JpGU-AGU Joint Meeting 2017

講演情報

[EE] ポスター発表

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-EM14] [EE] Dynamics in magnetosphere and ionosphere

2017年5月20日(土) 10:45 〜 12:15 ポスター会場 (国際展示場 7ホール)

コンビーナ:堀 智昭(東京大学大学院理学系研究科)、田中 良昌(国立極地研究所)、中溝 葵(情報通信研究機構 電磁波計測研究所)、尾崎 光紀(金沢大学理工研究域電子情報学系)

[PEM14-P16] Reconstruction of Plasmaspheric Density Distributions by Applying a Tomography Technique to Jason-1 plasmaspheric TEC Measurements

*Eunsol Kim1Yongha Kim1Geonhwa Jee2 (1.Chungnam National University、2.Korea Polar Research Institute)

キーワード:Plasmasphere, Tomography, Total Electron Content, GPS

GPS receiver onboard Jason-1 satellite provides the measurements of plasmaspheric total electron content (pTEC) between the altitudes of Jason-1 and GPS satellites (1,336 and 20,200 km, respectively). We developed a tomography algorithm and applied it to the Jason-1 pTEC data to reconstruct the plasmaspheric density distributions. To invert the observed pTECs into the vertical distribution of plasmaspheric electron density, we adopted a multiplicative algebraic reconstruction technique (MART) with an initial density from Huang et al. (2004). The reconstruction of the plasmaspheric density distribution was performed on Indian ( ), Pacific ( ), and Atlantic ( ) longitudinal planes during the periods of high solar activity ( ) and low geomagnetic activity ( ) from 2002 to 2005. It is found that the reconstructed density distribution displays general climatological characteristics of the plasmasphere. For all three longitudinal sectors, the reconstructed distributions show weak diurnal variations being greater during daytime (09 – 15 LT) than nighttime (21 – 03 LT). In the Atlantic sector, the reconstructed plasmaspheric density exhibits an annual anomaly (higher density in December than in June), while it was not apparent in the other longitude sectors. By fitting the reconstructed density profiles, we derived the empirical profiles of equatorial plasmaspheric density for four seasons (March, June, September, and December) and for three longitude sectors. The empirical profiles display the diurnal variation and the annual anomaly, and significantly differ from those obtained from other kinds of plasmaspheric measurements.