Abstract
We examine the spatial distribution of hard X-ray bremsstrahlung emission from an electron-heated target, using a self-consistent calculation of the hydrodynamic response of the atmosphere to heating by the electrons to compute the density-height structure of the target atmosphere at various times. In this way we derive the predicted temporal evolution of the hard X-ray spatial structure at various photon energies. We compare our results with existing observations from the Solar Maximum Mission Hard X-Ray Imaging Spectrometer and give a prognosis for the type of structure to be expected at the sub-arc second resolution planned for future instrumentation.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
