Results 121 to 130 of about 1,550 (181)

Unprecedented extreme depletion of Earth's ionosphere during the May 2024 super geomagnetic storm revealed by the Chinese Meridian Project. [PDF]

Natl Sci Rev
Cao J.
europepmc   +1 more source

A galactic cosmic ray cavity in Earth-Moon space. [PDF]

Sci Adv
Shang W, Liu J, Xu Z, Yue C, Guo R, Xiao C, Shi Q, Wimmer-Schweingruber RF, Guo J, Degeling AW, Rankin R, Tian A, Zong QG, Han C, Park JS, Wang H, Liu W, Fu S, Zhai LM, Chen D, Ni S, Chen TL.   +21 more
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Energetic neutral atom imaging reveals nearly 11-year cycle of the ring current of Saturn. [PDF]

Nat Commun
Li Y, Yue C, Sun Y, Jia X, Zong Q, Zhou X.   +5 more
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Analyzing AZ-non-Maxwellian distributions in Earth's magnetosphere: MMS observations. [PDF]

Sci Rep
Abid AA, Hussain MS, Esmaeili A, Khan A, Ali S, Alharbi M, Al-Hadeethi Y, Bedaiwi NM.   +7 more
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From the TRICE-2 Investigations to the TRACERS Mission. [PDF]

Space Sci Rev
Trattner KJ, LaBelle J, Santolik O, Kletzing CA, Miles DM, Fuselier SA, Bonnell JW, Bounds SR, Kolmasova I, Petrinec SM, Sawyer RP, Vines SK, Moser-Gauthier C, Cairns IH, Yeoman TK.   +14 more
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Pulsar magnetospheres

Nature Physical Science, 1971
Abstract The energy loss from the neutron star - as inferred from the secular increase in rotation period - is much greater than that emitted in either the radio or the other observed wavelengths. A primary motivation of magnetospheric theory is to trace the mode in which this energy and the associated angular momentum are in fact ...
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Magnetospheric Wind

Science, 1969
An experiment designed to detect the bulk flow of cool plasma within the magnetosphere has been flown on the ATS-1 (Applications Technology Satellite) synchronous satellite. This experiment has yielded evidence for gusts of streaming positive ions in the magnetospheric equatorial plane. This directed ion flow is interpreted as the result of large-scale
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Magnetospheric turbulence and properties of magnetospheric dynamics

Advances in Space Research, 2008
Abstract High level of turbulence is one of the main peculiarities inherent to magnetospheric dynamics. Mechanisms for generation of magnetospheric turbulence are analyzed. The instabilities in the plasma pressure distribution are examined as source of large and medium scale modes in the turbulence spectra.
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The Pulsar Magnetosphere

Astrophysics and Space Science, 2000
Domains of the pulsar magnetosphere, both within and without the light-cylinder, are studied under varying provisional assumptions. Some of the qualitative features emerging should persist in the ultimate synthesis of a completely self-consistent model.
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