurl =

    doi

  116. [124]

    , keywords =

    On mapping the magnetic field direction in molecular clouds by polarization measurements. , keywords =. doi:10.1086/183446 , adsurl =

    doi

  117. [125]

    Toward a Theory of Interstellar Turbulence. II. Strong Alfvenic Turbulence. , keywords =. doi:10.1086/175121 , adsurl =

    doi

  118. [126]

    , keywords =

    Three-dimensional Magnetohydrodynamic Modeling of the Gaseous Structure of the Galaxy: Setup and Initial Results. , keywords =. doi:10.1086/343129 , archivePrefix =. astro-ph/0207634 , primaryClass =

    doi arXiv

  119. [127]

    , keywords =

    Interstellar polarization and extinction in the Local Bubble and the Gould Belt. , keywords =. doi:10.1093/mnras/sty2978 , archivePrefix =. 1811.01411 , primaryClass =

    doi

  120. [128]

    , keywords =

    Velocity Gradients as a Tracer for Magnetic Fields. , keywords =. doi:10.3847/1538-4357/835/1/41 , archivePrefix =. 1608.06867 , primaryClass =

    doi arXiv

  121. [129]

    , keywords =

    A 3D Dust Map Based on Gaia, Pan-STARRS 1, and 2MASS. , keywords =. doi:10.3847/1538-4357/ab5362 , archivePrefix =. 1905.02734 , primaryClass =

    1905 doi arXiv

  122. [130]

    arXiv e-prints , keywords =

    Direction-Dependent Faraday Synthesis. arXiv e-prints , keywords =. doi:10.48550/arXiv.2504.00141 , archivePrefix =. 2504.00141 , primaryClass =

    doi

  123. [131]

    , keywords =

    Redshift estimates for fast radio bursts and implications on intergalactic magnetic fields. , keywords =. doi:10.1093/mnras/staa2572 , archivePrefix =. 2008.10536 , primaryClass =

    2008 doi

  124. [132]

    , keywords =

    Filamentary Dust Polarization and the Morphology of Neutral Hydrogen Structures. , keywords =. doi:10.3847/1538-4357/ad06aa , archivePrefix =. 2306.10107 , primaryClass =

    doi

  125. [133]

    , keywords =

    Imprints of the Local Bubble and Dust Complexity on Polarized Dust Emission. , keywords =. doi:10.3847/1538-4357/ad61e0 , archivePrefix =. 2404.11009 , primaryClass =

    doi

  126. [134]

    , year = 1908, month = dec, volume =

    The Zeeman Effect in the Sun. , year = 1908, month = dec, volume =. doi:10.1086/121847 , adsurl =

    1908 doi

  127. [135]

    Science , year = 1949, month = feb, volume =

    Observations of the Polarized Light from Stars. Science , year = 1949, month = feb, volume =. doi:10.1126/science.109.2825.166 , adsurl =

    1949 doi

  128. [136]

    , keywords =

    Pulsar Rotation Measures and Large-scale Magnetic Field Reversals in the Galactic Disk. , keywords =. doi:10.3847/1538-4365/aa9c45 , archivePrefix =. 1712.01997 , primaryClass =

    doi arXiv

  129. [137]

    , keywords =

    Observing Interstellar and Intergalactic Magnetic Fields. , keywords =. doi:10.1146/annurev-astro-091916-055221 , adsurl =

    doi

  130. [138]

    , keywords =

    Pulsar Rotation Measures and the Large-Scale Structure of the Galactic Magnetic Field. , keywords =. doi:10.1086/501444 , archivePrefix =. astro-ph/0601357 , primaryClass =

    doi arXiv

  131. [139]

    , keywords =

    Antisymmetric rotation measures in our Galaxy: evidence for an A0 dynamo. , keywords =

  132. [140]

    , keywords =

    The magnetic field in the disk of our Galaxy. , keywords =

  133. [141]

    , keywords =

    Cosmic Rays Can Drive Strong Outflows from Gas-rich High-redshift Disk Galaxies. , keywords =. doi:10.1088/2041-8205/777/2/L38 , archivePrefix =. 1310.3273 , primaryClass =

    doi arXiv

  134. [142]

    , keywords =

    Magnetic Fields in Large-diameter H II Regions Revealed by the Faraday Rotation of Compact Extragalactic Radio Sources. , keywords =. doi:10.1088/0004-637X/736/2/83 , archivePrefix =. 1106.0931 , primaryClass =

    doi arXiv

  135. [143]

    Magnetic Fields in Diffuse Media , year = 2015, editor =

    Magnetic Fields in the Milky Way. Magnetic Fields in Diffuse Media , year = 2015, editor =. doi:10.1007/978-3-662-44625-6_17 , archivePrefix =. 1406.0283 , primaryClass =

    2015 doi arXiv

  136. [144]

    , keywords =

    The Outer Scale of Turbulence in the Magnetoionized Galactic Interstellar Medium. , keywords =. doi:10.1086/587165 , archivePrefix =. 0802.2740 , primaryClass =

    doi arXiv

  137. [145]

    , keywords =

    Enhanced Small-Scale Faraday Rotation in the Galactic Spiral Arms. , keywords =. doi:10.1086/500543 , archivePrefix =. astro-ph/0512456 , primaryClass =

    doi arXiv

  138. [146]

