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Every paper Pith has read. Search by title, abstract, or pith.
138 papers in physics.space-ph · page 2
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CNN classifies Mars plasma regions from ion spectra alone
Automated Classification of Plasma Regions at Mars Using Machine Learning
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Solar cycle predictions before previous peak are meaningless
Solar Cycle Prediction: Challenges, Progress, and Future Perspectives
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Coronal seeds are evolved into solar wind switchbacks by local processes
Magnetic switchback formation: a review of proposed mechanisms
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Solar wind proton structures reduce ion-acoustic wave damping
The Damping and Instability of Ion-acoustic Waves in the Solar Wind: Solar Orbiter Observations
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Tailward reconnection yields similar cusp ions in two IMF geometries
Simultaneous TRACERS and THEMIS Observations of Reversed Cusp Ion Dispersions and Dual-Lobe Reconnection
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Spacecraft radio signal detects solar coronal activity
Probing Coronal Activity Using Radio Signals Based on the 2021 superior conjunction of Mars: the Downlink Data from Tianwen-1
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Tool standardizes solar jet length and curvature measurements
SJET: An Interactive Solar Jet Extraction Tool
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Turbulence suppresses FIP fractionation in solar corona
Chromospheric dynamics and turbulence regulate the solar FIP effect
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Electron impacts ionize Ganymede ten times more than sunlight
Constraining Electron-Impact Ionization of O$_2$ Through UV Aurora Observations at Ganymede
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CME creates sub-Alfvénic solar wind with weak MHD turbulence
MMS Insights into CME Driven Sub-Alfv\'enic Solar Wind at 1 AU
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One parameter sets wave attenuation or shock formation in pair plasmas
Interaction of Strong Electromagnetic Waves with Unmagnetized Pair Plasmas
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QBO amplitudes decouple from solar cycle strength with cycle-specific slopes
Spatio-temporal analysis of helioseismic quasi-biennial oscillations
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Waves scatter pickup ions to isotropize them at moons
Ion pickup and velocity space thermalization at outer planet moons
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ML identifies four solar wind regimes at Mars
Solar Wind Classifications at Mars using Machine Learning Techniques
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Suppressing chromospheric turbulence boosts wind mass flux tenfold
Chromospheric turbulence as a regulator of stellar wind mass flux
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Integrated panels give orbital AI 100 kW per ton
Reduced-Mass Orbital AI Inference via Integrated Solar, Compute, and Radiator Panels
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Spectral exponents predict Forbush decreases better than CME speeds
New insights from cross-correlation studies between solar activity indices and cosmic-ray flux during Forbush decrease events
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Three-component electrons trigger dual heat-flux instabilities
Modeling complex plasma instabilities in space plasmas - Three-component electron formalism of heat-flux instabilities
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Active streamers produce twice as many blobs as quiet ones
Statistics of blob properties in two types of coronal streamers
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Researchers trained LSTM neural networks on time series of solar continuum intensity and…
Prediction of Magnetic Flux Evolution During Solar Active Region Emergence using Long Short-Term Memory Networks
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Shocks heat solar wind protons differently by geometry
Proton Temperature Anisotropy Across Interplanetary Shocks: A Statistical Analysis with WIND observations
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Foreshock structures form alike but stay immature at interplanetary shocks
Compressive Structures in the Foreshock of Collisionless Shocks
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KAW turbulence forms density cavities without inertial cascade
Inertial-Range Suppression and Ponderomotive Density Cavitation in Broadband Sub-Alfv\'{e}nic Turbulence under Plasma Sheet Boundary Layer Conditions
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Force imbalance builds rising flux rope in solar simulation
Formation and rising phase of a flux rope through data-constrained simulations
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Dissipative model conserves angular momentum in N-body systems
An angular-momentum preserving dissipative model for the point-mass N -body problem
