Solar wind models from the chromosphere to 1 AU

Space Science Reviews

Volumn 172, Issue 1-4, 2012, Pages 89-121

  Hansteen, Viggo H ^a   Velli, Marco ^b  

^a UNIVERSITY OF OSLO   (Norway)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Energy conservation; Scaling laws; Solar wind acceleration; Solar wind origins; Thermal force

Indexed keywords

FAST SOLAR WINDS; FLOW SPEED; HIGHER ORDER MOMENTS; ION TEMPERATURE; MAGNETIC FIELD LINE; N-WAVES; PARALLEL BEAMS; PARTICLE EFFECT; PLASMA EXPANSION; SOLAR WIND ACCELERATION; THERMAL FORCES; THERMALLY DRIVEN; ULYSSES; UNIFIED SYSTEM; WIND MODELS; WIND STREAM;

ASTROPHYSICS; ELECTRIC FIELDS; ELECTRON TEMPERATURE; ENERGY CONSERVATION; MAGNETIC FIELDS; SCALING LAWS;

SOLAR WIND;

EID: 84869491687     PISSN: 00386308     EISSN: 15729672     Source Type: Journal    
DOI: 10.1007/s11214-012-9887-z     Document Type: Conference Paper

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