Abstract
Time-intensity profiles of 20-126 keV ions across interplanetary shocks are studied using data from ACE and Wind to determine the dependence of the profiles on spacecraft separation. Each pair of time-intensity profiles is examined to determine whether or not the same features (flat, classic energetic storm particle (ESP) rise, spikes, step functions, or complex patterns) are seen at both spacecraft. The persistence of particle profile patterns has a scale length in the plane of the shock of ∼2.9 Mkm, but the scale length along the shock normal direction is not well determined.
| Original language | English (US) |
|---|---|
| Article number | A12107 |
| Journal | Journal of Geophysical Research: Space Physics |
| Volume | 111 |
| Issue number | 12 |
| DOIs | |
| State | Published - Dec 1 2006 |
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ASJC Scopus subject areas
- Geophysics
- Space and Planetary Science
Cite this
Variability of low-energy ion flux profiles on interplanetary shock fronts. / Neugebauer, M.; Giacalone, Joe; Chollet, E.; Lario, D.
In: Journal of Geophysical Research: Space Physics, Vol. 111, No. 12, A12107, 01.12.2006.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - Variability of low-energy ion flux profiles on interplanetary shock fronts
AU - Neugebauer, M.
AU - Giacalone, Joe
AU - Chollet, E.
AU - Lario, D.
PY - 2006/12/1
Y1 - 2006/12/1
N2 - Time-intensity profiles of 20-126 keV ions across interplanetary shocks are studied using data from ACE and Wind to determine the dependence of the profiles on spacecraft separation. Each pair of time-intensity profiles is examined to determine whether or not the same features (flat, classic energetic storm particle (ESP) rise, spikes, step functions, or complex patterns) are seen at both spacecraft. The persistence of particle profile patterns has a scale length in the plane of the shock of ∼2.9 Mkm, but the scale length along the shock normal direction is not well determined.
AB - Time-intensity profiles of 20-126 keV ions across interplanetary shocks are studied using data from ACE and Wind to determine the dependence of the profiles on spacecraft separation. Each pair of time-intensity profiles is examined to determine whether or not the same features (flat, classic energetic storm particle (ESP) rise, spikes, step functions, or complex patterns) are seen at both spacecraft. The persistence of particle profile patterns has a scale length in the plane of the shock of ∼2.9 Mkm, but the scale length along the shock normal direction is not well determined.
UR - http://www.scopus.com/inward/record.url?scp=33947692700&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=33947692700&partnerID=8YFLogxK
U2 - 10.1029/2006JA011832
DO - 10.1029/2006JA011832
M3 - Article
AN - SCOPUS:33947692700
VL - 111
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
SN - 2169-9380
IS - 12
M1 - A12107
ER -