1971
DOI: 10.1007/978-94-010-3090-8_16
|View full text |Cite
|
Sign up to set email alerts
|

Equatorial Modulation in a Pulsating Aurora

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0

Year Published

1971
1971
1978
1978

Publication Types

Select...
3
1

Relationship

0
4

Authors

Journals

citations
Cited by 4 publications
(1 citation statement)
references
References 4 publications
0
1
0
Order By: Relevance
“…One of the most important characteristics of the auroral rapid variation is that the energy of the corresponding electrons is higher than that in more common aurora (EVANS, 1976;WHALEN et al, 1971;BRYANT et al, 1971;COURTIER et al, 1974;BRYANT et al, 1975;BROWN et al, 1976). The energy range of the corresponding electrons, in conjunction with the association of VLF chorus emissions and the association of geomagnetic pulsation as well, suggests that the coupling between energetic auroral electrons, VLF waves and HM waves in the magnetosphere plays an essential role in the region of after-effect.…”
Section: Summary and Discussionmentioning
confidence: 99%
“…One of the most important characteristics of the auroral rapid variation is that the energy of the corresponding electrons is higher than that in more common aurora (EVANS, 1976;WHALEN et al, 1971;BRYANT et al, 1971;COURTIER et al, 1974;BRYANT et al, 1975;BROWN et al, 1976). The energy range of the corresponding electrons, in conjunction with the association of VLF chorus emissions and the association of geomagnetic pulsation as well, suggests that the coupling between energetic auroral electrons, VLF waves and HM waves in the magnetosphere plays an essential role in the region of after-effect.…”
Section: Summary and Discussionmentioning
confidence: 99%