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INDEX

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

298 reviewed papers in physics.space-ph · newest first · page 4

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.soc-ph arXiv submitted 2026-04-25
    Static mineral lists can't protect quantum tech

    Min-Ha Lee +3 · “Towards Geostrategic Critical Minerals and Materials Resilience: Secure Supply-Chain and Criticality Analyses for Quantum Technologies in Arctic and Space Environments”

    2605.02926
  2. physics.soc-ph arXiv submitted 2026-04-25
    Quantum tech in space needs dynamic minerals tracking

    Min-Ha Lee +3 · “Towards Geostrategic Critical Minerals and Materials Resilience: Secure Supply-Chain and Criticality Analyses for Quantum Technologies in Arctic and Space Environments”

    2605.02926
  3. physics.space-ph arXiv submitted 2026-04-24
    Bubbles supply 40% of storm ring current energy

    Sina Sadeghzadeh +3 · “Revisiting the Role of Plasma Sheet Bubbles in Stormtime Energy Transport Using RCM-I”

    2604.23043
  4. astro-ph.SR arXiv submitted 2026-04-24
    Anisotropy boosts Alfvén wave decay near the Sun by 50%

    Hayato Saguchi +3 · “Radial evolution of Alfv\'en wave Parametric Decay Instability in the near-Sun solar wind: Effects of Temperature Anisotropy”

    2604.22489
  5. astro-ph.SR arXiv submitted 2026-04-24
    Anisotropy boosts Alfvén PDI growth rate by 50 percent near the Sun

    Hayato Saguchi +3 · “Radial evolution of Alfv\'en wave Parametric Decay Instability in the near-Sun solar wind: Effects of Temperature Anisotropy”

    2604.22489
  6. physics.plasm-ph arXiv submitted 2026-04-23
    Phase mixing alone makes radiation belts look diffusive

    Adnane Osmane +5 · “Collisionless Phase Mixing Mimics Diffusive Transport in Radiation Belt Observations”

    2604.21427
  7. physics.plasm-ph arXiv submitted 2026-04-23
    Phase mixing turns collisionless particle paths into apparent diffusion

    Adnane Osmane +5 · “Collisionless Phase Mixing Mimics Diffusive Transport in Radiation Belt Observations”

    2604.21427
  8. physics.space-ph arXiv submitted 2026-04-23
    Solar wind turbulence shifts with distance

    Xinmin Li (1) +33 · “Properties and Radial Evolution of Solar Wind Turbulence Near Mercury's Orbit”

    2604.21196
  9. physics.space-ph arXiv submitted 2026-04-23
    Inertial-range solar wind turbulence stays at -3/2 slope near Mercury

    Xinmin Li (1) +33 · “Properties and Radial Evolution of Solar Wind Turbulence Near Mercury's Orbit”

    2604.21196
  10. astro-ph.SR arXiv submitted 2026-04-22
    Localized heating fits into polytropic stellar wind models

    L. Westrich (1 +25 · “Polytropic stellar wind models with strongly localized heating”

    2604.20552
  11. astro-ph.EP arXiv submitted 2026-04-22
    Hubble reanalysis finds no water aurora on Europa

    L. Roth +15 · “Europa's Lyman-$\alpha$ emissions from HST/STIS observations”

    2604.20324
  12. astro-ph.EP arXiv submitted 2026-04-21
    NanoTug swarms de-orbit debris with fewer units via planned placement

    F. Alnaqbi +2 · “Conceptual Design and Analysis of a NanoTug Swarm for Active Debris Removal”

    2604.19214
  13. physics.plasm-ph arXiv submitted 2026-04-20
    Reconnection rate decreases with larger system size

    Yi-Min Huang +4 · “System Size Dependence of Collisionless Reconnection Rate”

    2604.18787
  14. physics.space-ph arXiv submitted 2026-04-20
    Time-shifted tetrahedra distort FAC estimates at hundreds of km

    R Gajewski +15 · “On the curlometer measurement of field-aligned and perpendicular currents in low Earth orbit: Swarm observations and whole geospace simulations”

    2604.18553
  15. physics.ao-ph arXiv submitted 2026-04-20
    SPHEREx maps exospheric helium and oxygen airglow globally

    Howard Hui +22 · “Observations of Atmospheric Helium and Oxygen with SPHEREx”

    2605.00851
  16. cs.LG arXiv submitted 2026-04-20
    Dynamic graphs forecast ionospheric irregularities on new satellite links

    Mert Can Turkmen +2 · “Forecasting Ionospheric Irregularities on GNSS Lines of Sight Using Dynamic Graphs with Ephemeris Conditioning”

