DSpace JSPUI
DSpace preserves and enables easy and open access to all types of digital content including text, images, moving images, mpegs and data sets
Learn More
Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/3390| Title: | Comparative morphology of EIT/SOHO images and HeII excitation |
| Authors: | Venkatakrishnan, P |
| Keywords: | Solar:line |
| Issue Date: | Jun-1999 |
| Publisher: | Kluwer Academic Publishers |
| Citation: | Solar Physics, Vol.187, No. 1, pp. 23 - 31 |
| Abstract: | Morphological differences between coronal images on the one hand, and a Hei image on the other, are used to demonstrate the independence of Heii excitation from coronal radiation. The distribution of magnetic flux is found to be more important for Heii excitation. Collisional excitation by non-thermal electrons produced in nano-flare events is proposed as the mechanism for Heii excitation. |
| Description: | Restricted Access |
| URI: | http://hdl.handle.net/2248/3390 |
| ISSN: | 0038-0938 |
| Appears in Collections: | IIAP Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Comparative morphology of EIT/SOHO images and HeII excitation Restricted Access | Restricted Access | 113.93 kB | Adobe PDF | View/Open Request a copy |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.