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Thermal evolution and radiative output of solar flares observed by the euv variability experiment (eve)
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Milligan, R. O. Woods, T. N. Chamberlin, P. C. |
| Copyright Year | 2012 |
| Description | This paper describes the methods used to obtain the thermal evolution and radiative output during solar flares as observed by the Extreme u ltraviolet Variability Experiment (EVE) onboard the Solar Dynamics Ob servatory (SDO). Presented and discussed in detail are how EVE measur ements, due to its temporal cadence, spectral resolution and spectral range, can be used to determine how the thermal plasma radiates at v arious temperatures throughout the impulsive and gradual phase of fla res. EVE can very accurately determine the radiative output of flares due to pre- and in-flight calibrations. Events are presented that sh ow the total radiated output of flares depends more on the flare duration than the typical GOES X-ray peak magnitude classification. With S DO observing every flare throughout its entire duration and over a la rge temperature range, new insights into flare heating and cooling as well as the radiative energy release in EUV wavelengths support exis ting research into understanding the evolution of solar flares. |
| File Size | 813187 |
| Page Count | 22 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20120013207 |
| Archival Resource Key | ark:/13960/t9q28x123 |
| Language | English |
| Publisher Date | 2012-03-06 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Solar Flares Solar Radiation Extreme Ultraviolet Radiation Sun Variability Solar Observatories Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |