Magnetic topology of coronal mass ejection events out of the ecliptic: Ulysses/HI-SCALE energetic particle observations [PDF]
Solar energetic particle fluxes (Ee > 38 keV) observed by the ULYSSES/HI-SCALE experiment are utilized as diagnostic tracers of the large-scale structure and topology of the Interplanetary Magnetic Field (IMF) embedded within two well ...
O. E. Malandraki +3 more
doaj +1 more source
The local dayside reconnection rate for oblique interplanetary magnetic fields [PDF]
We present an analysis of local properties of magnetic reconnection at the dayside magnetopause for various interplanetary magnetic field (IMF) orientations in global magnetospheric simulations.
Cassak, Paul A., Komar, Colin M.
core +3 more sources
Comparison of the mean photospheric magnetic field and the interplanetary magnetic field [PDF]
Photospheric and interplanetary magnetic field polarity and magnitude comparison, using Explorer ...
A. Severny +3 more
openaire +1 more source
Mars’s magnetosphere is hybrid, having contributions from both an induced magnetosphere like Venus and the localized crustal magnetic fields. However, the planetary fields also include large-scale, more global components.
Shaosui Xu +12 more
doaj +1 more source
32. Interplanetary magnetic field [PDF]
The magnetic field outside the sun (interplanetary magnetic field) is certainly far from a dipole field. A model of it has recently been suggested (Tellus,8, 1, 1956). This model is in agreement with cosmic ray and magnetic storm data and reconcilable with the coronal ray structure. Some possibilities to check the model are discussed.
openaire +1 more source
Extension of the Photospheric Magnetic Field Into Interplanetary Space [PDF]
Comparison of interplanetary magnetic field measurements made by Imp-I satellite and those obtained with solar magnetograph at Mount ...
John M. Wilcox, Norman F. Ness
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Oscillations in the open solar magnetic flux with a period of 1.68 years: imprint on galactic cosmic rays and implications for heliospheric shielding [PDF]
An understanding of how the heliosphere modulates galactic cosmic ray (GCR) fluxes and spectra is important, not only for studies of their origin, acceleration and propagation in our galaxy, but also for predicting their effects (on technology and on the
A. Rouillard, M. Lockwood, M. Lockwood
doaj +1 more source
Heliospheric Diffusion of Stochastic Parker Spirals in Radially Evolving Solar Wind Turbulence
We present a stochastic field line mapping model where the interplanetary magnetic field lines are described by a density distribution function satisfying a Fokker–Planck equation that is solved numerically.
N. H. Bian +3 more
doaj +1 more source
Interplanetary magnetic field control of dayside transient event occurrence and motion in the ionosphere and magnetosphere [PDF]
The pressure pulse model for dayside transient ionospheric events predicts dawnward moving events at and prior to local noon during periods of spiral interplanetary magnetic field (IMF) orientation, but duskward moving events at and after local noon ...
G. I. Korotova +4 more
doaj +1 more source
NASA Will Launch Third Interplanetary Monitoring Platform [PDF]
Explorer XVIII satellite Interplanetary Monitoring Platform /IMP/ measurements of magnetic fields, cosmic rays, solar wind, and lunar magnetosphere shock ...
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