Mirror instability upstream of the termination shock (TS) and in the heliosheath
BT Tsurutani, E Echer, OP Verkhoglyadova… - Journal of atmospheric …, 2011 - Elsevier
We experimentally identify mirror mode (MM) structures in the Voyager 1 heliosheath data
for the first time. This is done using the magnetic field data alone. The heliosheath MM …
for the first time. This is done using the magnetic field data alone. The heliosheath MM …
Statistical study of low‐frequency magnetic field fluctuations near Venus under the different interplanetary magnetic field orientations
The magnetic field fluctuations near Venus are investigated in the frequency range 0.03–0.3
Hz on the basis of the measurements observed by Venus Express from April 2006 to …
Hz on the basis of the measurements observed by Venus Express from April 2006 to …
Statistical study of low‐frequency magnetic field fluctuations near Venus during the solar cycle
SD Xiao, TL Zhang, GQ Wang - Journal of Geophysical …, 2017 - Wiley Online Library
We statistically investigate the solar cycle dependence of the magnetic field fluctuations in
the frequency range 30–300 MHz based on Venus Express data. We present the spatial …
the frequency range 30–300 MHz based on Venus Express data. We present the spatial …
[图书][B] Diamagnetic cavities and energetic particles in the Earth's magnetospheric cusps
J Niehof - 2011 - search.proquest.com
The Polar spacecraft provided over a decade of quality observations in the high latitude
regions of Earth's magnetosphere. After on-orbit operations terminated, some questions …
regions of Earth's magnetosphere. After on-orbit operations terminated, some questions …
Структура магнитослоя Земли при небольших флуктуациях направления межпланетного магнитного поля
ОМ Чугунова, ВА Пилипенко, ГН Застенкер… - Космические …, 2011 - elibrary.ru
Исследовалась пространственная структура магнитослоя Земли в условиях, когда не
наблюдается резких (более чем на 40 за 5 минут) изменений направления …
наблюдается резких (более чем на 40 за 5 минут) изменений направления …
Structure of the earth's magnetosheath at small fluctuations in the interplanetary magnetic field direction
OM Chugunova, VA Pilipenko, GN Zastenker… - Cosmic Research, 2011 - Springer
Spatial structure of the magnetosheath of the Earth was studied under the conditions when
no sharp (more than 40° during 5 min) changes in the interplanetary magnetic field direction …
no sharp (more than 40° during 5 min) changes in the interplanetary magnetic field direction …