Abstract
Some twenty five solar events photographed at the National Observatory, Athens, have been used for the production of isophotal contours. Curves showing the development with time of the energy emitted by the events at several intensity levels have been obtained. Examples are shown and general remarks about measurements of flares are made.
Similar content being viewed by others
References
Boischot, A. and Clavelier, B.: 1968, Ann. Astrophys. 31, 445.
Castelli, J. P. and Aarons, J.: 1967, J. Geophys. Res. 72, 5491.
Donnely, R. F.: 1969, Astrophys. J. 158, L 165.
ESSA Res. Lab. Boulder, No. 306 (suppl.), Solar-Geophysical Data, February 1970.
Falciani, R., Righini, A., and Rigutti, M.: 1967, Z. Astrophys. 67, 481.
Falciani, R., Landini, M., Righini, A., and Rigutti, M.: 1968, in K.O. Kiepenheuer (ed.), ‘Structure and Development in Solar Active Regions’, IAU Symp. 35, 451.
Frost, K. J.: 1969, Astrophys. J. 158, L 159.
Gregorio, P. de, Falciani, R., Righini, A., and Rigutti, M.: 1966, Mem. Soc. Astron. Ital. 37, 807.
Gregorio, P. de, Falciani, R., Righini, A., and Rigutti, M.: 1967, Mem. Soc. Astron. Ital. 38, 33.
Kreplin, R. W., Moser, P. J., and Castelli, J. P.: 1969, XII COSPAR, Prague.
Mazzucconi, F. and Righini, A.: 1971, Solar Phys. 17, 174.
Parks, G. K. and Winckler, J. R.: 1969, Astrophys. J. 155, L 117.
Teske, R. G. and Thomas, L. J.: 1969, Solar Phys. 8, 348.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Falciani, R., Rigutti, M. & Macris, C.J. Analysis of some aspects of 25 chromospheric events. Sol Phys 26, 108–113 (1972). https://doi.org/10.1007/BF00155111
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF00155111