JpGU-AGU Joint Meeting 2017

講演情報

[EE] 口頭発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM12] [EE] Space Weather, Space Climate, VarSITI

2017年5月23日(火) 13:45 〜 15:15 A01 (東京ベイ幕張ホール)

コンビーナ:片岡 龍峰(国立極地研究所)、Antti A Pulkkinen(NASA Goddard Space Flight Center)、草野 完也(名古屋大学宇宙地球環境研究所)、塩川 和夫(名古屋大学宇宙地球環境研究所)、座長:片岡 龍峰(国立極地研究所)

14:45 〜 15:00

[PEM12-38] GPS phase fluctuations associated with high speed flows in the cusp ionosphere

*Y. Wang1Qinghe Zhang1P. T. Jayachandran2Zanyang Xing1John Moen3J. M. Ruohoniemi4Richard Chadwick2Yuzhang Ma1Mark Lester5 (1.Shandong Univ.、2.Univ. of New Brunswick、3.Univ. of Oslo、4.Virginia Tech.、5.Univ. of Leicester)

Using ionospheric scintillation measurements from GPS receivers of Canadian High Arctic Ionospheric Network (CHAIN) and flows measured by both of Kapuskasing (KAP) and Saskatoon (SAS) SuperDARN radars, we found that near cusp region the GPS phase scintillations fluctuated mostly associated with the varied velocity of flows. After statistic study over a 3 year period (2013-2015), a surprising result will be presented in this work that it is nearly linear relationship between GPS phase fluctuations and flows around cusp region. On the contrary, the behavior of GPS amplitude scintillations is always quiet even with higher velocity of flows, which is obviously different from the manners of phase fluctuations. The two various different performance associated with high speed flows may caused by differentiated dependency of flows of their possible generation mechanisms. The results will be useful to further study the scintillation mechanisms and can help to improve the scintillation models in polar region.