    2604.18379
  17. cs.LG arXiv submitted 2026-04-20
    Dynamic graph model beats persistence on 2-hour ionosphere forecasts

    Mert Can Turkmen +2 · “Forecasting Ionospheric Irregularities on GNSS Lines of Sight Using Dynamic Graphs with Ephemeris Conditioning”

    2604.18379
  18. physics.space-ph arXiv submitted 2026-04-20
    Control variates cut drag moment error several-fold at fixed cost

    Jovan Boskovic +2 · “Multi-Fidelity Monte-Carlo Estimation of Satellite Drag in Very-Low-Earth Orbit”

    2604.21943
  19. physics.space-ph arXiv submitted 2026-04-20
    Hamiltonian method recovers lunar wake potentials from electrons

    Xin An +6 · “Inferring lunar wake potentials from electron phase space densities”

    2604.17825
  20. physics.space-ph arXiv submitted 2026-04-18
    CNN classifies Mars plasma regions from ion spectra alone

    Yilan Qin +8 · “Automated Classification of Plasma Regions at Mars Using Machine Learning”

    2604.17131
  21. astro-ph.SR arXiv submitted 2026-04-17
    Solar cycle predictions before previous peak are meaningless

    Bidya Binay Karak · “Solar Cycle Prediction: Challenges, Progress, and Future Perspectives”

    2604.16183
  22. astro-ph.SR arXiv submitted 2026-04-17
    Polar-field seeding limits solar-cycle forecasts to one cycle

    Bidya Binay Karak · “Solar Cycle Prediction: Challenges, Progress, and Future Perspectives”

    2604.16183
  23. astro-ph.SR arXiv submitted 2026-04-17
    Coronal seeds are evolved into solar wind switchbacks by local processes

    Peter F. Wyper +21 · “Magnetic switchback formation: a review of proposed mechanisms”

    2604.16166
  24. astro-ph.SR arXiv submitted 2026-04-15
    Solar wind proton structures reduce ion-acoustic wave damping

    Hao Ran +8 · “The Damping and Instability of Ion-acoustic Waves in the Solar Wind: Solar Orbiter Observations”

    2604.14311
  25. physics.space-ph arXiv submitted 2026-04-15
    Tailward reconnection yields similar cusp ions in two IMF geometries

    M. {\O}ieroset +22 · “Simultaneous TRACERS and THEMIS Observations of Reversed Cusp Ion Dispersions and Dual-Lobe Reconnection”

    2604.14104
  26. physics.space-ph arXiv submitted 2026-04-15
    Same reversed cusp signatures under two IMF geometries

    M. {\O}ieroset +22 · “Simultaneous TRACERS and THEMIS Observations of Reversed Cusp Ion Dispersions and Dual-Lobe Reconnection”

    2604.14104
  27. astro-ph.SR arXiv submitted 2026-04-15
    Spacecraft radio signal detects solar coronal activity

    Yu-Chen Liu +8 · “Probing Coronal Activity Using Radio Signals Based on the 2021 superior conjunction of Mars: the Downlink Data from Tianwen-1”

    2604.13670
  28. astro-ph.SR arXiv submitted 2026-04-15
    Tool standardizes solar jet length and curvature measurements

    Song Tan +6 · “SJET: An Interactive Solar Jet Extraction Tool”

    2604.13590
  29. astro-ph.SR arXiv submitted 2026-04-14
    Turbulence and low acoustic flux flip solar FIP fractionation

    Andy S.H. To +3 · “Chromospheric dynamics and turbulence regulate the solar FIP effect”

    2604.13174
  30. astro-ph.SR arXiv submitted 2026-04-14
    Turbulence suppresses FIP fractionation in solar corona

    Andy S.H. To +3 · “Chromospheric dynamics and turbulence regulate the solar FIP effect”

    2604.13174
  31. astro-ph.EP arXiv submitted 2026-04-14
    Electron impacts ionize Ganymede ten times more than sunlight

    Stefan Duling +5 · “Constraining Electron-Impact Ionization of O$_2$ Through UV Aurora Observations at Ganymede”

    2604.12729
  32. physics.space-ph arXiv submitted 2026-04-13
    CME creates sub-Alfvénic solar wind with weak MHD turbulence

    Harsha Gurram +6 · “MMS Insights into CME Driven Sub-Alfv\'enic Solar Wind at 1 AU”

    2604.12000
  33. physics.plasm-ph arXiv submitted 2026-04-13
    One parameter sets wave attenuation or shock formation in pair plasmas

    Navin Sridhar (1) +18 · “Interaction of Strong Electromagnetic Waves with Unmagnetized Pair Plasmas”

