A magnetic reconnection X-line extending more than 390 Earth radii in the solar wind

Nature

Volumn 439, Issue 7073, 2006, Pages 175-178

  Phan, T D ^a   Gosling, J T ^b   Davis, M S ^a   Skoug, R M ^c   Oieroset M ^a   Lin, R P ^a   Lepping, R P ^d   McComas, D J ^e   Smith, C W ^f   Reme, H ^g   Balogh, A ^h  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF COLORADO   (United States)

^c LOS ALAMOS NATIONAL LABORATORY   (United States)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

^e SOUTHWEST RESEARCH INSTITUTE   (United States)

^f University of New Hampshire   (United States)

^g IRAP   (France)

^h IMPERIAL COLLEGE LONDON   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

ASTROPHYSICS; BOUNDARY CONDITIONS; HIGH ENERGY PHYSICS; MAGNETOSPHERE; SPACECRAFT;

MAGNETIC ENERGY; MAGNETIC RECONNECTION; X-LINE;

MAGNETIC PROPERTIES;

SOLAR WIND;

ARTICLE; ASTRONOMY; ENERGY; FLOW RATE; MAGNETIC FIELD; MAGNETISM; PREDICTION; PRIORITY JOURNAL; QUANTITATIVE ANALYSIS; STEADY STATE;

EID: 30644475509     PISSN: 00280836     EISSN: 14764687     Source Type: Journal    
DOI: 10.1038/nature04393     Document Type: Article

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