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INDEX

Every paper Pith has read and judged, in one searchable index.

449 reviewed papers in physics.space-ph · newest first · page 9

Pith rank means recent reader upvotes with each upvote's ranking weight halved after 24 hours. The archive itself is sorted by arXiv submission date.

  1. physics.plasm-ph arXiv submitted 2025-02-03
    Beta diffusion, not alpha, drives dynamo field growth

    Kiwan Park · “Magnetic Field Amplification and Reconstruction in Rotating Astrophysical Plasmas: Verifying the Roles of $\alpha$ and $\beta$ in Dynamo Action”

    2502.01300
  2. astro-ph.SR arXiv submitted 2025-02-03
    Most solar cycle 25 forecasts underestimated its peak

    Floe Foxon · “Solar Cycles: Can They Be Predicted?”

    2502.00978
  3. astro-ph.SR arXiv submitted 2025-02-03
    Convection scales keep rising past 7 Mm in the Sun

    Irina N. Kitiashvili +1 · “Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling”

    2502.00974
  4. astro-ph.SR arXiv submitted 2025-01-31
    MHD model reproduces stealth CME's magnetic field at SolO and Earth

    Talwinder Singh +3 · “Magnetohydrodynamic Simulation of a Coronal Mass Ejection Observed During the Near-radial Alignment of Solar Orbiter and Earth”

    2502.00175
  5. physics.space-ph arXiv submitted 2025-01-30
    Neutron monitor data show a 7-21 hour lead on geomagnetic storms

    Imre Kisv\'ardai +6 · “Analysis of 42 years of Cosmic Ray Measurements by the Neutron Monitor at Lomnick\'y st\'it Observatory”

    2502.09627
  6. astro-ph.SR arXiv submitted 2025-01-27
    STEREO should detect nanodust again when the current sheet tilts low

    Nicole Meyer-Vernet · “Will nanodust reappear in STEREO/WAVES data?”

    2501.16133
  7. astro-ph.SR arXiv submitted 2025-01-27
    Icarus 3.0: refreshed solar-wind boundary beats steady driving in tests

    Tinatin Baratashvili +4 · “Icarus 3.0: Dynamic Heliosphere Modelling”

    2501.15923
  8. physics.space-ph arXiv submitted 2025-01-27
    Dense lunar dust clouds could crash landers on low orbits

    Oleksiy V. Arkhypov +1 · “Dangerous dust clouds above lunar surface”

    2501.16402
  9. astro-ph.SR arXiv submitted 2025-01-26
    Eruption's EUV wave shakes a prominence 600 Mm away

    Valeriia Liakh +1 · “Numerical study of solar eruption, extreme-ultraviolet wave propagation, and wave-induced prominence dynamics”

    2501.15697
  10. astro-ph.EP arXiv submitted 2025-01-26
    Streaming dark matter tied to 27.32-day rhythms

    A. Argiriou +18 · “Novel Dark Matter Signatures”

    2501.15498
  11. astro-ph.HE arXiv submitted 2025-01-26
    Disk-corona power fraction tracks black hole mass and feeding rate

    Labani Mallick (CITA National Fellow) +8 · “Constraining Disk-to-Corona Power Transfer Fraction, Soft X-ray Excess Origin, and Black Hole Spin Population of Type-1 AGN across Mass Scales”

    2501.15380
  12. astro-ph.SR arXiv submitted 2025-01-25
    First all-sky maps reveal the solar termination shock's strength

    E. J. Zirnstein +6 · “Global Heliospheric Termination Shock Strength in the Solar-Interstellar Interaction”

    2501.15004
  13. astro-ph.SR arXiv submitted 2025-01-24
    Two ways to average solar particle intensities can differ by up to 5x

    M. E. Cuesta +15 · “Comparing Methods for Calculating Solar Energetic Particle Intensities: Re-binning versus Spectral Binning”

    2501.14923
  14. astro-ph.SR arXiv submitted 2025-01-24
    Proton-beam waves could explain 3He-rich solar flares

    A. Fitzmaurice +2 · “Ion Beam Instabilities during Solar Flare Energy Release”

    2501.14898
  15. astro-ph.SR arXiv submitted 2025-01-24
    AI predicted May 2024 superstorm's full chain of events

    Sabrina Guastavino +3 · “Artificial Intelligence Could Have Predicted All Space Weather Events Associated with the May 2024 Superstorm”

    2501.14684
  16. astro-ph.SR arXiv submitted 2025-01-24
    Sector boundary crossings deepened the Nov 2023 solar storm

