日本地球惑星科学連合2019年大会

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-EM11] Dynamics of Magnetosphere and Ionosphere

2019年5月30日(木) 09:00 〜 10:30 A04 (東京ベイ幕張ホール)

コンビーナ:中溝 葵(情報通信研究機構 電磁波研究所)、尾崎 光紀(金沢大学理工研究域電子情報学系)、藤本 晶子(九州工業大学)、堀 智昭(名古屋大学宇宙地球環境研究所)、座長:中野 慎也(情報・システム研究機構 統計数理研究所)、野和田 基晴(山東大学)

10:00 〜 10:15

[PEM11-11] Magnetic Field Oscillations Observed by Swarm Satellites in the Nightside Upper Ionosphere During Low-latitude Pi2 Pulsations

*Khan-Hyuk Kim1Jae-Hee Park1 (1.School of Space Research, Kyung Hee Univ.)

キーワード:Pi2 pulsation

Pi2-associated geomagnetic oscillations in the nighside upper ionosphere are studied using magnetic field data acquired by low-Earth orbiting multispacecraft Swarm and at the low-latitude Bohyun (BOH) station located at magnetic shell of L = 1.3 on 22 October 2014. Four Pi2 events were identified from the BOH data near midnight (MLT = 1.5) while Swarm A, B, and C spacecraft were orbiting on the nightside (MLT = 21-22) upper ionosphere from 70° to --60° in magnetic latitude (MLAT) at 450-500 km altitudes. It is found that the horizontal H component of BOH data is well correlated with the radial (Bx) and compressional (Bz) components of ionospheric magnetic fields when Swarm spacecraft were at |MLAT| < 30°. Both Bx and Bz components exhibit in phase or out of phase with the BOH H oscillations depending on the location of the spacecraft (i.e., in the Northern Hemisphere or in the Southern Hemisphere). This indicates that Pi2-associated magnetic oscillation in the ionosphere is the consequence of field line displacement that is symmetric or odd mode about the magnetic equator. We also find that stationary magnetic field perturbation, which is similar to Pi2 oscillation but not associated Pi2 signals, in the upper ionosphere near magnetic equator. A statistical analysis for the global distribution of static/spatial magnetic field perturbations using low-latitude Pi2 oscillation as a reference is a subject of future work.