    , keywords =

    Magnetic Fields and Ionized Gas in the Inner Galaxy: An Outer Scale for Turbulence and the Possible Role of H II Regions. , keywords =. doi:10.1086/421341 , archivePrefix =. astro-ph/0403655 , primaryClass =

    doi arXiv

  139. [147]

    Galaxies , keywords =

    Magnetism Science with the Square Kilometre Array. Galaxies , keywords =. doi:10.3390/galaxies8030053 , archivePrefix =. 2006.03172 , primaryClass =

    2006 doi

  140. [148]

    Cosmic Magnetic Fields: From Planets, to Stars and Galaxies , year = 2009, editor =

    The Faraday rotation measure synthesis technique. Cosmic Magnetic Fields: From Planets, to Stars and Galaxies , year = 2009, editor =. doi:10.1017/S1743921309031421 , adsurl =

    2009 doi

  141. [149]

    The Local Bubble and Beyond: Lyman-Spitzer-Colloquium (Proc IAU Colloq 166) , year = 1998, editor =

    The Magnetic Field Near the Local Bubble. The Local Bubble and Beyond: Lyman-Spitzer-Colloquium (Proc IAU Colloq 166) , year = 1998, editor =. doi:doi.org/10.1007/BFb0104725 , adsurl =

    1998 doi

  142. [150]

    , keywords =

    The Local Direction and Curvature of the Galactic Magnetic Field Derived from Starlight Polarization. , keywords =. doi:10.1086/177153 , adsurl =

    doi

  143. [151]

    , keywords =

    Magnetic Fields in the Multiphase Interstellar Medium. , keywords =. doi:10.1007/s11214-012-9866-4 , adsurl =

    doi

  144. [152]

    , keywords =

    Magnetic Field Diagnostics Based on Far-Infrared Polarimetry: Tests Using Numerical Simulations. , keywords =. doi:10.1086/323489 , archivePrefix =. astro-ph/0103286 , primaryClass =

    doi arXiv

  145. [153]

    The role of magnetic field in molecular cloud formation and evolution. Front. Astron. Space Sci. , keywords =. doi:10.3389/fspas.2019.00005 , archivePrefix =. 1902.00798 , primaryClass =

    2019 doi

  146. [154]

    , keywords =

    Galactic magnetic X fields. , keywords =. doi:10.1051/0004-6361/202142330 , archivePrefix =. 2112.09023 , primaryClass =

    doi

  147. [155]

    Dispersion of Magnetic Fields in Molecular Clouds. I. , keywords =. doi:10.1088/0004-637X/696/1/567 , archivePrefix =. 0811.0813 , primaryClass =

    doi arXiv

  148. [156]

    Galaxies , keywords =

    Is There a Polarization Horizon?. Galaxies , keywords =. doi:10.3390/galaxies6040129 , archivePrefix =. 1810.12008 , primaryClass =

    doi arXiv

  149. [157]

    Science , year = 1949, month = feb, volume =

    Polarization of Light from Distant Stars by Interstellar Medium. Science , year = 1949, month = feb, volume =. doi:10.1126/science.109.2825.165 , adsurl =

    1949 doi

  150. [158]

    , keywords =

    Tracing of magnetic fields with gradients: subsonic turbulence. , keywords =. doi:10.1093/mnras/stad186 , archivePrefix =. 2301.13458 , primaryClass =

    doi

  151. [159]

    , keywords =

    A Comparison between Faraday Tomography and Synchrotron Polarization Gradients. , keywords =. doi:10.3847/1538-4357/ab578c , archivePrefix =. 1901.07731 , primaryClass =

    1901 doi

  152. [160]

    , keywords =

    Magnetohydrodynamic Effects of a First-Order Cosmological Phase Transition. , keywords =. doi:10.1103/PhysRevLett.51.1488 , adsurl =

    doi

  153. [161]

    Supernova-regulated ISM. V. Space and Time Correlations. , keywords =. doi:10.3847/1538-4357/aa93e7 , archivePrefix =. 1703.05187 , primaryClass =

    doi arXiv

  154. [162]

    , keywords =

    The observed spiral structure of the Milky Way. , keywords =. doi:10.1051/0004-6361/201424039 , archivePrefix =. 1407.7331 , primaryClass =

    doi arXiv

  155. [163]

    Dispersion of Magnetic Fields in Molecular Clouds. IV. Analysis of Interferometry Data. , keywords =. doi:10.3847/0004-637X/820/1/38 , archivePrefix =. 1602.01873 , primaryClass =

    doi arXiv

  156. [164]

    Dispersion of Magnetic Fields in Molecular Clouds. II. , keywords =. doi:10.1088/0004-637X/706/2/1504 , archivePrefix =. 0909.5227 , primaryClass =

    doi arXiv

  157. [165]

    , keywords =

    Probing the Magnetic Field with Molecular Ion Spectra. , keywords =. doi:10.1086/308980 , archivePrefix =. astro-ph/0311335 , primaryClass =

    doi arXiv

  158. [166]

    , year = 1974, month = jun, volume =

    Aperture Synthesis with a Non-Regular Distribution of Interferometer Baselines. , year = 1974, month = jun, volume =

    1974

  159. [167]

    , keywords =

    Intensity Gradients Technique: Synergy with Velocity Gradients and Polarization Studies. , keywords =. doi:10.3847/1538-4357/ab4b5e , archivePrefix =. 1908.09488 , primaryClass =

    1908 doi

  160. [168]

    , keywords =

    The Galactic Faraday rotation sky 2020. , keywords =. doi:10.1051/0004-6361/202140486 , archivePrefix =. 2102.01709 , primaryClass =

