JpGU-AGU Joint Meeting 2020

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)

[PEM20-02] Recent Insights into the Thermosphere-Ionosphere Response to External Forcing from the Global-scale Observations of the Limb and Disk (GOLD) Mission

★Invited Papers

*Richard Eastes1 (1.Laboratory for Atmospheric and Space Physics)

キーワード:ionosphere, thermosphere, equatorial ionization anomaly, coupling, forcing

Observations by the GOLD mission are able to follow spatial and temporal changes in the composition, density and temperature of Earth’s thermosphere, providing fundamental information for understanding the Thermosphere-Ionosphere system. GOLD images the Earth from geostationary orbit at 47.5 degrees W longitude, observing on a 30-minute cadence from 06:10 to 0:40 UT (03:00-21:3 LT at the satellite). The observations performed include limb scans; stellar occultations; and images the sunlit and nightside disk. These data provide simultaneous, synoptic daytime imaging of the composition and temperature near 160 km for the first time. Repeated observations of peak densities in the low-latitude, nighttime equatorial ionization anomaly (EIA) and the depletions within it also provide a new perspective on that region. These observations are providing significant tests of current models, tests that may lead to advances in the capabilities of global-scale models of the thermosphere and ionosphere system. Observations also clearly indicate the presence of waves in the thermosphere. There are also clear indications of waves and tides propagating from lower altitudes. Examples of these observations, as well as their potential for advancing models of the thermosphere-ionosphere system, will be presented and discussed.