Results 131 to 140 of about 940 (176)

The anomalous state of Uranus's magnetosphere during the Voyager 2 flyby. [PDF]

Nat Astron
Jasinski JM, Cochrane CJ, Jia X, Dunn WR, Roussos E, Nordheim TA, Regoli LH, Achilleos N, Krupp N, Murphy N.   +9 more
europepmc   +1 more source

Mars's induced magnetosphere can degenerate. [PDF]

Nature
Zhang Q, Barabash S, Holmstrom M, Wang XD, Futaana Y, Fowler CM, Ramstad R, Nilsson H.   +7 more
europepmc   +1 more source

Extreme dominance of Earth-origin heavy ions in the intense ring current near the Earth during the May 2024 super geomagnetic storm. [PDF]

Sci Adv
Kitamura N, Yamamoto K, Yokota S, Kasahara S, Matsuoka A, Asamura K, Ebihara Y, Kistler LM, Keika K, Shinbori A, Hori T, Miyoshi Y, Ieda A, Jun CW, Teramoto M, Nosé M, Hirahara M, Seki K, Higashio N, Shinohara I.   +19 more
europepmc   +1 more source

Phase space electron hole in the Venusian upper mantle boundary. [PDF]

Sci Rep
Gamal A, Moslem WM, Yousef MS, Ellithi AY.   +3 more
europepmc   +1 more source

On the origin of magnetosheath plasmoids and their relation to magnetosheath jets [PDF]

Journal of Geophysical Research: Space Physics, 2015
AbstractWe investigate localized magnetosheath and solar wind density enhancements, associated with clear magnetic field changes, and therefore referred to as magnetosheath/solar wind plasmoids, respectively. Using Cluster data, we show that there are two distinct populations of magnetosheath plasmoids, one associated with a decrease of magnetic field ...
Herbert Gunell, Maria Hamrin, Tomáš Karlsson   +2 more
exaly   +3 more sources

Causes of Jets in the Quasi-Perpendicular Magnetosheath [PDF]

Geophysical Research Letters, 2021
AbstractMagnetosheath jets are currently an important topic in the field of magnetosheath physics. It is thought that 97% of the jets are produced by the shock rippling at quasi‐parallel shocks. Recently, large statistical studies of magnetosheath jets have been performed, however, it is not clear whether rippling also produces jets found downstream of
Xóchitl Blanco-Cano, Primoz Kajdič, Savvas Raptis   +2 more
exaly   +3 more sources

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The Magnetosheath

Space Science Reviews, 2005
International ...
Lucek, E. A., Constantinescu, D., Goldstein, M. L., Pickett, J., Pincon, Jean-Louis, Sahraoui, F., Treumann, R. A., Walker, S. N.   +7 more
openaire   +3 more sources

The Magnetosheath and Magnetotail of Venus

Space Science Reviews, 1991
We describe the observational history and assess the current understanding of the magnetosheath and magnetotail of Venus, stressing recent developments. We make recommendations for research that can be done using existing observations, as well as desirable trajectory and instrumentation characteristics for future spacecraft missions.
John L. Phillips, David J. McComas
openaire   +2 more sources

On the form of the flow in the magnetosheath

Journal of Geophysical Research: Space Physics, 1992
The form of the flow field in the subsonic and transsonic magnetosheath has received little attention since the proposal of a depletion layer adjacent to the magnetopause by Zwan and Wolf. Recently, observations of density enhancements just upstream of the magnetopause which have been interpreted as slow mode compressional fronts appear to contradict ...
David J. Southwood, Margaret G. Kivelson
openaire   +1 more source

magnetosheath lion roars

Journal of Geophysical Research, 1976
The characteristics of lion roars, which are intense packets of electromagnetic waves characteristically found in the magnetosheath, are studied. The average frequency of the emissions is 120 Hz, with over 90% occurring between 90 and 160 Hz (which is near one-half the local electron gyrofrequency); over 70% of all emissions last a mere 2 sec or less ...
Edward J. Smith, Bruce T. Tsurutani
openaire   +1 more source