Results 61 to 70 of about 103,965 (278)

Solar Wind–Magnetosphere Coupling by the Kelvin–Helmholtz Instability at Mercury

The Astrophysical Journal
The Kelvin–Helmholtz instability (KHI) has been considered important in the energy transfer and momentum coupling between the solar wind and planetary magnetospheres.
S. H. Lai, Y.-C. Wang, Y.-H. Yang, W.-H. Ip   +3 more
doaj   +1 more source

Electron radiation belt dynamics during magnetic storms and in quiet time

Solar-Terrestrial Physics, 2018
The paper discusses the outer electron belt dynamics, adiabatic and nonadiabatic mechanisms of increases and losses of energetic electrons. Under undisturbed conditions, the outer electron belt gradually empties: in the inner magnetosphere due to ...
Lazutin L.L., Dmitriev A.V., Suvorova A.V.   +2 more
doaj   +1 more source

Spaceborne and spaceborn: Physiological aspects of pregnancy and birth during interplanetary flight

Experimental Physiology, EarlyView.
Abstract Crewed interplanetary return missions that are on the planning horizon will take years, more than enough time for initiation and completion of a pregnancy. Pregnancy is viewed as a sequence of processes – fertilization, blastocyst formation, implantation, gastrulation, placentation, organogenesis, gross morphogenesis, birth and neonatal ...
Arun V. Holden
wiley   +1 more source

The role of the Hall effect in the global structure and dynamics of planetary magnetospheres: Ganymede as a case study [PDF]

, 2015
We present high resolution Hall MHD simulations of Ganymede's magnetosphere demonstrating that Hall electric fields in ion-scale magnetic reconnection layers have significant global effects not captured in resistive MHD simulations. Consistent with local
Collinson, Glyn, Dorelli, John C., Glocer, Alex, Tóth, Gábor   +3 more
core   +1 more source

Transport of Mirror Mode Structures through Saturn’s Magnetopause Reconnection

The Astrophysical Journal
Magnetopause reconnection plays a significant role in transferring plasma and energy from the solar wind to planetary magnetospheres. Using a Cassini measurement, we reported a magnetopause reconnection at Saturn, identified by the Hall magnetic field ...
S. B. Xu, S. Y. Huang, Z. G. Yuan, K. Jiang, H. H. Wu, J. Zhang, Z. Wang, Q. Y. Xiong, R. T. Lin   +8 more
doaj   +1 more source

EMIC Waves in the Outer Magnetosphere: Observations of an Off-Equator Source Region. [PDF]

, 2019
Electromagnetic ion cyclotron (EMIC) waves at large L shells were observed away from the magnetic equator by the Magnetospheric MultiScale (MMS) mission nearly continuously for over four hours on 28 October 2015.
B. J. Anderson, C. T. Russell, J. L. Burch, King J. H., M. J. Engebretson, P. A. Lindqvist, R. B. Torbert, R. C. Allen, R. E. Ergun, R. J. Strangeway, S. A. Fuselier, S. K. Vines, Zhang J.‐C.   +12 more
core   +1 more source

Dawn–dusk asymmetries in the coupled solar wind–magnetosphere–ionosphere system: a review [PDF]

, 2014
. Dawn–dusk asymmetries are ubiquitous features of the coupled solar-wind–magnetosphere–ionosphere system. During the last decades, increasing availability of satellite and ground-based measurements has made it possible to study these phenomena in more ...
A. Walsh, S. Haaland, C. Forsyth, A. Keesee, J. Kissinger, K. Li, A. Runov, J. Souček, B. M.Walsh, S. Wing, M. Taylor   +10 more
semanticscholar   +1 more source

Geomagnetic pulsations in 1–4 mHz frequency range (Pc5/Pi3) in the magnetotail at different levels of disturbances in the interplanetary medium

Solar-Terrestrial Physics, 2022
In this paper, we study parameters of geomagnetic pulsations in the 1–4 mHz frequency range (Pc5/Pi3) in the magnetotail, utilizing data obtained by Cluster satellites at different levels of fluctuations in the interplanetary magnetic field (IMF) and the
Yagova N. V., Kozyreva O. V., Nosikova N. S.   +2 more
doaj   +1 more source

A quantitative assessment of empirical magnetic field models at geosynchronous orbit during magnetic storms [PDF]

, 2008
[1] We evaluate the performance of recent empirical magnetic field models (Tsyganenko, 1996, 2002a, 2002b; Tsyganenko and Sitnov, 2005, hereafter referred to as T96, T02 and TS05, respectively) during magnetic storm times including both pre- and post ...
Huang, Chia-Lin L., Singer, H. J., Spence, Harlan E., Tsyganenko, N. A.   +3 more
core   +3 more sources

From physics of polar aurora to changes of the fundamental approaches to the physics of the magnetospheric processes

Frontiers in Astronomy and Space Sciences, 2022
One of the main problems of modern magnetospheric physics is the lack of a self-consistent explanation of the main physical processes based on the laws of plasma physics.
Elizaveta E. Antonova, Elizaveta E. Antonova   +1 more
doaj   +1 more source