Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1763557 | Advances in Space Research | 2015 | 11 Pages |
Abstract
A new empirical model of the topside ionospheric density was developed to describe the measured topside profile accurately. This profiler is a composite of two separate layers of different ion species in the topside ionosphere, the O+ layer and the light-ions (H+ and He+) layer. The light-ions layer is characterized by an α-Chapman function with a linearly increasing scale height with altitude. This new model appears to perform the best as compared to five other typical topside profilers in representing data from ISIS-1&2 and Alouette-1&2 observations. We also analyzed the magnetic latitude dependence, seasonal variation, and day-night difference of the characteristic parameters of the light-ions layer during the magnetic quiet (Kp < 4) and low solar activity (f107 < 120 solar flux unit, sfu) period within magnetic latitudes from â60° to 90°. The statistical results show the expected different behaviors of light-ions and O+ parameters. In addition, the portion of the light-ion components contributing to the topside-ionospheric total electron content (TTEC) was studied also. The results suggest that the light ions make a great contribution to the TTEC, especially in magnetic low- and middle-latitudes at night.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Jie Zhu, Biqiang Zhao, Weixing Wan, Baiqi Ning, Shunrong Zhang,