First direct observations of atmospheric sputtering at Mars. [PDF]
Curry SM+10 more
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Detection of visible-wavelength aurora on Mars. [PDF]
Knutsen EW+27 more
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Investigating Solar Wind Outflows from Open-Closed Magnetic Field Structures Using Coordinated Solar Orbiter and Hinode Observations. [PDF]
Ngampoopun N+15 more
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Interhemispheric Asymmetry in the High-Latitude Neutral Density Variations During the 13-14 March 2022 Storm. [PDF]
Zhu Q, Lu G, Vines S, Hairston M.
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SMILE Modeling Working Group: Modeling and Analysis of X-ray and Ultraviolet Images of Solar Wind - Earth Interactions. [PDF]
Connor HK+15 more
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Wavelet Coherence Analysis of Plasma Beta, Alfven Mach Number, and Magnetosonic Mach Number during Different Geomagnetic Storms. [PDF]
Giri A+4 more
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In situ evidence of the magnetospheric cusp of Jupiter from Juno spacecraft measurements. [PDF]
Xu Y+15 more
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Interplanetary Magnetic Field and the Auroral Zones
Physical Review Letters, 1961Abstract : 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, 1965Observations 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
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Interplanetary Magnetic Fields
Science, 1962Preliminary 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
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