Topside electron temperature models for low and high solar activity

Pandey, V. K. ; Sethi, N. K. ; Mahajan, K. K. (2004) Topside electron temperature models for low and high solar activity Advances in Space Research, 33 (6). pp. 959-962. ISSN 0273-1177

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Official URL: http://www.sciencedirect.com/science/article/pii/S...

Related URL: http://dx.doi.org/10.1016/j.asr.2003.07.011

Abstract

It is now well known that in the topside ionosphere thermal conduction from the protonosphere becomes the dominant factor over the heating and loss terms in shaping the ionospheric electron temperature (Te) profile. By analyzing a limited database of incoherent scatter (IS) Te measurements, Mahajan and Pandey [J. Geophys. Res. 85 (1980) 213] reported a correlation between the electron heat flux and electron density in the topside ionosphere. Since attention has been steadily mounting for the empirical modeling of Te, we now exploit the large database of IS measurements of Te and Ne at Arecibo during 1989-1990 (high solar activity), as well as during 1975-1976 (low solar activity) for this purpose. We again find a functional relationship between heat flux and electron density in the topside ionosphere during both the solar activities. These functional relationships are used to generate topside Te profiles.

Item Type:Article
Source:Copyright of this article belongs to Elsevier Science.
Keywords:Ionosphere; Topside Ionosphere; Heat Flux; Electron Density; High Solar Activity
ID Code:75825
Deposited On:27 Dec 2011 12:54
Last Modified:27 Dec 2011 12:54

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