Other
Scientific paper
Sep 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..528...91m&link_type=abstract
ACCELERATION AND TRANSPORT OF ENERGETIC PARTICLES OBSERVED IN THE HELIOSPHERE: ACE 2000 Symposium. AIP Conference Proceedings, V
Other
Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays
Scientific paper
We investigate the solar origin and propagation of a series of well collimated energetic electron events measured in situ by the EPAM experiment on the ACE spacecraft. EPAM measures electrons in the energy of range of 40 to 300 keV over a wide range look directions and with better than 1 minute time resolution. During the events in our study, these particles are strongly collimated along the magnetic field. As such, these near-relativistic (beta=0.4-0.7) particles tend to be scatter free and their observed arrival at ACE provides a good estimate of the release time back to the Sun. We combine these observations with fast imaging of the solar corona in the meter wave domain provided by the Nançay radioheliograph and dynamic spectral information from the WAVES experiment on the WIND spacecraft. Together, this complement of observations of solar energetic particles events provides insight into the onset times and sites of particle acceleration in the low corona. .
Hawkins Eduard S.
Maia Dalmiro
Pick Monique
Roelof Edmond C.
No associations
LandOfFree
Coronal origin of particle events detected by EPAM: Multi-instrument observations 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 Coronal origin of particle events detected by EPAM: Multi-instrument observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Coronal origin of particle events detected by EPAM: Multi-instrument observations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1523541