Magnetic field evolution of AR 0486 before and after the X17 flare on October 28, 2003

European Space Agency, (Special Publication) ESA SP

Volumn , Issue 575, 2004, Pages 519-522

  Regnier S ^a   Fleck, B ^a  

^a EUROPEAN SPACE AGENCY   (Netherlands)

Author keywords

Flares; Magnetic fields; Sun:xorona

Indexed keywords

COMPUTATIONAL METHODS; EXTRAPOLATION; GEOMETRY; MAGNETIC FIELDS; TOPOLOGY; VECTORS;

FLARES; MAGNETIC ENERGY; SUN:CORONA; SUNSPOT;

SUN;

EID: 22144484511     PISSN: 03796566     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Conference Paper

References (6)

1. Amari, T., Aly, J. J., Luciani, J. F., Boulmezaoud, T. Z., Mikic, Z., 1997, Sol. Phys., 174, 129
2. Amari, T., Boulmezaoud, T. Z., Mikic, Z., 1999, A&A, 350, 1051
3. Labonte, B. J., Mickey, D. L., Leka, K. D., 1999, Sol. Phys., 189, 1
4. Lin, H., Kuhn, J.R., Coulter, R., 2004, ApJ 613, L177
5. Mickey, D. L., Canfield, R. C., Labonte, B. J., Leka, K. D., Waterson, M. F., Weber, H. M., 1996, Sol. Phys., 168, 229
6. Régnier, S., Amari, T., Kersalé, E., 2002, A&A, 392, 1119