37 citations · 188 across the 13 of their papers we have counts for
13 papers
Variability of interplanetary shock and associated energetic particle properties as a function of the time window around the shock
Kimberly Moreland, Maher Dayeh, Gang Li +3
We study the effect of sampling windows on derived shock and associated energetic storm particle (ESP) properties in 296 fast-forward interplanetary shocks using ACE measurements a…
MMS Observations of the Velocity-Space Signature of Shock-Drift Acceleration
Peter Montag, Gregory Howes, Daniel McGinnis +3
Collisionless shocks play a key role in the heliosphere at planetary bow shocks by governing the conversion of the upstream bulk kinetic energy of the solar wind flow to other form…
Solar Cycle Variation of 0.3-1.29 MeV/nucleon Heavy Ion Composition during Quiet Times near 1 AU in Solar Cycles 23 and 24
B. L. Alterman, Mihir I. Desai, Maher A. Dayeh +2
We report on the annual variation of quiet-time suprathermal ion composition for C through Fe using Advanced Composition Explorer (ACE)/Ultra-Low Energy Isotope Spectrometer (ULEIS…
Modelling Solar Energetic Neutral Atoms from Solar Flares and CME-driven Shocks
Gang Li, Albert Y. Shih, Robert C. Allen +5
We examine the production of energetic neutral atoms (ENAs) in solar flares and CME-driven shocks and their subsequent propagation to 1 au. Time profiles and fluence spectra of sol…
Variable Ion Compositions of Solar Energetic Particle Events in the Inner Heliosphere: A Field-line Braiding Model with Compound Injections
Fan Guo, Lulu Zhao, Christina M. S. Cohen +8
We propose a model for interpreting highly variable ion composition ratios in solar energetic particles (SEP) events recently observed by Parker Solar Probe (PSP) at a…
Direct Evidence for Magnetic Reflection of Heavy Ions from High Mach Number Collisionless Shocks
Hadi Madanian, Steven J. Schwartz, Stephen A. Fuselier +5
Strong shocks in collisionless plasmas, such as supernovae shocks and shocks driven by coronal mass ejections, are known to be a primary source of energetic particles. Due to their…