Four Solar Orbiter interplanetary shocks show energetic particle pressure dominating upstream, indicating particle-mediated modification of collisionless shocks.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
MHD models predict that above 10 keV the solar magnetic field collimates plasma into high-latitude lobes, producing a factor of ~2 ENA enhancement at 80 keV that IMAP can detect.
citing papers explorer
-
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.
-
Prediction for IMAP: Revealing the Role of the Solar Magnetic Field in the Heliotail
MHD models predict that above 10 keV the solar magnetic field collimates plasma into high-latitude lobes, producing a factor of ~2 ENA enhancement at 80 keV that IMAP can detect.