Results 21 to 30 of about 300 (160)

Current sheets in planetary magnetospheres [PDF]

open access: yesPlasma Physics and Controlled Fusion, 2019
Abstract In this article we aim to highlight the problems related to the structure and stability of the comparatively thin current sheets that were relatively recently discovered by space missions in the magnetospheres of the Earth and planets, as well as in the solar wind. These magnetoplasma structures are universal in collisionless
Lev Zelenyi   +4 more
openaire   +3 more sources

Behavior of Earth Magnetosphere Radius during Strong Geomagnetic Storms

open access: yesIraqi Journal of Physics, 2019
Magnetosphere is a region of space surrounding Earth magnetic field, the formation of magnetosphere depends on many parameters such as; surface magnetic field of the planet, an ionized plasma stream (solar wind) and the ionization of the planetary upper
Mais Mohammed Algbory   +1 more
doaj   +1 more source

Planetary magnetospheres

open access: yesGeofísica Internacional, 1991
La serie de naves espaciales Pionero, Marinero y Viajero nos ha dado a conocer una impresionante variedad de magnetosferas planetarias. Debido a su cercanía, la magnetosfera terrestre es la que mejor entendemos. El viento solar provee parte del plasma y, aun mas importante, provee la energía que da lugar a una amplia variedad de fen6menos que se ...
openaire   +2 more sources

Development of ground pipeline system for high-level scientific data products of the Hisaki satellite mission and its application to planetary space weather

open access: yesJournal of Space Weather and Space Climate, 2019
The Hisaki satellite is the first-ever space telescope mission dedicated to planetary sciences. Atmospheres and magnetospheres of our solar system planets are continuously monitored by the extreme ultraviolet (EUV) spectrometer onboard Hisaki. This paper
Kimura Tomoki   +9 more
doaj   +1 more source

Research on Jupiter's magnetic field: Review and prospect

open access: yes地球与行星物理论评
The internal structure and dynamics of different planets are different, so some planets have an intrinsic magnetic field, and some have not yet found an intrinsic magnetic field.
Weidong Gu   +6 more
doaj   +1 more source

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

open access: yesExperimental 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

Global-scale magnetosphere convection driven by dayside magnetic reconnection

open access: yesNature Communications
Plasma convection on a global scale is a fundamental feature of planetary magnetosphere. The Dungey cycle explains that steady-state convection within the closed part of the magnetosphere relies on magnetic reconnection in the nightside magnetospheric ...
Lei Dai   +10 more
doaj   +1 more source

Mercury’s plasma environment after BepiColombo’s third flyby

open access: yesCommunications Physics
Understanding Mercury’s magnetosphere is crucial for advancing our comprehension of how the solar wind interacts with the planetary magnetospheres. Despite previous missions, several gaps remain in our knowledge of Mercury’s plasma environment.
Lina Z. Hadid   +24 more
doaj   +1 more source

Statistics of the Interplanetary Magnetic Field from 0.1 to 30 au. II. Dynamical Variability

open access: yesThe Astrophysical Journal
The interplanetary magnetic field (IMF) governs the coupling between the solar wind and planetary magnetospheres through a series of complex interactions.
Jiutong Zhao   +10 more
doaj   +1 more source

First Observation of Electron Rolling‐Pin Distribution in Jupiter's Magnetosphere

open access: yesGeophysical Research Letters
The electron rolling‐pin distribution, showing electron pitch angles primarily at 0°, 90°, and 180°, has been widely studied in the Earth's magnetosphere, but has never been reported in other planetary environments.
C. Q. Wang   +8 more
doaj   +1 more source

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