DIFFERENTIAL DOPPLER TRACKING FOR THE EQUATORIAL ANOMALY CRESTS OF THE IONOSPHERE

Liu Xuan-mou; Huang Tian-xi; Liu Rong-dao

doi:10.11728/cjss1989.01.052

Volume 9 Issue 1

Jan. 1989

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Article Navigation > Chinese Journal of Space Science > 1989 > 9(1): 52-57

Liu Xuan-mou, Huang Tian-xi, Liu Rong-dao. DIFFERENTIAL DOPPLER TRACKING FOR THE EQUATORIAL ANOMALY CRESTS OF THE IONOSPHERE[J]. Chinese Journal of Space Science, 1989, 9(1): 52-57. doi: 10.11728/cjss1989.01.052

Citation:

Liu Xuan-mou, Huang Tian-xi, Liu Rong-dao. DIFFERENTIAL DOPPLER TRACKING FOR THE EQUATORIAL ANOMALY CRESTS OF THE IONOSPHERE[J]. Chinese Journal of Space Science, 1989, 9(1): 52-57. doi: 10.11728/cjss1989.01.052

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DIFFERENTIAL DOPPLER TRACKING FOR THE EQUATORIAL ANOMALY CRESTS OF THE IONOSPHERE

doi: 10.11728/cjss1989.01.052 cstr: 32142.14.cjss1989.01.052

Department of Space Physics, Wuhan University

Received Date: 1988-01-26
Rev Recd Date: 1900-01-01
Publish Date: 1989-01-24

Abstract

Abstract

In this paper, the differential Doppler measurements for the equatorial anomaly crests in Wuhan (30.5°N, 114.4°E) is presented. The study of the experimental data indicates that the equatorial anomaly crests in the Far East is situated somewhere between Changsa (28.1°N, 113.0°E) and Guangzhou (23.2°N, 113.3°E). The northern hump of the equatorial anomaly is mostly between Hengyang (26.8°N, 112.5°E) and Yingde (24.2°N, 113°E). Some useful results about hump behaviour are also given.