Comparing Equatorial Plasma Irregularities across Scale Sizes with GOLD and COSMIC

Jeffrey Klenzing; Alexa Jean Halford; Jonathon Smith; Carlos Martinis

講演情報

[E] 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-EM20] Recent Advances in Ionosphere Observation and Modeling through New Observation Opportunities

コンビーナ:CHIYEN LIN(Center for Astronautical Physics and Engineering, National Central University, TAIWAN)、Yen-Jung Wu(Space Sciences Laboratory, University of California, Berkeley)、Yang-Yi Sun(China University of Geosciences)、Charles Lin(Department of Earth Sciences, National Cheng Kung University)

[PEM20-03] Comparing Equatorial Plasma Irregularities across Scale Sizes with GOLD and COSMIC

*Jeffrey Klenzing¹、Alexa Jean Halford¹、Jonathon Smith^1,2、Carlos Martinis³ (1.NASA Goddard Space Flight Center、2.Catholic University of America、3.Boston University)

キーワード：plasma irregularities, plasma bubbles, scintillation

Near the geomagnetic equator, large depleted plumes of plasma (whimsically referred to as “bubbles”) can form when bottomside ionospheric plasma is lifted up hundreds of kilometers, piercing through the ionospheric layer. This uplift is caused by a Rayleigh-Taylor instability in the bottomside ionosphere, which can grow over the course of several hours. These meso-scale structures (10s to 100s of km) can lead to the formation of fine-scale (10s to 100s of m) plasma irregularities in the vicinity of large plasma density gradients. These smaller scale structures are important because they are of the right scale size to interfere with GPS signals. This study will compare the formation times of the meso-scale bubbles from space-borne airglow images from GOLD with the fine-scale S4 measurements from the COSMIC spacecraft.