    M. Temmer +10 · “Comparative analysis of two episodes of strongly geoeffective CME events in November and December 2023”

    2501.14295
  17. astro-ph.HE arXiv submitted 2025-01-23
    Firehose-stressed plasma can still carry Alfvén waves

    A. F. A. Bott +4 · “Thermodynamics and collisionality in firehose-susceptible high-$\beta$ plasmas”

    2501.13663
  18. astro-ph.SR arXiv submitted 2025-01-21
    Jets and switchbacks show matching rates

    Nina Bizien +4 · “Tracing magnetic switchbacks to their source: An assessment of solar coronal jets as switchback precursors”

    2501.12340
  19. astro-ph.SR arXiv submitted 2025-01-20
    CMEs grow 47% on the way to Earth

    Manuela Temmer · “CME Observations -- from Sun to Impact on Geospace”

    2501.11345
  20. physics.space-ph arXiv submitted 2025-01-16
    A five-step turbulence chain can forge electron-scale magnetic holes

    Joaqu\'in Espinoza-Troni +3 · “Electron scale magnetic holes generation driven by Whistler-to-Bernstein mode conversion in fully kinetic plasma turbulence”

    2501.09651
  21. astro-ph.IM arXiv submitted 2025-01-15
    Sixteen competing concepts preceded JWST

    Pierre Y. Bely +17 · “Genesis of the James Webb Space Telescope Architecture: The Designers' Story”

    2501.09072
  22. astro-ph.SR arXiv submitted 2025-01-14
    Biggest Forbush decrease in 20 years: 15.7% in May 2024

    M. A. Abunina +4 · “On the features of great Forbush effect during May 2024 extreme geomagnetic storm”

    2501.08029
  23. cs.AI arXiv submitted 2025-01-14
    Vision-language agents pilot spacecraft from screen images

    Alejandro Carrasco +5 · “Visual Language Models as Operator Agents in the Space Domain”

    2501.07802
  24. astro-ph.SR arXiv submitted 2025-01-13
    Near-Chandrasekhar delayed-detonation models match JWST spectra

    P. Hoeflich +10 · “Numerical and Physical Challenges to Nebular Spectroscopy in Thermonuclear Supernovae”

    2501.07654
  25. physics.space-ph arXiv submitted 2025-01-09
    Protons from the Sun reach deep into Mercury's magnetosphere

    Daniel Teubenbacher +9 · “Solar wind entry into Mercury's magnetosphere: Simulation results for the second swingby of BepiColombo”

    2501.05363
  26. physics.space-ph arXiv submitted 2025-01-09
    Mexico City UVA irradiance stayed flat over 2018-2021

    C. H. Zepeda Fern\'andez +5 · “Solar irradiance statistical analysis in Mexico City from 2018 to 2021”

    2501.13934
  27. physics.space-ph arXiv submitted 2025-01-08
    3D model reproduces solar wind charge states

    Pete Riley +2 · “Ion Charge States from a Global Time-Dependent Wave-Turbulence-Driven Model of the Solar Wind: Comparison with in-situ Measurements”

    2501.04868
  28. astro-ph.EP arXiv submitted 2025-01-08
    Chondrule dust rims grow only below a 10 cm/s impact threshold

    Chuchu Xiang +4 · “Chondrule dust rim growth: Influence of restructuring using molecular dynamics simulations”

    2501.04625
  29. physics.ins-det arXiv submitted 2025-01-08
    First laser SET test of 4N35 optocoupler reports limits

    Kavin Dave +4 · “Ultrafast pulsed laser evaluation of Single Event Transients in opto-couplers”

    2501.07590
  30. astro-ph.SR arXiv submitted 2025-01-07
    Crescent electron beams out-emit rings in solar radio bursts

    Mehdi Yousefzadeh · “Emission Characteristics of Energetic Electrons with Crescent-shaped Velocity Distributions”

    2501.03559
  31. astro-ph.SR arXiv submitted 2025-01-06
    Shock flank, not diffusion, delayed Parker Solar Probe's SEPs

    A. Kouloumvakos +12 · “Shock and SEP Modeling Study for the 5 September 2022 SEP Event”

    2501.03066
  32. astro-ph.SR arXiv submitted 2025-01-06
    Oxygen ratio drop mislabels slow wind as coronal hole wind

    Verena Heidrich-Meisner +3 · “Challenges in identifying the coronal hole wind”

    2501.02935
  33. astro-ph.SR arXiv submitted 2025-01-06
    Parker's wind model hides Chapman's static corona exactly

    Bhimsen Shivamoggi · “On the Role of Chapman's Hydrostatic Solar Wind Mechanism in Parker's Hydrodynamic Solar Wind Model”

