Results 151 to 160 of about 1,320 (193)

Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]

Living Rev Sol Phys
Veronig AM, Dissauer K, Kliem B, Downs C, Hudson HS, Jin M, Osten R, Podladchikova T, Prasad A, Qiu J, Thompson B, Tian H, Vourlidas A.   +12 more
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Monitoring the daily variation of Sun-Earth magnetic fields using galactic cosmic rays. [PDF]

Innovation (Camb)
LHAASO Collaborationnanyc@ihep.ac.cnchensz@ihep.ac.cnfengcf@sdu.edu.cn.
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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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On interplanetary electric and magnetic fields

Solar Physics, 1982
A kinematic model of the stationary electromagnetic fields in interplanetary space with finite conductivity is considered. The electrodynamic problem is solved for a medium with uniform conductivity and radial plasma outflow from a spherical source. Simple analytical formulae are obtained for electric and magnetic fields, currents and charges in the ...
I. I. Alexeev, A. P. Kropotkin, I. S. Veselovsky   +2 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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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 ...
N F, Ness, J M, Wilcox
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The interplanetary plasma and magnetic field

2nd Annual Meeting, 1965
Solar wind plasma and interplanetary magnetic field influence on propagation of nonlinear wave ...
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Substorms and the interplanetary magnetic field

Journal of Geophysical Research, 1976
Although it has been established that there is a strong relationship between observed substorms and the southward component of the interplanetary field B/sub z/, there remains a controversy concerning models explaining this relationship. An analysis of a statistical study of isolated substorms and the related interplanetary fields had previously ...
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REGULATION OF THE INTERPLANETARY MAGNETIC FIELD

1992
In this study we use a recently developed technique for measuring the combined magnitudes of inward and outward (sunward and antisunward) pointing 2D magnetic flux in the ecliptic plane to examine (1) the long term variation of the amount of magnetic field open to interplanetary space and (2) the apparent rate at which coronal mass ejections (CMEs) may
D.J. McComas, J.T. Gosling, J.L. Phillips   +2 more
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The interplanetary magnetic field structure

Nature, 1976
The seasonal bias in the sector structure of the interplanetary magnetic field has led to the suggestion that the field in each hemisphere of the solar cavity has the same polarity as the average magnetic field at the corresponding solar pole, and that the surface which separates the two polarity regions is only slightly warped.
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