Results 171 to 180 of about 20,985 (231)

A New Facility Will Harness Plasma to Guide Interplanetary Craft. [PDF]

ACS Cent Sci
Bourzac K.
europepmc   +1 more source

Chaotic, rational and irrational oscillations of nonlinear waves in the Earth's magnetosheath featuring bi-regularized κ -distributed electrons. [PDF]

Sci Rep
Sarkar J, Saha A.
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Bow shock oscillations of Mars under weakly disturbed solar wind conditions. [PDF]

Nat Commun
Cheng L, Wang Y, Ma Y, Lillis R, Halekas J, Langlais B, Zhang T, Zhang A, Wang G, Xiao S, Zou Z, Chi Y, Hao X, Li Y, Pan Z, Liu K.   +15 more
europepmc   +1 more source

Global heliospheric termination shock strength in the solar-interstellar interaction. [PDF]

Nat Astron
Zirnstein EJ, Kumar R, Shrestha BL, Swaczyna P, Dayeh MA, Heerikhuisen J, Szalay JR.   +6 more
europepmc   +1 more source

Global-scale magnetosphere convection driven by dayside magnetic reconnection. [PDF]

Nat Commun
Dai L, Zhu M, Ren Y, Gonzalez W, Wang C, Sibeck D, Samsonov A, Escoubet P, Tang B, Zhang J, Branduardi-Raymont G.   +10 more
europepmc   +1 more source

Detrimental impact of solar and geomagnetic activity on plasma B-complex vitamins in the VA normative aging study cohort. [PDF]

Sci Rep
Zilli Vieira CL, Liu CS, Rudke AP, Wang Y, Wang VA, Schwartz JD, Vokonas P, Koutrakis P.   +7 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

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Interplanetary Magnetic Fields

Science, 1962
Preliminary analysis of Mariner II magnetometer data indicates a persistent interplanetary field varying between a least 2 and 10 gamma (1γ = 10 -5 gauss). The interplanetary field appears to lie mainly in the ecliptic plane, although there is a substantial, fluctuating, transverse component.
Coleman, P. J., Jr., Davis, Leverett, Jr., Smith, E. J., Sonett, C. P.   +3 more
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Interplanetary magnetic fields

Reviews of Geophysics, 1979
Within the past four years, significant scientific progress has been possible as a result of improvements in observations of the interplanetary field. First, the range of radial distances over which observations are available has been greatly extended; measurements have been made as near the Sun as 0.3 AU and as far away as 8.5 AU. Second, the range of
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Interplanetary magnetic field and magnetospheric substorms

Planetary and Space Science, 1977
The interplanetary magnetic field (IMF) changes and the associated responses of the magnetosphere on November 1, 1972, are examined. IMF Bz changes consisted of a sudden southward turning, a slow northward turning, and a subsequent steady northward sense. Magnetospheric substorms occurred throughout this period.
S.-I. Akasofu, R.P. Lepping
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