VizieR Online Data Catalog: Global energetics of solar flares. IX. (Aschwanden, 2019)
Abstract
We analyzed the same data set of 173 solar flares presented in PaperI, which includes all M- and X-class flares observed with the Solar Dynamics Observatory (SDO) during the first 3.5yr of the mission (2010 June 1 to 2014 January 31). We use the 45s line-of-sight magnetograms from Helioseismic and Magnetic Imager (HMI/SDO) and make use of all coronal Extreme Ultraviolet Variability (EUV) channels of Atmospheric Imaging Assembly (AIA/SDO) (in the six wavelengths 94, 131, 171, 193, 211, 335Å), in the temperature range of T~0.6-16MK. The spatial resolution is ~1.6" for AIA, and the pixel size of HMI is 0.5".
(1 data file).- Publication:
-
VizieR Online Data Catalog
- Pub Date:
- March 2021
- DOI:
- 10.26093/cds/vizier.18850049
- Bibcode:
- 2021yCat..18850049A
- Keywords:
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- Sun;
- Stars: flare;
- Magnetic fields;
- Ultraviolet