Results 41 to 50 of about 2,907 (207)
The Evolution of Whistler Hiss‐Like Waves Across Plasmapause: Hiss to Exohiss
Geophysical Research Letters, 2023 The exohiss waves are hiss‐like whistler mode waves that occur outside plasmapause. Although these waves can cause the loss of radiation belt electrons ∼
Bopu Feng +7 more
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Response of convection electric fields in the magnetosphere to IMF orientation change [PDF]
, 2009 [1] The transient response of convection electric fields in the inner magnetosphere to southward turning of the interplanetary magnetic field (IMF) is investigated using in‐situ electric field observations by the CRRES and Akebono spacecraft.
Brautigam, D. +7 more
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Ionospheric Pc1 waves during a storm recovery phase observed by the China Seismo-Electromagnetic Satellite [PDF]
Annales Geophysicae, 2020 During the storm recovery phase on 27 August 2018, the China Seismo-Electromagnetic Satellite (CSES) detected Pc1 wave activities in both the Northern Hemisphere and Southern Hemisphere in the high-latitude, post-midnight ionosphere with a central ...
X. Gou +15 more
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Solar-Terrestrial Physics, 2016 We present results of the analysis of an unusually long narrow-band emission in the Pc1 range with increasing carrier frequency. The event was observed against the background of the main phase of a strong magnetic storm caused by arrival of a high-speed ...
Potapov A.S. +4 more
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Cluster observations of mid-latitude hiss near the plasmapause [PDF]
Annales Geophysicae, 2004 In the vicinity of the plasmapause, around the geomagnetic equator, the four Cluster satellites often observe banded hiss-like electromagnetic emissions (BHE); below the electron gyrofrequency but above the lower hybrid resonance, from 2kHz to 10kHz ...
A. Masson +4 more
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Model study of plasmapause motion [PDF]
Journal of Geophysical Research, 1970 The ambient plasma in the equatorial plane is predominantly subject to the E×B drift. By approximating the earth's magnetic field by a dipole, characteristic steady state streamlines in the equatorial plane are determined, assuming the interaction between the solar wind and the magnetosphere is characterized by a constant electric field directed from ...
openaire +1 more source
Earth and Planetary Physics, 2017 The plasmapause locations determined from the Chang’e-3 (CE-3) Extreme Ultraviolet Camera (EUVC) images and the auroral boundaries determined from the Defense Meteorological Satellite Program (DMSP) Special Sensor Ultraviolet Spectrographic Imager (SSUSI)
XiaoXin Zhang +4 more
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Wave and plasma measurements and GPS diagnostics of the main ionospheric trough as a hybrid method used for Space Weather purposes [PDF]
Annales Geophysicae, 2008 The region of the main ionospheric trough is a unique region of the ionosphere, where different types of waves and instabilities can be generated. This region of the ionosphere acts like a lens, focusing a variety of indicators from the equator of ...
H. Rothkaehl +6 more
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Magnetospheric processes in the plasmapause
Eos, Transactions American Geophysical Union, 1984 The current experimental and theoretical status on the existence and importance of the plasmapause as a magnetospheric boundary was the subject of a conference on Fundamental Magnetospheric Processes in the Plasmapause Region, held at Huntsville, Ala., October 25–27, 1983, under the joint sponsorship of the Marshall Space Flight Center and the ...
James L. Green, James L. Horwitz
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A new model for plasmapause locations derived from IMAGE RPI and Van Allen Probes data
Journal of Space Weather and Space ClimateThe outer boundary of the plasmasphere, the plasmapause, is characterized by a sharp electron density gradient that changes under varying space weather conditions.
Banyś Daniela +6 more
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