Nonradial and nonpolytropic astrophysical outflows VII. Fitting ULYSSES solar wind data during minimum

Astronomy and Astrophysics

Volumn 432, Issue 2, 2005, Pages 687-698

  Sauty, C ^a   Lima, J J G ^b,c   Iro, N ^a   Tsinganos, K ^d  

^a OBSERVATOIRE DE PARIS   (France)

^b CENTRO DE ASTROFÍSICA   (Portugal)

^c UNIVERSITY OF PORTO   (Portugal)

^d UNIVERSITY OF ATHENS   (Greece)

Author keywords

Magnetohydrodynamics (MHD); Solar wind; Stars: winds, outflows; Sun: Corona; Sun: Magnetic fields

Indexed keywords

COMPUTER SIMULATION; HEATING; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; PROTONS; VELOCITY MEASUREMENT; WIND;

NONPOLYTROPIC ASTROPHYSICAL OUTFLOWS; OUTFLOWS; SOLAR WIND DATA; STARS: WINDS;

SOLAR SYSTEM;

EID: 15244358437     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041606     Document Type: Article

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