    2020 doi

  161. [169]

    , keywords =

    The Galactic Faraday depth sky revisited. , keywords =. doi:10.1051/0004-6361/201935479 , archivePrefix =. 1903.06735 , primaryClass =

    1903 doi

  162. [170]

    , keywords =

    Galactic interstellar turbulence across the southern sky seen through spatial gradients of the polarization vector. , keywords =. doi:10.1051/0004-6361/201322982 , archivePrefix =. 1404.6077 , primaryClass =

    doi arXiv

  163. [171]

    First LOFAR Galactic foreground detection

    Studying Galactic interstellar turbulence through fluctuations in synchrotron emission. First LOFAR Galactic foreground detection. , keywords =. doi:10.1051/0004-6361/201322013 , archivePrefix =. 1308.2804 , primaryClass =

    doi arXiv

  164. [172]

    , keywords =

    Fisher analysis on wide-band polarimetry for probing the intergalactic magnetic field. , keywords =. doi:10.1093/pasj/pst007 , archivePrefix =. 1308.5696 , primaryClass =

    doi arXiv

  165. [173]

    Galaxies , year = 2018, month = dec, volume =

    Faraday Tomography Tutorial. Galaxies , year = 2018, month = dec, volume =. doi:10.3390/galaxies6040140 , adsurl =

    2018 doi

  166. [174]

    Galaxies , keywords =

    Practical Modeling of Large-Scale Galactic Magnetic Fields: Status and Prospects. Galaxies , keywords =. doi:10.3390/galaxies7020052 , archivePrefix =. 1904.12689 , primaryClass =

    1904 doi arXiv

  167. [175]

    , keywords =

    Comparing polarized synchrotron and thermal dust emission in the Galactic plane. , keywords =. doi:10.1093/mnras/stt200 , archivePrefix =. 1302.0143 , primaryClass =

    doi arXiv

  168. [176]

    , keywords =

    Modelling the Galactic magnetic field on the plane in two dimensions. , keywords =. doi:10.1111/j.1365-2966.2009.15745.x , archivePrefix =. 0907.3994 , primaryClass =

    2009 doi

  169. [177]

    , keywords =

    A New Model of the Galactic Magnetic Field. , keywords =. doi:10.1088/0004-637X/757/1/14 , archivePrefix =. 1204.3662 , primaryClass =

    doi arXiv

  170. [178]

    , keywords =

    Linear polarization structures in LOFAR observations of the interstellar medium in the 3C 196 field. , keywords =. doi:10.1051/0004-6361/201526638 , archivePrefix =. 1508.06650 , primaryClass =

    doi arXiv

  171. [179]

    , keywords =

    Magnetically aligned straight depolarization canals and the rolling Hough transform. , keywords =. doi:10.1051/0004-6361/201833291 , archivePrefix =. 1806.06634 , primaryClass =

    doi arXiv

  172. [180]

    , keywords =

    Bayesian Revisit of the Relationship between the Total Field Strength and the Volume Density of Interstellar Clouds. , keywords =. doi:10.3847/1538-4357/ab672b , adsurl =

    doi

  173. [181]

    arXiv e-prints , keywords =

    Faraday Rotation Measures through the Cores of Southern Galaxy Clusters. arXiv e-prints , keywords =. doi:10.48550/arXiv.astro-ph/0411045 , archivePrefix =. astro-ph/0411045 , primaryClass =

    doi arXiv

  174. [182]

    Polarimetry of the Interstellar Medium , year = 1996, editor =

    Observational Constraints on Grain Alignment Mechanisms. Polarimetry of the Interstellar Medium , year = 1996, editor =

    1996

  175. [183]

    , keywords =

    Detection of a Coherent Magnetic Field in the Magellanic Bridge through Faraday Rotation. , keywords =. doi:10.1093/mnras/stx206 , archivePrefix =. 1701.05962 , primaryClass =

    doi arXiv

  176. [184]

    , keywords =

    Aspect ratios of far-infrared and H I filaments in the diffuse interstellar medium at high Galactic latitudes. , keywords =. doi:10.1051/0004-6361/202245200 , archivePrefix =. 2303.16183 , primaryClass =

    doi

  177. [185]

    Steep power spectra associated with cold gas

    H I anisotropies associated with radio-polarimetric filaments . Steep power spectra associated with cold gas. , keywords =. doi:10.1051/0004-6361/201629627 , archivePrefix =. 1707.05672 , primaryClass =

    doi arXiv

  178. [186]

    , keywords =

    Anisotropies in the HI gas distribution toward 3C 196. , keywords =. doi:10.1051/0004-6361/201629113 , archivePrefix =. 1608.05369 , primaryClass =

    doi arXiv

  179. [187]

    , keywords =

    Study of velocity centroids based on the theory of fluctuations in position-position-velocity space. , keywords =. doi:10.1093/mnras/stw2512 , archivePrefix =. 1607.04316 , primaryClass =

    doi arXiv

  180. [188]

    , keywords =

    Primordial magnetogenesis. , keywords =. doi:10.1016/j.physrep.2011.03.001 , archivePrefix =. 1007.3891 , primaryClass =

    2011 doi arXiv

  181. [189]

    Soviet Journal of Experimental and Theoretical Physics , year = 1968, month = may, volume =

    Enhancement of a Magnetic Field by a Conducting Fluid. Soviet Journal of Experimental and Theoretical Physics , year = 1968, month = may, volume =

