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X-ray Emission Characteristics of Flares Associated with CMEs
X-ray flares rise time duration peak intensity CME linear velocity acceleration
2010/9/16
We present the study of 20 solar flares observed by “Solar X-ray Spectrometer (SOXS)” mission during November 2003 to December 2006 and found associated with coronal mass ejections (CMEs) seen by LASC...
UV Diagnostics for the Energy Budget of Flares and CMEs
Sun corona flares coronal mass ejections
2010/9/16
Solar flares and coronal mass ejections convert large amounts of magnetic free energy into thermal, kinetic and potential energies, and into energy of non-thermal particles. The partitioning among the...
X-ray Emission from Solar Flares
Solar flares X-ray detectors X-ray line emission and continuum break energy microflares
2010/9/15
Solar X-ray Spectrometer (SOXS), the first space-borne solar astronomy experiment of India was designed to improve our current understanding of X-ray emission from the Sun in general and solar flares ...
X-ray Emission Characteristics of Flares Associated with CMEs
X-ray flares: rise time duration peak intensity CME:linear velocity acceleration
2009/5/6
We present the study of 20 solar flares observed by “Solar
X-ray Spectrometer (SOXS)” mission during November 2003 to December
2006 and found associated with coronal mass ejections (CMEs) seen by
...