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Kappa distributions fix solar corona temperature mismatch
The diagnostic temperature discrepancy as evidence for non-Maxwellian coronal electrons
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Early galaxies recycle just 15-20 percent of their stellar mass
The Baryon Budget of Galaxies across the First Billion Years
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Lense-Thirring model fits 20-day precession in AT2020afhd
The no-hair theorems at work in the tidal disruption event AT2020afhd
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Slow modes dominate solar wind compressibility near the Sun
Characterization of compressible fluctuations in solar wind streams dominated by balanced and imbalanced turbulence: Parker Solar Probe, Solar Orbiter and Wind observations
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Compensated helicity density stabilizes Saffman plateaus in turbulence decay
Kinetic Route to Helicity-Constrained Decay
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Kinetic KHI mixes plasma only in narrow zones
Plasma Mixing Driven by the Collisionless Kelvin-Helmholtz Instability: Insights from fully kinetic simulation and density-based diagnostics
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Four L1 spacecraft find ICME turbulence varies over 80 Earth radii
Unprecedented Multipoint Observation of Spatially Varying ICME Turbulence of Different Ages during October 2024 Extreme Solar Storm at 1 AU
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Initial in-situ data forecasts CME magnetic fields with ~5 hour errors
Towards a Fully Automated Pipeline for Short-Term Forecasting of In Situ Coronal Mass Ejection Magnetic Field Structure
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Q-exponential approximation speeds Kappa sampling on GPUs
An approximate Kappa generator for particle simulations
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Superposition of timescales yields 1/f spectrum in solar wind data
$1/f$ Noise in Synthetic and Solar Wind Data: Superposition Principles
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GNN emulators forecast 5D plasma fields with 0.95 correlation at 100x speedup
Deterministic and probabilistic neural surrogates of global hybrid-Vlasov simulations
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Spacecraft electrons contaminate detector above potential threshold
Modelling spacecraft-emitted electrons measured by SWA-EAS experiment on board Solar Orbiter mission
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Simulations link solar wave biases to geometry plus rotation
Investigating the Center-to-Limb Effects in Helioseismic Data Using 3D Radiative Hydrodynamic Simulations
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Steep turbulence yields universal power-law tails in plasmas
Non-thermal particle acceleration in multi-species kinetic plasmas: universal power-law distribution functions and temperature inversion in the solar corona
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50 nm aluminum blocks 99.6% light on skipper-CCDs
Light-tight skipper-CCDs for X-ray detection in space
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Mercury tail spectra show energy injection at ion scales
Spectral Properties and Energy Injection in Mercury's Magnetotail Current Sheet
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CubeSat detects nuclear weapon at 4 km via cosmic protons
Verification of the Outer Space Treaty with Cosmic Protons
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Multi-task net raises solar particle detection rates
Solar Energetic Particle Forecasting with Multi-Task Deep Learning: SEPNET
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Speed predicts solar wind turbulence energy
A robust empirical relationship between speed and turbulence energy in the near-Earth solar wind
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Heat flux in magnetosheath shaped by draped field and whistler limits
Electron Heat Flux and Whistler Instability in the Earth's Magnetosheath
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Impact plasma amplifies ancient Mercury magnetic field tenfold
Impact Plasma Amplification of the Ancient Mercury Magnetic Field
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Flux ropes form inside solar reconnection exhausts near the Sun
Magnetic flux ropes within reconnection exhausts close to the centers of heliospheric current sheets near the Sun
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Updated CR-MHD models fix errors in cosmic ray transport on galaxy scales
Cosmic Rays on Galaxy Scales: Progress and Pitfalls for CR-MHD Dynamical Models
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Upstream Solar Orbiter data forecasts geomagnetic storms hours ahead of L1
Real-time prediction of two geomagnetic storms using Solar Orbiter as a far upstream solar wind monitor
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Neural network tracks cosmic rays to 1.4° resolution
A Neural-Network Framework for Tracking and Identification of Cosmic-Ray Nuclei in the RadMap Telescope