Saturation of Nonthermal Hard X‐Ray Emission in Solar Flares

Flare Solar flare Saturation (graph theory)
DOI: 10.1086/520331 Publication Date: 2007-08-31T19:39:45Z
ABSTRACT
We consider a number of flares spanning range magnitudes over two decades in GOES soft X-ray luminosity and demonstrate an observational confirmation the saturation nonthermal hard photon flux large solar flares. Using unprecedented spectral spatial resolution RHESSI telescope, we find that integrated above 20 keV asymptotically approaches limiting value with increasing flare intensity, suggesting production for high electron-beam fluxes This result is strengthened by considering each as aggregation multiple fiducial energy release events identified using RHESSI. argue sets transition from Coulomb collisions to return current ohmic dissipation dominating losses increase.
SUPPLEMENTAL MATERIAL
Coming soon ....
REFERENCES (32)
CITATIONS (36)
EXTERNAL LINKS
PlumX Metrics
RECOMMENDATIONS
FAIR ASSESSMENT
Coming soon ....
JUPYTER LAB
Coming soon ....