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Volumn 330, Issue 6000, 2010, Pages 81-84

Identifying the driver of pulsating aurora

Author keywords

[No Author keywords available]

Indexed keywords

ATMOSPHERIC ELECTRICITY; AURORA; ELECTROMAGNETIC WAVE; ELECTRON; GROUND-BASED MEASUREMENT; MAGNETIC FIELD; POLAR REGION; SATELLITE IMAGERY; UPPER ATMOSPHERE;

EID: 77957368239     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1193186     Document Type: Article
Times cited : (274)

References (33)
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    • 77957340255 scopus 로고    scopus 로고
    • We also analyzed other events (table S1)
    • We also analyzed other events (table S1).
  • 25
    • 77957330402 scopus 로고    scopus 로고
    • note
    • c.
  • 26
    • 77957346997 scopus 로고    scopus 로고
    • note
    • The auroral intensity did not diminish following the decrease in the ECH intensity but stayed at a high level. This is attributable to the long lifetime (∼1 min) of excited oxygen atom at higher altitudes (32) due to the precipitation of lower-energy electrons (∼1 keV), as expected from resonance with ECH (11).
  • 33
    • 77957354794 scopus 로고    scopus 로고
    • note
    • This work was supported by NASA contract NAS5-02099, 9F007-046101; NSF grants ATM-0802843 and AGS-0840178; and a Research Fellowship from the Japan Society for the Promotion of Science. The French involvement (Search-coil magnetometer) on THEMIS is supported by CNES and CNRS.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.