In AWSoM, switching from a non-conservative to a conservative energy equation raises CME kinetic energy by 232%, with hotter current-sheet pressure prolonging reconnection.
Title resolution pending
7 Pith papers cite this work, alongside 515 external citations. Polarity classification is still indexing.
7
Pith papers citing it
515
external citations · OpenAlex
citation-role summary
background 2
citation-polarity summary
years
2026 7roles
background 2polarities
background 2representative citing papers
Four Solar Orbiter interplanetary shocks show energetic particle pressure dominating upstream, indicating particle-mediated modification of collisionless shocks.
Hybrid simulations demonstrate formation of hammerhead proton distributions via beam-driven right-handed wave instabilities under young solar wind conditions, consistent with quasi-linear theory.
The C-SWIM model estimates $5.2 billion in capital losses to the US satellite fleet and daily economic impacts ranging from $70 million to $1.3 billion under a 1-in-100-year solar energetic particle event.
Statistical multipoint observations indicate ICME shock acceleration efficiency increases with heliocentric distance up to 0.7 AU before decreasing.
Statistical analysis of solar events shows type II radio burst starting frequencies vary by source region and anti-correlate with proton spectral indices, constraining SEP acceleration mechanisms.
citing papers explorer
-
The Effects of Energy Conservation in Simulating Solar Eruptions
In AWSoM, switching from a non-conservative to a conservative energy equation raises CME kinetic energy by 232%, with hotter current-sheet pressure prolonging reconnection.
-
Energetic particle-mediated interplanetary shocks observed by Solar Orbiter
Four Solar Orbiter interplanetary shocks show energetic particle pressure dominating upstream, indicating particle-mediated modification of collisionless shocks.
-
Hybrid simulations of the proton beam instabilities in the young solar wind. The formation of hammerhead-like distributions
Hybrid simulations demonstrate formation of hammerhead proton distributions via beam-driven right-handed wave instabilities under young solar wind conditions, consistent with quasi-linear theory.
-
C-SWIM: A Coupled Space Weather Impact Model for Satellite Fleet Vulnerability and Economic Loss Under a 1-in-100-Year Solar Energetic Particle Event
The C-SWIM model estimates $5.2 billion in capital losses to the US satellite fleet and daily economic impacts ranging from $70 million to $1.3 billion under a 1-in-100-year solar energetic particle event.
-
Radial Dependency of ICME-associated Particle Acceleration Processes: Statistical Multipoint Observations from 2016-2023
Statistical multipoint observations indicate ICME shock acceleration efficiency increases with heliocentric distance up to 0.7 AU before decreasing.
-
Solar Energetic Particle Events and Associated Type II Radio Bursts from Different Source Regions
Statistical analysis of solar events shows type II radio burst starting frequencies vary by source region and anti-correlate with proton spectral indices, constraining SEP acceleration mechanisms.
- Counterintuitive Magnetic Connectivity and Energetic Particle Flux Differences among Nearby Spacecraft During the 2023 February 24 Solar Energetic Particle Event