    1968

  182. [190]

    , keywords =

    The Size Distribution of Interstellar Dust Particles as Determined from Polarization: Spheroids. , keywords =. doi:10.1086/175604 , adsurl =

    doi

  183. [191]

    , keywords =

    Formation and Fragmentation of Gaseous Spurs in Spiral Galaxies. , keywords =. doi:10.1086/339352 , archivePrefix =. astro-ph/0111398 , primaryClass =

    doi arXiv

  184. [192]

    , keywords =

    Magnetic Field Strength Maps for Molecular Clouds: A New Method Based on a Polarization-Intensity Gradient Relation. , keywords =. doi:10.1088/0004-637X/747/1/79 , archivePrefix =. 1201.4263 , primaryClass =

    doi arXiv

  185. [193]

    Akademiia Nauk SSSR Doklady , year = 1941, month = jan, volume =

    The Local Structure of Turbulence in Incompressible Viscous Fluid for Very Large Reynolds' Numbers. Akademiia Nauk SSSR Doklady , year = 1941, month = jan, volume =

    1941

  186. [194]

    , keywords =

    The coherent magnetic field of the Milky Way halo, the Local Bubble, and the Fan region. , keywords =. doi:10.1051/0004-6361/202451440 , archivePrefix =. 2407.02148 , primaryClass =

    doi

  187. [195]

    , keywords =

    Density Fluctuations in MHD Turbulence: Spectra, Intermittency, and Topology. , keywords =. doi:10.1086/511515 , archivePrefix =. astro-ph/0608051 , primaryClass =

    doi arXiv

  188. [196]

    The Role of Magnetic Fields in Setting the Star Formation Rate and the Initial Mass Function. Front. Astron. Space Sci. , keywords =. doi:10.3389/fspas.2019.00007 , archivePrefix =. 1902.02557 , primaryClass =

    2019 doi

  189. [197]

    , keywords =

    Nonlinear Hydromagnetic Wave Support of a Stratified Molecular Cloud. , keywords =. doi:10.1086/377495 , archivePrefix =. astro-ph/0306473 , primaryClass =

    doi arXiv

  190. [198]

    , year = 1969, month = may, volume =

    The Effect of Wave-Particle Interactions on the Propagation of Cosmic Rays. , year = 1969, month = may, volume =. doi:10.1086/149981 , adsurl =

    1969 doi

  191. [199]

    Jansky Very Large Array Sky Survey (VLASS)

    The Karl G. Jansky Very Large Array Sky Survey (VLASS). Science Case and Survey Design. , keywords =. doi:10.1088/1538-3873/ab63eb , archivePrefix =. 1907.01981 , primaryClass =

    1907 doi

  192. [200]

    , keywords =

    Gaia-2MASS 3D maps of Galactic interstellar dust within 3 kpc. , keywords =. doi:10.1051/0004-6361/201834695 , archivePrefix =. 1902.04116 , primaryClass =

    1902 doi arXiv

  193. [201]

    , keywords =

    3D mapping of the dense interstellar gas around the Local Bubble. , keywords =. doi:10.1051/0004-6361:20031214 , adsurl =

    doi

  194. [202]

    Large-Scale Magnetic Fields in the Universe

    The Role of Magnetic Fields in the Interstellar Medium of the Milky Way. Large-Scale Magnetic Fields in the Universe. Series: Space Sciences Series of ISSI , year = 2013, editor =. doi:10.1007/978-1-4614-5728-2_10 , adsurl =

    2013 doi

  195. [203]

    Evidence from the Diffuse Polarized Radio Emission

    The Role of Magnetic Fields in the Interstellar Medium of the Milky Way. Evidence from the Diffuse Polarized Radio Emission. , keywords =. doi:10.1007/s11214-011-9796-6 , adsurl =

    doi

  196. [204]

    , keywords =

    Reconnection Diffusion in Turbulent Fluids and Its Implications for Star Formation. , keywords =. doi:10.1007/s11214-013-0031-5 , adsurl =

    doi

  197. [205]

    , keywords =

    Statistical Description of Synchrotron Intensity Fluctuations: Studies of Astrophysical Magnetic Turbulence. , keywords =. doi:10.1088/0004-637X/747/1/5 , archivePrefix =. 1105.4617 , primaryClass =

    doi arXiv

  198. [206]

    , keywords =

    Magnetic Reconnection and Turbulent Mixing: From ISM to Clusters of Galaxies. , keywords =. doi:10.1023/B:ASTR.0000014959.27744.9b , archivePrefix =. astro-ph/0302104 , primaryClass =

    doi

  199. [207]

    Magnetic Field Strength from Turbulence Theory. I. Using Differential Measure Approach. , keywords =. doi:10.3847/1538-4357/ac6877 , archivePrefix =. 2204.09731 , primaryClass =

    doi

  200. [208]

    , keywords =

    Gradients of Synchrotron Polarization: Tracing 3D Distribution of Magnetic Fields. , keywords =. doi:10.3847/1538-4357/aad3ca , archivePrefix =. 1802.00028 , primaryClass =

    doi arXiv

  201. [209]

    , keywords =

    Tracing Magnetic Fields with Spectroscopic Channel Maps. , keywords =. doi:10.3847/1538-4357/aaa241 , archivePrefix =. 1703.03119 , primaryClass =

    doi arXiv

  202. [210]

