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/2248/356| Title: | Ca II K Emission from the Solar Chromosphere |
| Authors: | Sivaraman, K. R |
| Keywords: | Ca II K emission solar chromosphere |
| Issue Date: | 1986 |
| Publisher: | Indian Institute of Astrophysics, Bangalore |
| Citation: | Kodaikanal Observatory Bulletins Series A, Vol. 6, pp. 11-18 |
| Abstract: | The role of the Ca II K line as a reliable diagnostic of the chromospheric activity on the Sun is reviewed. The chromospheric structures seen in this line serve as good indicators of the photospheric magnetic structures and also mimic the morphological changes in the surface magnetic features associated with the solar cycle. Similar changes can be expected to take place in other sun-like stars and could therefore be used as a diagnostic for inferring the kind of structures of surface magnetic fields in them. |
| URI: | http://hdl.handle.net/2248/356 |
| ISSN: | 0374-3632 |
| Appears in Collections: | IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 ) |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Ca II K Emission From The Solar Chromosphere.pdf | 260.52 kB | Adobe PDF |  View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.