Study of ionospheric scintillation during geomagnetic storms at equatorial anomaly region Bhopal

被引:1
作者
Rashmi, Gupta C. [1 ]
Choudhary, S. [1 ]
Gwal, A. K. [1 ]
机构
[1] AISECT Univ, Dept Phys, Ctr Earth & Space Plasma, Bhopal, India
关键词
GPS; Scintillation; Ionosphere; S4; DST; SPREAD-F;
D O I
10.1007/s12648-020-01781-9
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
GPS L-band signals get affected by ionospheric scintillation; as a result, satellite navigation too gets affected. The most extreme scintillation activity is expected to occur near the equatorial region during geomagnetic storms. The behavior and morphology of low-latitude ionosphere are different from the other latitudes. The space weather conditions in low latitude show different nature because of the geomagnetic field. Due to penetration of soft, high energetic particles, the plasma density increases, which is the main source of generation of ionospheric irregularities scintillation. GPS scintillation at low latitudes is primarily associated with equatorial spreadF. Equatorial spreadFis caused by ionospheric irregularities with a spatial spectrum extending from 100 km to less than 1 m. When GPS signals encounter the ionospheric irregularities of various sizes produced during high geomagnetic and solar activity, they undergo drastic changes in their phase and amplitude scintillation indices. The accuracy and reliability of GPS system get affected by scintillation. Also the atmosphere air molecule's content and deviation of electrons, protons, neutrons according to flow rate are observed. In the present paper, we have studied the scintillation activity at low-latitude station Bhopal.
引用
收藏
页码:1069 / 1077
页数:9
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