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Volumn 516, Issue 18, 2010, Pages

Coronal hole boundaries evolution at small scales: II. XRT view. Can small-scale outflows at CHBs be a source of the slow solar wind?

Author keywords

methods: data analysis; methods: observational; Sun: atmosphere; Sun: corona

Indexed keywords

AUTOMATED PROCEDURES; BRIGHT POINTS; CORONAL BRIGHT; CORONAL HOLE; FIELD STRUCTURES; FINE STRUCTURES; HIGH RESOLUTION; LOOP STRUCTURE; MAGNETIC FIELD LINE; MAGNETIC RECONNECTIONS; METHODS:DATA ANALYSIS; METHODS:OBSERVATIONAL; QUIET SUN; SMALL SCALE; SOLAR CORONA; SUN: ATMOSPHERE; SUN: CORONA; VISUAL ANALYSIS; X RAY TELESCOPE; X-RAY TEMPERATURES;

EID: 77957826675     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (71)

References (34)
  • 17
    • 0002729622 scopus 로고
    • Saito, K. 1965, PASJ, 17, 1
    • (1965) PASJ , vol.17 , pp. 1
    • Saito, K.1
  • 26
    • 0040595283 scopus 로고    scopus 로고
    • in Cool Stars, Stellar Systems, and the Sun, ed. R. Pallavicini, & A. K. Dupree
    • Von Steiger, R. 1996, in Cool Stars, Stellar Systems, and the Sun, ed. R. Pallavicini, & A. K. Dupree, ASP Conf. Ser., 109, 491
    • (1996) ASP Conf. Ser. , vol.109 , pp. 491
    • Von Steiger, R.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.