publication venue for

• The hydrogen Lyman α line shape in the exospheres of terrestrial objects in the solar system 2025
• The effects of plasma source on adiabatic electron acceleration at dipolarization fronts 2025
• Day-to-day and longitudinal variability of the equatorial electrojet as viewed from the Sun-synchronous CSES satellite 2024
• Radiation belt phase space density: calculation analysis and model dependence 2024
• Characteristics of plasma boundaries with large density gradients and their effects on Kelvin-Helmholtz instability 2024
• Quantifying adiabatic motion in the outer radiation belt and ring current with invariant matching 2024
• Science return of probing magnetospheric systems of ice giants 2024
• Gradient calculation techniques for multi-point ionosphere/thermosphere measurements from GDC 2024
• Editorial: Observations and simulations of layering phenomena in the middle/upper atmosphere and ionosphere 2024
• Statistical analysis of overlapping double ion energy dispersion events in the northern cusp 2024
• Forecasting solar flares with a transformer network 2024
• The effects of particle injections on the ring current development during the 7-8 September 2017 geomagnetic storm 2023
• Testing adiabatic models of energetic electron acceleration at dipolarization fronts 2023
• Simulation of radiation belt wave-particle interactions in an MHD-particle framework 2023
• Evaluating the performance of empirical models of total electron density and whistler-mode wave amplitude in the Earth's inner magnetosphere 2023
• Deep learning model of hiss waves in the plasmasphere and plumes and their effects on radiation belt electrons 2023
• Heliospheric 3-D MHD ENLIL simulations of multi-CME and multi-spacecraft events 2023
• The complexity of the day-side X-line during southward interplanetary magnetic field 2023
• Mesoscale phenomena and their contribution to the global response: a focus on the magnetotail transition region and magnetosphere-ionosphere coupling 2023
• MAVEN mission perspectives and approaches to inclusion 2023
• Agile collaboration: Citizen science as a transdisciplinary approach to heliophysics 2023
• Making an executable paper with the Python in Heliophysics Community to foster open science and improve reproducibility 2023
• Delineating the effect of upward propagating migrating solar tides with the TIEGCM-ICON 2023
• Editorial: Machine learning and statistical methods for solar flare prediction 2023
• Modeling of the cold electron plasma density for radiation belt physics 2023
• Enhancing demographics and career pathways of the space physics workforce in the US 2023
• Plasma-neutral interactions in the lower thermosphere-ionosphere: The need for in situ measurements to address focused questions 2023
• Daedalus MASE (mission assessment through simulation exercise): A toolset for analysis of in situ missions and for processing global circulation model outputs in the lower thermosphere-ionosphere 2023
• Spatio-temporal comparisons of the hydrogen-alpha line width and ALMA 3 mm brightness temperature in the weak solar network 2023
• A comparison of energetic particle energization observations MMS at and injections at Van Allen Probes 2023
• Deciphering the birth region, formation, and evolution of ambient and transient solar wind using heavy ion observations 2022
• pyGPI5: A python D- and E-region chemistry and ionization model 2022
• How open data and interdisciplinary collaboration improve our understanding of space weather: A risk and resiliency perspective 2022
• On the importance of neutral composition and temperature measurements in the 100-200 km altitude region 2022
• Near-ultraviolet continuum modeling of the 1985 April 12 great flare of AD Leo 2022
• Next generation magnetic field measurements from low-earth orbit satellites enable enhanced space weather operations 2022
• Impacts of acoustic and gravity waves on the ionosphere 2022
• Improving ionospheric predictability requires accurate simulation of the mesospheric polar vortex 2022
• Understanding the properties, wave drivers, and impacts of electron microburst precipitation: Current understanding and critical knowledge gaps 2022
