Results 171 to 180 of about 1,308 (218)

Characteristics of Ionospheric Responses over China During the November 2023 Geomagnetic Storm and Evaluation of Positioning Performance of CORS in Low-Latitude Regions. [PDF]

Sensors (Basel)
Li L, Wang Y, Zhang J, Tang J, Yu F, Wang J, Zhang Z.   +6 more
europepmc   +1 more source

Magnetoacoustic wave propagation in the solar corona and filament dynamics. [PDF]

Sci Rep
Somaiyeh S, Stefaan P.
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

Complexity analyses of geomagnetic and solar activity indices time series. [PDF]

Sci Rep
Javaherian M, Mollaei S, Zolghadr N, Moradpour H, Yousefzadeh M.   +4 more
europepmc   +1 more source

Day-to-Day Boundary Fluctuations in Coronal Holes: Causes and Consequences. [PDF]

Sol Phys
Ugarte-Urra I, Wang YM, Muglach K, Sheeley NR.   +3 more
europepmc   +1 more source

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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 ...
Igor Veselovsky, A P Kropotkin, Kropotkin A P   +2 more
exaly   +2 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., Davis, Leverett, Jr., Smith, E. J., Sonett, C. P.   +3 more
openaire   +3 more sources

Intermittent character of interplanetary magnetic field fluctuations

Physics of Plasmas, 2007
Interplanetary magnetic field magnitude fluctuations are notoriously more intermittent than velocity fluctuations in both fast and slow wind. This behavior has been interpreted in terms of the anomalous scaling observed in passive scalars in fully developed hydrodynamic turbulence.
Roberto Bruno, Vincenzo Carbone, Luca Sorriso-Valvo   +2 more
exaly   +6 more sources

Solar and Interplanetary Magnetic Fields

Science, 1966
John M Wilcox
exaly   +2 more sources

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
exaly   +2 more sources