Rapid variability has been found in two active region coronal loops observed by the X-ray Polychromator (XRP) and the Hard X-ray Imaging Spectrometer (HXIS) onboard the Solar Maximum Mission (SMM). There appear to be surprisingly few observations of the short-time scale behavior of hot loops, and the evidence presented herein lends support to the hypothesis that coronal heating may be impulsive and driven by flaring.
Dynamical behaviour in coronal loops
Advances in Space Research ; 6 , 6 19
1986-01-01
Miscellaneous
No indication
English
Impulsive Heating in Coronal Loops
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