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The possible importance of synchrotron/inverse compton losses to explain fast mm-wave and hard x-ray emission of a solar event
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Correia, E. Kaufmann, P. Zodivaz, A. M. Dennis, B. R. Costa, J. E. R. |
| Copyright Year | 1986 |
| Description | The solar burst of 21 May 1984, presented a number of unique features. The time profile consisted of seven major structures (seconds), with a turnover frequency of greater than or approximately 90 GHz, well correlated in time to hard X-ray emission. Each structure consisted of multiple fast pulses (0.1 seconds), which were analyzed in detail. A proportionality between the repetition rate of the pulses and the burst fluxes at 90 GHz and greater than or approximately 100 keV hard X-rays, and an inverse proportionality between repetition rates and hard X-ray power law indices were found. A synchrotron/inverse Compton model was applied to explain the emission of the fast burst structures, which appear to be possible for the first three or four structures. |
| File Size | 345690 |
| Page Count | 9 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19870012369 |
| Archival Resource Key | ark:/13960/t5jb11w1h |
| Language | English |
| Publisher Date | 1986-01-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Pulse Rate Time Dependence Solar Flares Millimeter Waves X Ray Spectra Flux Rate Solar Radiation Synchrotron Radiation Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
