Climatology of the Equatorial Plasma Bubbles Captured by FORMOSAT‐3/COSMIC
Climatology of the Equatorial Plasma Bubbles Captured by FORMOSAT‐3/COSMIC
复制标题
FORMOSAT-3/COSMIC 捕获的赤道等离子体气泡的气候学
DOI:
10.1029/2019ja027680
复制
发表时间:
2019
期刊:
影响因子:
--
通讯作者:
J. Braun
中科院分区:
文献类型:
--
作者:
M. Chou;Qian Wu;N. Pedatella;I. Cherniak;W. Schreiner;J. Braun
The FORMOSAT‐3/COSMIC (F3/C) satellites are used to study the climatology of equatorial plasma bubbles (EPBs) during the low to moderate solar flux years (2008–2013). We use the F3/C total electron content to identify the presence of EPBs and investigate the background conditions for the initiation of EPBs. The results reveal that the EPB activities have strong solar dependence. The longitudinal and seasonal trends of EPBs are highly correlated to the angle between the dusk solar terminator and magnetic field lines near the magnetic equator. Asymmetries of EPBs between solstices and equinoxes exist and could be due partly to the asymmetry of equatorial ionization anomaly structures, which result in longitudinal differences as well. EPBs extend to higher altitudes and latitudes during the ascending phase of Solar Cycle 24 (2011–2013) due mainly to the increase of background electron density. However, an altitudinal asymmetry of EPBs occurs in moderate solar flux years, which is likely due to the suppression or lower growth and occurrence rates of EPBs. In addition to vertical drift, tidal forcing also contributes to the longitudinal and seasonal distributions of EPBs. Upwellings and precursor waves preceding the EPBs are observed climatologically, which likely play a vital role in initiating the EPBs. This study also reveals a vertical connection between the equatorial ionospheric irregularities and atmospheric forcing on a climatological basis.
影响因子:
3.9
作者:
H. Nakata;Akira Takahashi;T. Takano;A. Saito;T. Sakanoi
通讯作者:
H. Nakata;Akira Takahashi;T. Takano;A. Saito;T. Sakanoi
影响因子:
2.8
作者:
Nishioka, M.;Saito, A.;Tsugawa, T.
通讯作者:
Tsugawa, T.
DOI:
--
发表时间:
2011
期刊:
影响因子:
--
作者:
W.Ohashi;H.Hirota;T.Yamazaki;Yulin Gao;小川泰信
通讯作者:
小川泰信