TY - JOUR
T1 - ERG - A small-satellite mission to investigate the dynamics of the inner magnetosphere
AU - Shiokawa, K.
AU - Seki, K.
AU - Miyoshi, Y.
AU - Ieda, A.
AU - Ono, T.
AU - Iizima, M.
AU - Nagatsuma, T.
AU - Obara, T.
AU - Takashima, T.
AU - Asamura, K.
AU - Kasaba, Y.
AU - Matsuoka, A.
AU - Saito, Y.
AU - Saito, H.
AU - Hirahara, M.
AU - Tonegawa, Y.
AU - Toyama, F.
AU - Tanaka, M.
AU - Nose, M.
AU - Kasahara, Y.
AU - Yumoto, K.
AU - Kawano, H.
AU - Yoshikawa, A.
AU - Ebihara, Y.
AU - Yukimatsu, A.
AU - Sato, N.
AU - Watanabe, S.
PY - 2006
Y1 - 2006
N2 - The Earth's inner magnetosphere (inside 10 Re) is a region where particle energy increases to the relativistic energy range. This region is very important as a laboratory where high-energy particle acceleration can be directly measured in a dipolar field configuration, as well as for human activities in space including space weather prediction. Despite abundant in situ satellite measurements, this region has been "missing" because of several difficulties arising from the measurements, such as high-energy particle contamination of low-energy particle measurement, protection against the possible incidence of radiation belt particles on the satellite, and the difficulties of measuring three-dimensional particles over a broad energy range, from a few electron volts to more than 10 MeV. In this paper, we address important scientific topics and propose a possible configuration of small satellites termed Energization and Radiation in Geospace (ERG), which would provide new insights into the dynamics of the inner magnetosphere and strongly contribute to the International Living With a Star project.
AB - The Earth's inner magnetosphere (inside 10 Re) is a region where particle energy increases to the relativistic energy range. This region is very important as a laboratory where high-energy particle acceleration can be directly measured in a dipolar field configuration, as well as for human activities in space including space weather prediction. Despite abundant in situ satellite measurements, this region has been "missing" because of several difficulties arising from the measurements, such as high-energy particle contamination of low-energy particle measurement, protection against the possible incidence of radiation belt particles on the satellite, and the difficulties of measuring three-dimensional particles over a broad energy range, from a few electron volts to more than 10 MeV. In this paper, we address important scientific topics and propose a possible configuration of small satellites termed Energization and Radiation in Geospace (ERG), which would provide new insights into the dynamics of the inner magnetosphere and strongly contribute to the International Living With a Star project.
KW - Inner magnetosphere
KW - Magnetic storm
KW - Radiation belt
KW - Small satellite mission
UR - http://www.scopus.com/inward/record.url?scp=33846089744&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=33846089744&partnerID=8YFLogxK
U2 - 10.1016/j.asr.2005.05.089
DO - 10.1016/j.asr.2005.05.089
M3 - Article
AN - SCOPUS:33846089744
SN - 0273-1177
VL - 38
SP - 1861
EP - 1869
JO - Advances in Space Research
JF - Advances in Space Research
IS - 8
ER -