    2501.02731
  34. astro-ph.SR arXiv submitted 2025-01-04
    Solar dynamo runs only twice past the critical switch

    Sanket Wavhal +2 · “Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical”

    2501.02262
  35. astro-ph.SR arXiv submitted 2025-01-04
    Wave pressure drives Alfvénic slow wind

    Yeimy J. Rivera +20 · “Differentiating the acceleration mechanisms in the slow and Alfv\'enic slow solar wind”

    2501.02163
  36. astro-ph.SR arXiv submitted 2025-01-02
    Electron deficit drives solar wind anti-sunward whistlers

    Alfredo Micera +3 · “Quasi-parallel anti-sunward propagating whistler waves associated to the electron-deficit in the near-Sun solar wind: Particle-in-Cell simulation”

    2501.01331
  37. astro-ph.EP arXiv submitted 2025-01-02
    Planet magnetism can be read from spectral line ratios

    M.Rumenskikh +3 · “Probing exoplanetary magnetism via atomic alignment effect”

    2501.01122
  38. cs.LG arXiv submitted 2025-01-02
    SOHO images alone predict which CMEs trigger geomagnetic storms

    Khalid A. Alobaid +8 · “Prediction of Geoeffective CMEs Using SOHO Images and Deep Learning”

    2501.01011
  39. physics.space-ph arXiv submitted 2024-12-31
    Same-batch ferrite cores match to under 0.6% in noise

    S. Saraf +4 · “Performance Variance of Low Noise Resonant Capacitance Bridges While Replacing their Ungapped MnZn Ferrite Cores”

    2501.00681
  40. physics.geo-ph arXiv submitted 2024-12-31
    CNN pairs Mars landforms with Qaidam Basin analogues

    Fanwei Meng +6 · “Deep learning selection of analogues for Mars landing sites in the Qaidam Basin, Qinghai-Tibet Plateau”

    2501.08584
  41. astro-ph.SR arXiv submitted 2024-12-31
    Thermal conduction accelerates tearing

    Sripan Mondal +2 · “Dynamics and Energetics of Resistive, Thermally Conductive, and Radiative Plasma in Coronal Current Sheets due to Asymmetric External Perturbation”

    2501.00255
  42. astro-ph.SR arXiv submitted 2024-12-30
    Electromotive field closes the dynamo–turbulence loop in plasmas

    Philippe-A. Bourdin +1 · “Electromotive field in space and astrophysical plasmas”

    2501.00181
  43. astro-ph.SR arXiv submitted 2024-12-30
    1872 magnetic storm joins Carrington

    Hisashi Hayakawa +21 · “The Extreme Space Weather Event of 1872 February: Sunspots, Magnetic Disturbance, and Auroral Displays”

    2501.00176
  44. physics.ins-det arXiv submitted 2024-09-02
    Entangled BEC sensor designed for microgravity tests

    O. Anton +23 · “INTENTAS -- An entanglement-enhanced atomic sensor for microgravity”

    2409.01051
  45. physics.space-ph arXiv submitted 2024-08-30
    Electron distributions trace Alfvén wing topologies at Earth

    Harsha Gurram +8 · “Earth's Alfv\'{e}n Wings: Unveiling Dynamic Variations of Field-line Topologies with Electron Distributions”

    2409.00247
  46. astro-ph.SR arXiv submitted 2024-07-25
    Reconnection flux rises linearly with erupting rope speed

    Samriddhi Sankar Maity +3 · “Evolution of reconnection flux during eruption of magnetic flux ropes”

    2407.18188
  47. physics.space-ph arXiv submitted 2024-03-27
    MMS spots electron jets and agyrotropy at KH vortex edges in storm

    Harsha Gurram +7 · “Turbulence properties and kinetic signatures of electron in Kelvin-Helmholtz waves during a geomagnetic storm”

    2403.18990
  48. astro-ph.SR arXiv submitted 2023-02-13
    Hall term sets Alfvén wave packet evolution timescale

    Anna Tenerani +4 · “Dispersive and kinetic effects on kinked Alfv\'en wave packets: a comparative study with fluid and hybrid models”

    2302.06150
  49. physics.plasm-ph arXiv submitted 2019-07-26
    Kink instability turns 10% of jet magnetic energy into nonthermal ions

    E. Paulo Alves +2 · “Nonthermal ion acceleration by the kink instability in nonrelativistic jets”

    1907.11693
  50. physics.space-ph arXiv submitted 2019-07-25
    Energy and cross-helicity transfers share scaling in plasma turbulence

    Luca Sorriso-Valvo +20 · “Sign singularity of the local energy transfer in space plasma turbulence”

    1907.11108