    , keywords =

    Distribution of Velocity Gradient Orientations: Mapping Magnetization with the Velocity Gradient Technique. , keywords =. doi:10.3847/1538-4357/aad7ff , archivePrefix =. 1802.02984 , primaryClass =

    doi arXiv

  203. [211]

    , keywords =

    Synchrotron Intensity Gradients as Tracers of Interstellar Magnetic Fields. , keywords =. doi:10.3847/1538-4357/aa74c6 , adsurl =

    doi

  204. [212]

    , keywords =

    Tracing magnetic fields with aligned grains. , keywords =. doi:10.1016/j.jqsrt.2007.01.038 , archivePrefix =. 0707.0858 , primaryClass =

    2007 doi arXiv

  205. [213]

    , keywords =

    Radiative torques: analytical model and basic properties. , keywords =. doi:10.1111/j.1365-2966.2007.11817.x , archivePrefix =. 0707.0886 , primaryClass =

    2007 doi

  206. [214]

    , keywords =

    A New Constraint on the Relative Disorder of Magnetic Fields between Neutral Interstellar Medium Phases. , keywords =. doi:10.3847/1538-4357/ad5ade , archivePrefix =. 2312.03846 , primaryClass =

    doi

  207. [215]

    , keywords =

    Charting nearby dust clouds using Gaia data only. , keywords =. doi:10.1051/0004-6361/201935093 , archivePrefix =. 1901.05971 , primaryClass =

    1901 doi

  208. [216]

    Analysis of polarimetric data in the light of HIPPARCOS parallaxes

    Interstellar dust and magnetic field at the boundaries of the Local Bubble. Analysis of polarimetric data in the light of HIPPARCOS parallaxes. , keywords =

  209. [217]

    Galaxies , keywords =

    Magnetic Fields in Molecular Clouds Observation and Interpretation. Galaxies , keywords =. doi:10.3390/galaxies9020041 , archivePrefix =. 2106.08172 , primaryClass =

    doi

  210. [218]

    , keywords =

    Mapping the magnetic field in the Taurus/B211 filamentary cloud with SOFIA HAWC + and comparing with simulation. , keywords =. doi:10.1093/mnras/stab3448 , archivePrefix =. 2111.12864 , primaryClass =

    doi

  211. [219]

    The application of compressive sampling to radio astronomy. II. Faraday rotation measure synthesis. , keywords =. doi:10.1051/0004-6361/201015890 , archivePrefix =. 1106.1709 , primaryClass =

    doi arXiv

  212. [220]

    , keywords =

    Probing the Turbulence Dissipation Range and Magnetic Field Strengths in Molecular Clouds. , keywords =. doi:10.1086/529581 , archivePrefix =. 0801.2757 , primaryClass =

    doi arXiv

  213. [221]

    , keywords =

    Heightened Faraday complexity in the inner 1 kpc of the galactic centre. , keywords =. doi:10.1093/mnras/stab253 , archivePrefix =. 2102.01139 , primaryClass =

    doi

  214. [222]

    , keywords =

    Calibrating the Davis-Chandrasekhar-Fermi Method with Numerical Simulations: Uncertainties in Estimating the Magnetic Field Strength from Statistics of Field Orientations. , keywords =. doi:10.3847/1538-4357/ac0cec , archivePrefix =. 2106.09934 , primaryClass =

    doi

  215. [223]

    Science , keywords =

    A Bright Millisecond Radio Burst of Extragalactic Origin. Science , keywords =. doi:10.1126/science.1147532 , archivePrefix =. 0709.4301 , primaryClass =

    doi arXiv

  216. [224]

    , keywords =

    The complex large-scale magnetic fields in the first Galactic quadrant as revealed by the Faraday depth profile disparity. , keywords =. doi:10.1093/mnras/staa2105 , archivePrefix =. 2007.07893 , primaryClass =

    2007 doi

  217. [225]

    , keywords =

    Turbulence in the Interstellar Medium. , keywords =. doi:10.1023/B:ASTR.0000014961.72318.7c , adsurl =

    doi

  218. [226]

    Reviews of Modern Physics , keywords =

    Control of star formation by supersonic turbulence. Reviews of Modern Physics , keywords =. doi:10.1103/RevModPhys.76.125 , archivePrefix =. astro-ph/0301093 , primaryClass =

    doi arXiv

  219. [227]

    , keywords =

    Modelling Local Bubble analogs: synthetic dust polarization maps. , keywords =. doi:10.1093/mnras/stad1854 , archivePrefix =. 2212.06598 , primaryClass =

    doi

  220. [228]

    Astronomical Polarimetry: Current Status and Future Directions , year = 2005, editor =

    A Southern Optical/Infrared Survey of Interstellar Polarization. Astronomical Polarimetry: Current Status and Future Directions , year = 2005, editor =

    2005

  221. [229]

    , keywords =

    The Australia Telescope National Facility Pulsar Catalogue. , keywords =. doi:10.1086/428488 , archivePrefix =. astro-ph/0412641 , primaryClass =

    doi arXiv

  222. [230]

    , keywords =

    New Constraints on the Galactic Halo Magnetic Field Using Rotation Measures of Extragalactic Sources toward the Outer Galaxy. , keywords =. doi:10.1088/0004-637X/755/1/21 , archivePrefix =. 1206.3314 , primaryClass =

    doi arXiv

  223. [231]

