메뉴 건너뛰기




Volumn 180, Issue 1-2, 1998, Pages 285-298

Spatial structure of solar coronal magnetic loops revealed by transient microwave brightenings

Author keywords

[No Author keywords available]

Indexed keywords


EID: 0032363023     PISSN: 00380938     EISSN: None     Source Type: Journal    
DOI: 10.1023/a:1005020207482     Document Type: Article
Times cited : (3)

References (14)
  • 4
    • 0042521156 scopus 로고
    • Solar Active Region Evolution: Comparing Models with Observation
    • K. S. Balasubramaniam and G. W. Simon (eds.)
    • Gopalswamy, N.: 1994, in K. S. Balasubramaniam and G. W. Simon (eds.), 'Solar Active Region Evolution: Comparing Models with Observation', ASP Conference Series, Vol. 68, p. 395.
    • (1994) ASP Conference Series , vol.68 , pp. 395
    • Gopalswamy, N.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.