Results 171 to 180 of about 2,952 (203)

The role of pressure gradients in driving sunward magnetosheath flows and magnetopause motion

, 2014
Martin Archer, D. L. Turner, J. P. Eastwood, T. S. Horbury, S. J. Schwartz   +4 more
openalex   +1 more source

Ion Anisotropy-driven waves in the Earth's magnetosheath and plasma depletion layer

, 1994
R. E. Denton, B. J. Anderson, S. A. Fuselier, S. Peter Gary, M. K. Hudson   +4 more
openalex   +2 more sources

A Novel Determination of the Foreshock ULF Boundary: Statistical Approach. [PDF]

J Geophys Res Space Phys
Salohub A, Šafránková J, Němeček Z, Pi G.   +3 more
europepmc   +1 more source

Acceleration noise due to space magnetic field for heliocentric gravitational wave detector. [PDF]

Sci Rep
Peng JH, Zhang JX, Hong W, Su W, Ni Y, Guo J, Zheng R.   +6 more
europepmc   +1 more source

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
europepmc   +1 more source

Two distinct current systems in the ionosphere of Mars. [PDF]

Nat Commun
Gao J, Li S, Mittelholz A, Rong Z, Persson M, Shi Z, Lu H, Zhang C, Wang X, Dong C, Klinger L, Cui J, Wei Y, Pan Y.   +13 more
europepmc   +1 more source

Future opportunities in solar system plasma science through ESA's exploration programme. [PDF]

NPJ Microgravity
Holmstrom M, Lester M, Sanchez-Cano B.
europepmc   +1 more source

Wandering of the auroral oval 41,000 years ago. [PDF]

Sci Adv
Mukhopadhyay A, Panovska S, Garvey R, Liemohn MW, Ganjushkina N, Brenner A, Usoskin I, Balikhin M, Welling DT.   +8 more
europepmc   +1 more source

Plasma structuring within an expanded polar cap and cusp studied with the SS-520-3 sounding rocket

Buschmann LM, Asamura K, Clausen L, Jin Y, Kojima H, Kumamoto A, Kurita S, Ogawa Y, Oksavik K, Saito Y, Spicher A, Yokota S, Miloch W.   +12 more
europepmc   +1 more source

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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