Results 251 to 260 of about 899,551 (302)

First direct observations of atmospheric sputtering at Mars. [PDF]

open access: yesSci Adv
Curry SM   +10 more
europepmc   +1 more source

Detection of visible-wavelength aurora on Mars. [PDF]

open access: yesSci Adv
Knutsen EW   +27 more
europepmc   +1 more source

Investigating Solar Wind Outflows from Open-Closed Magnetic Field Structures Using Coordinated Solar Orbiter and Hinode Observations. [PDF]

open access: yesSol Phys
Ngampoopun N   +15 more
europepmc   +1 more source

SMILE Modeling Working Group: Modeling and Analysis of X-ray and Ultraviolet Images of Solar Wind - Earth Interactions. [PDF]

open access: yesSpace Sci Rev
Connor HK   +15 more
europepmc   +1 more source

In situ evidence of the magnetospheric cusp of Jupiter from Juno spacecraft measurements. [PDF]

open access: yesNat Commun
Xu Y   +15 more
europepmc   +1 more source

Interplanetary Magnetic Field and the Auroral Zones

Physical Review Letters, 1961
Abstract : It was found that a model with a southward interplanetary magnetic field leads to a natural explanation of the SD currents. Speculative aspects of the problem as they appear at this time are discussed. It should be remembered that this problem is amenable to revolutionary progress by observations from rockets or satellites which go out more ...
J. Dungey
openaire   +3 more sources

Sector Structure of the Quiet Interplanetary Magnetic Field

Science, 1965
Observations of the interplanetary magnetic field by the Imp-1 satellite have revealed a regular longitudinal sector structure in this field. The sectors co-rotate with the sun; as an average sector sweeps past the earth the magnitude of the interplanetary field decreases from greater than 6 gammas (1 gamma = 10 -5 ...
John M. Wilcox, Norman F. Ness
openaire   +4 more sources

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.   +3 more
openaire   +4 more sources

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