Mahajan, K. K. (1967) 10.7 cm-Solar radio flux and ionospheric temperatures Journal of Atmospheric and Terrestrial Physics, 29 (9). pp. 1153-1158. ISSN 0021-9169
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Official URL: http://www.sciencedirect.com/science/article/pii/0...
Related URL: http://dx.doi.org/10.1016/0021-9169(67)90147-X
Abstract
Electron and ion temperatures, derived from backscatter spectra, are examined during the current rising phase of solar activity. There is a strong positive correlation between the 10·7 cm-solar radio flux and night-time ion and electron temperatures, the temperature increase being about 3·4° K for each unit increase of 1× 10-22 W/m2 per c/s bandwidth in S̅10.7. Any correlation of the noontime electron temperature, and the noontime ion temperature for heights above 400 km, with the 10·7 cm-solar flux, if present, is masked by the more predominant effect associated with the wide day-to-day electron density variations.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to Elsevier Science. |
| ID Code: | 75757 |
| Deposited On: | 27 Dec 2011 13:08 |
| Last Modified: | 27 Dec 2011 13:08 |
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