    , keywords =

    A Survey of Extragalactic Faraday Rotation at High Galactic Latitude: The Vertical Magnetic Field of the Milky Way Toward the Galactic Poles. , keywords =. doi:10.1088/0004-637X/714/2/1170 , archivePrefix =. 1003.4519 , primaryClass =

    doi arXiv

  224. [232]

    , keywords =

    The Alignment of Interstellar Grains. , keywords =. doi:10.1086/164499 , adsurl =

    doi

  225. [233]

    , keywords =

    The radial component of the local Galactic magnetic field in 3D. , keywords =. doi:10.1093/mnras/stag640 , archivePrefix =. 2604.01093 , primaryClass =

    doi

  226. [234]

    , keywords =

    Theory of Star Formation. , keywords =. doi:10.1146/annurev.astro.45.051806.110602 , archivePrefix =. 0707.3514 , primaryClass =

    doi arXiv

  227. [235]

    , keywords =

    Magnetic Field Strengths and Variations in Grain Alignment in the Local Bubble Wall. , keywords =. doi:10.3847/1538-4357/ab063c , archivePrefix =. 1901.07692 , primaryClass =

    1901 doi arXiv

  228. [236]

    , year = 1956, month = jan, volume =

    Star formation in magnetic dust clouds. , year = 1956, month = jan, volume =. doi:10.1093/mnras/116.5.503 , adsurl =

    1956 doi

  229. [237]

    , keywords =

    Magnetic braking during star formation - III. , keywords =. doi:10.1093/mnras/187.2.337 , adsurl =

    doi

  230. [238]

    , keywords =

    Observation of Turbulent Fluctuations in the Interstellar Plasma Density and Magnetic Field on Spatial Scales of 0.01 to 100 Parsecs. , keywords =. doi:10.1086/176803 , adsurl =

    doi

  231. [239]

    , keywords =

    The effect of HII regions on rotation measure of pulsars. , keywords =. doi:10.1051/0004-6361:20021702 , adsurl =

    doi

  232. [240]

    , keywords =

    Separation of anomalous and synchrotron emissions using WMAP polarization data. , keywords =. doi:10.1051/0004-6361:200809484 , archivePrefix =. 0802.3345 , primaryClass =

    doi arXiv

  233. [241]

    , keywords =

    Performance test of QU-fitting in cosmic magnetism study. , keywords =. doi:10.1093/mnras/sty2862 , archivePrefix =. 1710.01485 , primaryClass =

    doi arXiv

  234. [242]

    Progress in Particle and Nuclear Physics , keywords =

    Progress in high-energy cosmic ray physics. Progress in Particle and Nuclear Physics , keywords =. doi:10.1016/j.ppnp.2017.10.002 , archivePrefix =. 1710.11155 , primaryClass =

    2017 doi arXiv

  235. [243]

    , keywords =

    The coexistence of odd and even parity magnetic fields in disc galaxies. , keywords =. doi:10.1051/0004-6361:200809808 , adsurl =

    doi

  236. [244]

    Nonhomologous contraction and equilibria of self-gravitating, magnetic interstellar clouds embedded in an intercloud medium: star formation. II. Results. , keywords =. doi:10.1086/154478 , adsurl =

    doi

  237. [245]

    , keywords =

    The angular momentum problem and magnetic braking: an exact, time-dependent solution. , keywords =. doi:10.1086/157077 , adsurl =

    doi

  238. [246]

    , keywords =

    Magnetic braking of an aligned rotator during star formation - an exact, time-dependent solution. , keywords =. doi:10.1086/157936 , adsurl =

    doi

  239. [247]

    , keywords =

    On the Dispersion in Direction of Interstellar Polarization. , keywords =. doi:10.1086/170070 , adsurl =

    doi

  240. [248]

    , keywords =

    An underlying universal pattern in galaxy halo magnetic fields. , keywords =. doi:10.1051/0004-6361/202039622 , archivePrefix =. 2101.05291 , primaryClass =

    doi

  241. [249]

    , keywords =

    Theoretical Challenges in Galaxy Formation. , keywords =. doi:10.1146/annurev-astro-081913-040019 , archivePrefix =. 1612.06891 , primaryClass =

    doi arXiv

  242. [250]

    , keywords =

    Contraction of Magnetic Interstellar Clouds. , keywords =

  243. [251]

    , keywords =

    Faraday rotation measures of Northern hemisphere pulsars using CHIME/Pulsar. , keywords =. doi:10.1093/mnras/staa1658 , archivePrefix =. 2006.06538 , primaryClass =

    2006 doi

  244. [252]

    , keywords =

    The Magnetic Field of the Milky Way from Faraday Rotation of Pulsars and Extragalactic Sources. , keywords =. doi:10.1007/s11214-011-9860-2 , adsurl =

    doi

  245. [253]

    , keywords =

    New pulsar rotation measures and the Galactic magnetic field. , keywords =. doi:10.1111/j.1365-2966.2008.13188.x , archivePrefix =. 0803.0677 , primaryClass =

    2008 doi

  246. [254]

    , keywords =

    A dynamo amplifying the magnetic field of a Milky-Way-like galaxy. , keywords =. doi:10.1051/0004-6361/202037835 , archivePrefix =. 2006.12574 , primaryClass =

    2006 doi

  247. [255]

    , keywords =

    The role of magnetic fields in the structure and interaction of supershells. , keywords =. doi:10.1051/0004-6361/201629268 , archivePrefix =. 1701.03696 , primaryClass =

    doi arXiv

  248. [256]

    , keywords =

    The random magnetic field in the Galaxy. , keywords =. doi:10.1093/mnras/262.4.953 , adsurl =

    doi

  249. [257]

