Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/2653| Title: | Variability of the solar chromospheric network over the solar cycle |
| Authors: | Kariyappa, R Sivaraman, K. R |
| Keywords: | Calcium K Lines Line Shape Network Analysis Photosphere Solar Activity Correlation Coefficients Periodic Variations Solar Cycles |
| Issue Date: | Jun-1994 |
| Publisher: | Springer |
| Citation: | Solar Physics, Vol. 152, No. 1, pp. 139 - 144 |
| Abstract: | From a large sample of the Kodaikanal spectroheliograms in the Ca II K line we have studied the variations in the intensity of the network elements over two solar cycles and have estimated their contribution to the overall variability seen in the disk-averaged K line profiles. The relative contribution of the network elements and the bright points to the K-emission are of the order of 25% and 15% respectively. We have shown that the area of the network elements is anti-correlated with the solar activity, and it increases by about 24% during the solar minimum compared to the maximum period. |
| URI: | http://hdl.handle.net/2248/2653 |
| ISSN: | 0038-0938 |
| Appears in Collections: | IIAP Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Kariyappa R.pdf | 511.23 kB | Adobe PDF | ![]() View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.
