Statistical study of soho/sumer full-sun images

European Space Agency, (Special Publication) ESA SP

Volumn , Issue 547, 2004, Pages 337-340

  Buchlin, Eric ^a,b   Vial, J C ^a   Lemaire, P ^a   Galtier, S ^a  

^a UNIVERSITÉ PARIS SUD   (France)

^b INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

COMPUTER SIMULATION; DATA REDUCTION; FUNCTIONS; HEAT RADIATION; METHOD OF MOMENTS; SOLAR ENERGY; STATISTICAL METHODS; SUN;

DATA SETS; FULL-SUN IMAGES; PIXEL STATISTICS; STRUCTURE FUNCTIONS;

IMAGE ANALYSIS;

EID: 18644373482     PISSN: 03796566     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Conference Paper

References (4)

1. Abramenko, V. I., Yurchyshyn, V. B., Wang, H., Spirock, T. J., and Goode, P. R. (2002). Scaling Behavior of Structure Functions of the Longitudinal Magnetic Field in Active Regions on the Sun. ApJ, 577, 487-495.
2. Aletti, V., Velli, M., Bocchialini, K., Einaudi, G., Georgoulis, M., and Vial, J.-C. (2000). Microscale structures on the quiet sun and coronal heating. ApJ, 544, 550-557.
3. Buchlin, E., Aletti, V., Galtier, S., Velli, M., Einaudi, G., and Vial, J.-C. (2003). A simplified numerical model of coronal energy dissipation based on reduced MHD. Astron. Astrophys., 406, 1061-1070.
4. Isliker, H., Anastasiadis, A., and Vlahos, L. (2000). MHD consistent cellular automata (CA) models - I. basic features. Astron. Astrophys., 363, 1134-1144.