    , keywords =

    The Local Bubble Is a Local Chimney: A New Model from 3D Dust Mapping. , keywords =. doi:10.3847/1538-4357/ad61de , archivePrefix =. 2403.04961 , primaryClass =

    doi

  250. [258]

    , keywords =

    Estimating extragalactic Faraday rotation. , keywords =. doi:10.1051/0004-6361/201423995 , archivePrefix =. 1404.3701 , primaryClass =

    doi arXiv

  251. [259]

    , keywords =

    An improved map of the Galactic Faraday sky. , keywords =. doi:10.1051/0004-6361/201118526 , archivePrefix =. 1111.6186 , primaryClass =

    doi arXiv

  252. [260]

    , keywords =

    GMIMS-DRAGONS: A Faraday Depth Survey of the Northern Sky Covering 350--1030 MHz. , keywords =. doi:10.3847/1538-4365/ae2471 , archivePrefix =. 2510.09759 , primaryClass =

    doi

  253. [261]

    , keywords =

    Three-dimensional structure of the magnetic field in the disk of the Milky Way. , keywords =. doi:10.1051/0004-6361/201730740 , archivePrefix =. 1704.08663 , primaryClass =

    doi arXiv

  254. [262]

    , keywords =

    Turbulence and star formation efficiency in molecular clouds: solenoidal versus compressive motions in Orion B. , keywords =. doi:10.1051/0004-6361/201629220 , archivePrefix =. 1701.00962 , primaryClass =

    doi arXiv

  255. [263]

    , keywords =

    Galactic synchrotron emission with cosmic ray propagation models. , keywords =. doi:10.1093/mnras/stt1718 , archivePrefix =. 1309.2947 , primaryClass =

    doi arXiv

  256. [264]

    , keywords =

    The Faraday Rotation Measure Grid of the LOFAR Two-metre Sky Survey: Data Release 2. , keywords =. doi:10.1093/mnras/stac3820 , archivePrefix =. 2301.07697 , primaryClass =

    doi

  257. [265]

    , keywords =

    Complex Faraday depth structure of active galactic nuclei as revealed by broad-band radio polarimetry. , keywords =. doi:10.1111/j.1365-2966.2012.20554.x , archivePrefix =. 1201.3161 , primaryClass =

    2012 doi

  258. [266]

    , keywords =

    Density, Velocity, and Magnetic Field Structure in Turbulent Molecular Cloud Models. , keywords =. doi:10.1086/318290 , archivePrefix =. astro-ph/0008454 , primaryClass =

    doi arXiv

  259. [267]

    Mapping the Galactic magnetic field with pulsar observations

    The Thousand-Pulsar-Array programme on MeerKAT - XVI. Mapping the Galactic magnetic field with pulsar observations. , keywords =. doi:10.1093/mnras/staf645 , archivePrefix =. 2504.09722 , primaryClass =

    doi

  260. [268]

    , keywords =

    JVLA S- and X-band polarimetry of the merging cluster Abell 2256. , keywords =. doi:10.1093/pasj/psv082 , archivePrefix =. 1508.01317 , primaryClass =

    doi arXiv

  261. [269]

    System set-up and early results

    The MPIfR-MeerKAT Galactic Plane Survey - I. System set-up and early results. , keywords =. doi:10.1093/mnras/stad1900 , archivePrefix =. 2303.09231 , primaryClass =

    doi

  262. [270]

    , keywords =

    Theoretical Models of Polarized Dust Emission from Protostellar Cores. , keywords =. doi:10.1086/322504 , archivePrefix =. astro-ph/0104231 , primaryClass =

    doi arXiv

  263. [271]

    , keywords =

    Spectral index of synchrotron emission: insights from the diffuse and magnetised interstellar medium. , keywords =. doi:10.1051/0004-6361/202140799 , archivePrefix =. 2106.10929 , primaryClass =

    doi

  264. [272]

    , keywords =

    Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis. , keywords =. doi:10.1086/513699 , archivePrefix =. astro-ph/0603450 , primaryClass =

    doi arXiv

  265. [273]

    , keywords =

    Magnetic field formation in the Milky Way like disc galaxies of the Auriga project. , keywords =. doi:10.1093/mnras/stx1074 , archivePrefix =. 1701.07028 , primaryClass =

    doi arXiv

  266. [274]

    , keywords =

    Faraday rotation maps of disc galaxies. , keywords =. doi:10.1093/mnras/sty2601 , archivePrefix =. 1807.02113 , primaryClass =

    doi arXiv

  267. [275]

    , keywords =

    A method for reconstructing the Galactic magnetic field using dispersion of fast radio bursts and Faraday rotation of radio galaxies. , keywords =. doi:10.1093/mnras/stac2314 , archivePrefix =. 2208.06417 , primaryClass =

    doi

  268. [276]

    , keywords =

    A Compilation of Optical Starlight Polarization Catalogs. , keywords =. doi:10.3847/1538-4365/ad8b21 , archivePrefix =. 2307.05752 , primaryClass =

    doi

  269. [277]

    , keywords =

    Demonstration of Magnetic Field Tomography with Starlight Polarization toward a Diffuse Sightline of the ISM. , keywords =. doi:10.3847/1538-4357/aafdb2 , archivePrefix =. 1809.09804 , primaryClass =

    doi arXiv

  270. [278]

