Physics
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsh42a..01l&link_type=abstract
American Geophysical Union, Fall Meeting 2006, abstract #SH42A-01
Physics
2111 Ejecta, Driver Gases, And Magnetic Clouds, 2114 Energetic Particles (7514), 2139 Interplanetary Shocks, 2162 Solar Cycle Variations (7536)
Scientific paper
Energetic particle observations at 1 AU provide us with a plethora of phenomena including solar energetic particle (SEP) events, energetic storm particle (ESP) events associated with the passage of transient interplanetary shocks, events associated with corotating interaction regions (CIRs), galactic cosmic rays (GCRs) and Jovian electron events. Previous missions traveling into the innermost part of the heliosphere, such as the Helios and the Mariner-10 spacecraft, provided data that allowed one to infer the radial component of the intensity gradients of all these phenomena within 1 AU of the Sun. I will review prior analysis of these observations taken closer to the Sun. These observations will allow us to determine how the energetic particle environment evolves with radial distance, and what the characteristics of the energetic particle phenomena encountered by future planned missions such as Sentinels and Solar Orbiter will be.
No associations
LandOfFree
Energetic particle environment in the innermost part of the heliosphere does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Energetic particle environment in the innermost part of the heliosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Energetic particle environment in the innermost part of the heliosphere will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-968422