LaBonte, Barry J. (1978) Thick Target Models of Impulsive Chromospheric Flares. Big Bear Solar Observatory Publications . pp. 1-31. https://resolver.caltech.edu/CaltechAUTHORS:20120928-203218270
![[img]](https://authors.library.caltech.edu/style/images/fileicons/application_pdf.png)
|
PDF
- Published Version
See Usage Policy. 7MB |
Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20120928-203218270
Abstract
The most impulsive flares show large amplitude intensity variations in times of order 10 s. An attempt is made to reproduce the properties of these events with a model in which the heating of a static chromosphere by a nonthermal electron beam is balanced by thermal radiation cooling. The computed results suggest that the assumed static equilibrium may be achieved in some parts of the flares, and indicate improvements necessary for more accurate models of this type of flare.
| Item Type: | Article | ||||||
|---|---|---|---|---|---|---|---|
| Additional Information: | We thank R. Moore for useful discussions, and R. Canfield for other discussions on radiative cooling. This research was supported by NASA under grant NASA NGR 05 002 034 and NSF under grant ATM76-21132. | ||||||
| Group: | Big Bear Solar Observatory | ||||||
| Funders: |
| ||||||
| Other Numbering System: |
| ||||||
| Record Number: | CaltechAUTHORS:20120928-203218270 | ||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20120928-203218270 | ||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||
| ID Code: | 34570 | ||||||
| Collection: | CaltechAUTHORS | ||||||
| Deposited By: | Joy Painter | ||||||
| Deposited On: | 04 Oct 2012 21:28 | ||||||
| Last Modified: | 03 Oct 2019 04:20 |
Repository Staff Only: item control page