    2604.11698
  34. physics.plasm-ph arXiv submitted 2026-04-13
    One parameter decides how far pulses travel in pair plasmas

    Navin Sridhar (1) +18 · “Interaction of Strong Electromagnetic Waves with Unmagnetized Pair Plasmas”

    2604.11698
  35. astro-ph.SR arXiv submitted 2026-04-12
    QBO amplitudes decouple from solar cycle strength with cycle-specific slopes

    Amir Hasanzadeh +3 · “Spatio-temporal analysis of helioseismic quasi-biennial oscillations”

    2604.10698
  36. physics.space-ph arXiv submitted 2026-04-11
    Waves scatter pickup ions to isotropize them at moons

    Xin An +4 · “Ion pickup and velocity space thermalization at outer planet moons”

    2604.10083
  37. physics.space-ph arXiv submitted 2026-04-09
    ML identifies four solar wind regimes at Mars

    Catherine E. Regan +7 · “Solar Wind Classifications at Mars using Machine Learning Techniques”

    2604.08710
  38. astro-ph.SR arXiv submitted 2026-04-09
    Suppressing chromospheric turbulence boosts wind mass flux tenfold

    Munehito Shoda +2 · “Chromospheric turbulence as a regulator of stellar wind mass flux”

    2604.08020
  39. cs.DC arXiv submitted 2026-04-09
    Integrated panels give orbital AI 100 kW per ton

    Stephen Gaalema +2 · “Reduced-Mass Orbital AI Inference via Integrated Solar, Compute, and Radiator Panels”

    2604.07760
  40. astro-ph.SR arXiv submitted 2026-04-07
    Spectral exponents predict Forbush decreases better than CME speeds

    Mihailo Savi\'c +6 · “New insights from cross-correlation studies between solar activity indices and cosmic-ray flux during Forbush decrease events”

    2604.06383
  41. physics.plasm-ph arXiv submitted 2026-04-07
    Three-component electrons trigger dual heat-flux instabilities

    Dustin L. Schr\"oder +4 · “Modeling complex plasma instabilities in space plasmas - Three-component electron formalism of heat-flux instabilities”

    2604.05729
  42. astro-ph.SR arXiv submitted 2026-04-07
    Active streamers produce twice as many blobs as quiet ones

    Haiyi Li +6 · “Statistics of blob properties in two types of coronal streamers”

    2604.05295
  43. astro-ph.IM arXiv submitted 2026-04-04
    Storms suppress, then triple, pre-satellite plate flashes at GEO

    Kevin Cann · “Storm-Driven Suppression and Post-Storm Enhancement of Photographic Plate Transient Detections at Geosynchronous Altitude: Empirical Evidence and a Candidate Dusty Plasma Mechanism”

    2604.06234
  44. astro-ph.SR arXiv submitted 2026-04-03
    Researchers trained LSTM neural networks on time series of solar continuum intensity and…

    Eren Dogan +7 · “Prediction of Magnetic Flux Evolution During Solar Active Region Emergence using Long Short-Term Memory Networks”

    2604.03507
  45. physics.space-ph arXiv submitted 2026-04-02
    Shocks heat solar wind protons differently by geometry

    Zeping Jin +8 · “Proton Temperature Anisotropy Across Interplanetary Shocks: A Statistical Analysis with WIND observations”

    2604.02452
  46. astro-ph.SR arXiv submitted 2026-04-01
    Curved source surface nearly triples open solar flux

    Ziqi Wu +9 · “A Non-Spherical Model for the Solar Coronal Magnetic Field”

    2604.01028
  47. astro-ph.SR arXiv submitted 2026-04-01
    Lyα emission can map a star’s astrosphere within HST reach

    Ziqi Wu +7 · “Imaging magnetically driven astrospheres: a forward modelling approach”

    2604.00925
  48. astro-ph.SR arXiv submitted 2026-03-30
    SKA radio imaging can reveal where solar particles accelerate

    Diana E. Morosan +8 · “Solar energetic particles and their association with radio emissions”

    2603.28408
  49. physics.space-ph arXiv submitted 2026-03-27
    Suprathermal tails weaken equatorial density pile-up

    Joaqu\'in Espinoza-Troni +2 · “Non-thermal plasma density redistribution in planetary magnetospheres due to ion-cyclotron waves”

    2603.26419
  50. physics.space-ph arXiv submitted 2026-03-18
    Foreshock structures form alike but stay immature at interplanetary shocks

    Savvas Raptis +13 · “Compressive Structures in the Foreshock of Collisionless Shocks”

    2603.17882