1975
DOI: 10.1016/0032-0633(75)90164-6
|View full text |Cite
|
Sign up to set email alerts
|

Precipitation of > 115 kev protons in the evening and forenoon sectors in relation to the magnetic activity

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
4
1

Citation Types

0
12
0

Year Published

1977
1977
2018
2018

Publication Types

Select...
8
1

Relationship

0
9

Authors

Journals

citations
Cited by 31 publications
(12 citation statements)
references
References 20 publications
0
12
0
Order By: Relevance
“…A remarkable feature of energetic proton precipitation is their isotropic precipitation (with¯uxes being isotropic over the loss cone) which exists at any local time in any disturbance conditions (Hauge and Soraas, 1975;Lundblad et al, 1979) and forms the oval-shaped isotropic precipitation zone (Sergeev and Gvozdevsky, 1995). Recently this precipitation attracted much attention because of its potential importance for evaluation of magnetotail magnetic con®guration.…”
Section: Introductionmentioning
confidence: 99%
“…A remarkable feature of energetic proton precipitation is their isotropic precipitation (with¯uxes being isotropic over the loss cone) which exists at any local time in any disturbance conditions (Hauge and Soraas, 1975;Lundblad et al, 1979) and forms the oval-shaped isotropic precipitation zone (Sergeev and Gvozdevsky, 1995). Recently this precipitation attracted much attention because of its potential importance for evaluation of magnetotail magnetic con®guration.…”
Section: Introductionmentioning
confidence: 99%
“…They also noted that in some theoretical RC models the wave-particle scattering process is greatly simplified and therefore does not predict the strong pitch-angle diffusion postulated by Cornwall et al (1970) and observed by others (Hauge and Soraas, 1975;Soraas et al, 1999;Walt and Voss, 2001;Yahnina et al, 2000).…”
Section: Introductionmentioning
confidence: 91%
“…The steep equatorward boundary where the proton precipitation drops from 410 3 to o10 2 ðcm 2 s sr keVÞ À1 is approximately co-located with the equatorward boundary of isotropic precipitation. The IB moves to lower latitudes as the ring current and plasma sheet move earthward with increasing convection field (Sergeev et al, 1983;Gussenhoven et al, 1987;Hauge and Søraas, 1975;Hultqvist et al, 1976) thus it gives information about the temporal and spatial dynamics of the inner part of the ring current and plasma sheet. As explained in Section 2 and shown in Fig.…”
Section: Article In Pressmentioning
confidence: 99%