Morphology, dynamics and plasma parameters of plumes and inter-plume regions in solar coronal holes

Astronomy and Astrophysics Review

Volumn 19, Issue 1, 2011, Pages

  Wilhelm, K ^a   Abbo, L ^c   Auchere F ^d   Barbey, N ^d   Feng, L ^a,b   Gabriel, A H ^d   Giordano, S ^c   Imada, S ^e   Llebaria, A ^f   Matthaeus, W H ^g   Poletto, G ^h   Raouafi, N E ⁱ   Suess, S T ^j   Teriaca, L ^a   Wang, Y M ^k  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b CHINESE ACADEMY OF SCIENCES   (China)

^c OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

^d UNIVERSITÉ PARIS SUD   (France)

^e JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^f OBSERVATOIRE DE MARSEILLE   (France)

^g UNIVERSITY OF DELAWARE   (United States)

^h INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

ⁱ JOHNS HOPKINS UNIVERSITY APPLIED PHYSICS LABORATORY   (United States)

^j NATIONAL SPACE SCIENCE AND TECHNOLOGY CENTER   (United States)

^k NAVAL RESEARCH LABORATORY   (United States)

more..

Author keywords

Corona; Coronal holes; Coronal plumes; Inter plume regions; Solar wind; Sun

Indexed keywords

CORONA; CORONAL HOLE; CORONAL PLUMES; CROSS SECTION; ELECTRON DENSITIES; GENERATION PROCESS; HIGH-SPEED; INTER-PLUME REGIONS; ION TEMPERATURE; MAGNETIC FIELD CONFIGURATIONS; NONTHERMAL; PHYSICAL CONDITIONS; PLASMA BULK; PLASMA PARAMETER; PLUME SIGNATURE; PLUME STRUCTURE; PROMINENT FEATURES; RELATIVE CONTRIBUTION; SOLAR PHENOMENA; SPACE SCIENCE; STRUCTURE AND DYNAMICS; THREE-DIMENSIONAL RECONSTRUCTION;

MAGNETIC FIELDS; PLASMA DENSITY; SOLAR WIND;

PLASMA DIAGNOSTICS;

EID: 80051511269     PISSN: 09354956     EISSN: None     Source Type: Journal    
DOI: 10.1007/s00159-011-0035-7     Document Type: Review

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