The Motions of the Hard X‐Ray Sources in Solar Flares: Images and Statistics
- 1 September 2005
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 630 (1), 561-572
- https://doi.org/10.1086/431918
Abstract
No abstract availableThis publication has 22 references indexed in Scilit:
- Hard X-Ray Source Motions in the 2002 July 23 Gamma-Ray FlareThe Astrophysical Journal, 2003
- Evolution of Conjugate Footpoints inside Flare Ribbons during a Great Two‐Ribbon Flare on 2001 April 10The Astrophysical Journal, 2003
- Spectral and Spatial Variations of Flare Hard X-ray FootpointsSolar Physics, 2002
- Ideal spatial adaptation by wavelet shrinkageBiometrika, 1994
- The Hard X-ray Telescope (HXT) for the SOLAR-A missionSolar Physics, 1991
- Solar surface velocity fields determined from small magnetic featuresSolar Physics, 1990
- Magnetic reconnection on the separator as a cause of a two-ribbon flareAdvances in Space Research, 1990
- Photospheric vortex flows as a cause for two-ribbon flares: A topological modelSolar Physics, 1988
- Image reconstruction from incomplete and noisy dataNature, 1978
- Restoring with Maximum Likelihood and Maximum Entropy*Journal of the Optical Society of America, 1972