• First looks at solar active regions with ALMA 2022
• Interplanetary mesoscale observatory (InterMeso): A mission to untangle dynamic mesoscale structures throughout the heliosphere 2022
• The Space Physics Environment Data Analysis System in Python 2022
• A global view of Pc3 wave activity in near-Earth space: Results from hybrid-Vlasov simulations 2022
• Magnetospheric responses to solar wind Pc5 density fluctuations: Results from 2D hybrid Vlasov simulation 2022
• Importance of lower atmospheric forcing and magnetosphere-ionosphere coupling in simulating neutral density during the February 2016 geomagnetic storm 2022
• Prediction of plasmaspheric hiss spectral classes 2022
• Statistical investigation on equatorial pitch angle distribution of energetic electrons in Earth's outer radiation belt during CME- and CIR-driven storms 2022
• Proton aurora and relativistic electron microbursts scattered by electromagnetic ion cyclotron waves 2022
• A Statistical Study of Magnetopause Boundary Layer Energetic Electron Enhancements Using MMS 2022
• Plasma Imaging, LOcal Measurement, and Tomographic Experiment (PILOT): A Mission Concept for Transformational Multi-Scale Observations of Mass and Energy Flow Dynamics in Earth's Magnetosphere 2022
• Differentiating Between the Leading Processes for Electron Radiation Belt Acceleration 2022
• ULF Wave Modeling, Effects, and Applications: Accomplishments, Recent Advances, and Future 2022
• Sulfur- and Iron-Rich Mineralogical Features Preserved in Permafrost in the Canadian High Arctic: Analogs for the Astrobiological Exploration of Mars 2022
• Microbial Survival in an Extreme Martian Analog Ecosystem: Poas Volcano, Costa Rica 2022
• Observations of Pole-to-Pole, Stratosphere-to-Ionosphere Connection 2022
• Secondary Magnetic Reconnection at Earth's Flank Magnetopause 2021
• Ion Dynamics in the Meso-scale 3-D Kelvin-Helmholtz Instability: Perspectives From Test Particle Simulations 2021
• Bifurcated Current Sheet Observed on the Boundary of Kelvin-Helmholtz Vortices 2021
• MMS Observations of Double Mid-Latitude Reconnection Ion Beams in the Early Non-Linear Phase of the Kelvin-Helmholtz Instability 2021
• The Current State and Future Directions of Modeling Thermosphere Density Enhancements During Extreme Magnetic Storms 2021
• The Occurrence and Prevalence of Time Domain Structures in the Kelvin-Helmholtz Instability at Different Positions Along the Earth's Magnetospheric Flanks 2021
• Thermospheric Neutral Winds as the Cause of Drift Shell Distortion in Earth's Inner Radiation Belt 2021
• On the Impacts of Ions of Ionospheric Origin and Their Composition on Magnetospheric EMIC Waves 2021
• Langmuir Turbulence in the Auroral Ionosphere: Origins and Effects 2021
• Iterative Tomography: A Key to Providing Time-Dependent 3-D Reconstructions of the Inner Heliosphere and the Unification of Space Weather Forecasting Techniques 2020
• A General Overview for Localizing Short Gamma-Ray Bursts with a CubeSat Mega-Constellation 2020
• Solar-Terrestrial Data Science: Prior Experience and Future Prospects 2020
• Convolutional Neural Networks for Predicting the Strength of the Near-Earth Magnetic Field Caused by Interplanetary Coronal Mass Ejections 2020
• MMS SITL Ground Loop: Automating the Burst Data Selection Process 2020
• Spectral Deconvolution With Deep Learning: Removing the Effects of Spectral PSF Broadening 2020
• Relativistic Particle Beams as a Resource to Solve Outstanding Problems in Space Physics 2019
• Atmospheric Effects of a Relativistic Electron Beam Injected From Above: Chemistry, Electrodynamics, and Radio Scattering 2019
• Understanding the Death of Massive Stars Using an Astrophysical Transients Observatory 2018
• Infrared Dual-Line Hanle Diagnostic of the Coronal Vector Magnetic Field 2016
• ROAM: A Radial-Basis-Function Optimization Approximation Method for Diagnosing the Three-Dimensional Coronal Magnetic Field 2016
• A survey of solar wind conditions at 5 AU: a tool for interpreting solar wind-magnetosphere interactions at Jupiter 2014