2004
DOI: 10.5194/angeo-22-1297-2004
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Multiple discrete-energy ion features in the inner magnetosphere: 9 February 1998, event

Abstract: Abstract. Multiple discrete-energy ion bands observed by the Polar satellite in the inner magnetosphere on 9 February 1998 were investigated by means of particle simulation with a realistic model of the convection electric field. The multiple bands appeared in the energy vs. L spectrum in the 1-100 keV range when Polar traveled in the heart of the ring current along the outbound and inbound paths. We performed particle tracing, and simulated the energy vs. L spectra of proton fluxes under the dipole magnetic f… Show more

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Cited by 38 publications
(57 citation statements)
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“…However, this interpretation is unlikely to explain the bands observed by CODIF on the 11 April 2002, since no dipolarization signature is observed during the 8 h prior to the event (AE index very low). Using a realistic electric and magnetic field model (with solar wind data as input), Ebihara et al (2004) simulated the same event as Li et al (2000). They were thus able to conclude that these bands were most likely to be produced by two combined process, i.e.…”
Section: Multi-nose Not Reproduced By the Modelmentioning
confidence: 89%
See 4 more Smart Citations
“…However, this interpretation is unlikely to explain the bands observed by CODIF on the 11 April 2002, since no dipolarization signature is observed during the 8 h prior to the event (AE index very low). Using a realistic electric and magnetic field model (with solar wind data as input), Ebihara et al (2004) simulated the same event as Li et al (2000). They were thus able to conclude that these bands were most likely to be produced by two combined process, i.e.…”
Section: Multi-nose Not Reproduced By the Modelmentioning
confidence: 89%
“…However, using a realistic large scale electric field model, our simulations couldn't reproduce the bands observed by CODIF during the 11 April 2002 event. As a consequence, the interpretation made by Ebihara et al (2004) is unlikely to explain CODIF structures in that case. Moreover, using real LANL/MPA data as input in our model, no change in the source distribution function was able to explain the creation of low energy structures.…”
Section: Multi-nose Not Reproduced By the Modelmentioning
confidence: 95%
See 3 more Smart Citations