Correlation between coronal hole and quiet Sun intensities: Evidence for continuous reconnection

Astronomy and Astrophysics

Volumn 432, Issue 1, 2005, Pages 341-347

  Raju, K P ^a,c   Bromage, B J I ^a   Chapman, S A ^a   Del Zanna, G ^b  

^a UNIVERSITY OF CENTRAL LANCASHIRE   (United Kingdom)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c INDIAN INSTITUTE OF ASTROPHYSICS   (India)

Author keywords

Sun: Corona; Sun: Transition region

Indexed keywords

ASTROPHYSICS; CARRIER CONCENTRATION; CORRELATION METHODS; MAGNETIC FIELDS; PROBABILITY; SIGNAL TO NOISE RATIO; SOLAR RADIATION;

CHROMOSPHERE; CORONAL HOLES; SUN: CORONA; SUN: TRANSITION REGION;

SUN;

EID: 14844298706     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20042179     Document Type: Article

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