    , keywords =

    Fast Dynamos, Cosmic Rays, and the Galactic Magnetic Field. , keywords =. doi:10.1086/172046 , adsurl =

    doi

  271. [279]

    The Generation of Magnetic Fields in Astrophysical Bodies. II. The Galactic Field. , year = 1971, month = jan, volume =. doi:10.1086/150765 , adsurl =

    1971 doi

  272. [280]

    , year = 1955, month = sep, volume =

    Hydromagnetic Dynamo Models. , year = 1955, month = sep, volume =. doi:10.1086/146087 , adsurl =

    1955 doi

  273. [281]

    , keywords =

    Analysis of spiral arms using anisotropic wavelets: gas, dust and magnetic fields in M 51. , keywords =. doi:10.1051/0004-6361:20065225 , archivePrefix =. astro-ph/0609787 , primaryClass =

    doi arXiv

  274. [282]

    , keywords =

    The JCMT BISTRO Survey: The Magnetic Field Strength in the Orion A Filament. , keywords =. doi:10.3847/1538-4357/aa80e5 , archivePrefix =. 1707.05269 , primaryClass =

    doi arXiv

  275. [283]

    , keywords =

    Testing Galactic Magnetic Field Models Using Near-infrared Polarimetry. , keywords =. doi:10.1088/0004-637X/749/1/71 , archivePrefix =. 1202.1020 , primaryClass =

    doi arXiv

  276. [284]

    , keywords =

    Using Red Clump Stars to Decompose the Galactic Magnetic Field with Distance. , keywords =. doi:10.1088/0004-6256/148/3/49 , archivePrefix =. 1407.7268 , primaryClass =

    doi arXiv

  277. [285]

    , keywords =

    The first degree-scale starlight-polarization-based tomography map of the magnetized interstellar medium. , keywords =. doi:10.1051/0004-6361/202349015 , archivePrefix =. 2404.10821 , primaryClass =

    doi

  278. [286]

    , keywords =

    Starlight-polarization-based tomography of the magnetized ISM: PASIPHAE's line-of-sight inversion method. , keywords =. doi:10.1051/0004-6361/202244625 , archivePrefix =. 2208.02278 , primaryClass =

    doi

  279. [287]

    , keywords =

    Galactic magnetic field reconstruction using the polarized diffuse Galactic emission: formalism and application to Planck data. , keywords =. doi:10.1051/0004-6361/201833962 , archivePrefix =. 1807.10515 , primaryClass =

    doi

  280. [288]

    , keywords =

    Modeling the magnetized Local Bubble from dust data. , keywords =. doi:10.1051/0004-6361/201937157 , archivePrefix =. 1911.09691 , primaryClass =

    1911 doi

  281. [289]

    , keywords =

    Detection of magnetic fields in superclusters of galaxies. , keywords =. doi:10.1051/0004-6361/202553709 , adsurl =

    doi

  282. [290]

    , keywords =

    Magnetic Fields in High-mass Infrared Dark Clouds. , keywords =. doi:10.1088/0004-637X/799/1/74 , archivePrefix =. 1410.7390 , primaryClass =

    doi arXiv

  283. [291]

    , keywords =

    Models of Vertically Stratified Two-Phase ISM Disks with MRI-Driven Turbulence. , keywords =. doi:10.1086/518103 , archivePrefix =. astro-ph/0703648 , primaryClass =

    doi arXiv

  284. [292]

    Planck 2018 results. XI. Polarized dust foregrounds. , keywords =. doi:10.1051/0004-6361/201832618 , archivePrefix =. 1801.04945 , primaryClass =

    2018 doi

  285. [293]

    Planck intermediate results. XXXII. The relative orientation between the magnetic field and structures traced by interstellar dust. , keywords =. doi:10.1051/0004-6361/201425044 , archivePrefix =. 1409.6728 , primaryClass =

    doi arXiv

  286. [294]

    Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust. , keywords =. doi:10.1051/0004-6361/201424082 , archivePrefix =. 1405.0871 , primaryClass =

    doi arXiv

  287. [295]

    Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds. , keywords =. doi:10.1051/0004-6361/201525896 , archivePrefix =. 1502.04123 , primaryClass =

    doi arXiv

  288. [296]

    Planck intermediate results. XLII. Large-scale Galactic magnetic fields. , keywords =. doi:10.1051/0004-6361/201528033 , archivePrefix =. 1601.00546 , primaryClass =

    doi arXiv

  289. [297]

    , keywords =

    A more detailed look at Galactic magnetic field models: using free-free absorption in HII regions. , keywords =. doi:10.1051/0004-6361/201937042 , archivePrefix =. 2002.09204 , primaryClass =

    2002 doi

  290. [298]

    , keywords =

    Low-frequency measurements of synchrotron absorbing HII regions and modeling of observed synchrotron emissivity. , keywords =. doi:10.1051/0004-6361/201834405 , archivePrefix =. 1811.10310 , primaryClass =

    doi arXiv

  291. [299]

    , keywords =

    Deriving the Global Structure of the Galactic Magnetic Field from Faraday Rotation Measures of Extragalactic Sources. , keywords =. doi:10.1088/0004-637X/738/2/192 , archivePrefix =. 1103.0814 , primaryClass =

    doi arXiv

  292. [300]

    The Dusty Universe , year = 1975, editor =

    Interstellar grains as pinwheels. The Dusty Universe , year = 1975, editor =

    1975

Pith tools

Reviewed June 28, 2026 · model on record in the stance chip above.