Results 11 to 20 of about 1,308 (218)
The Interplanetary Magnetic Field [PDF]
In 1974 a number of observations of the magnetic field at about 1 AU were already available and the concept of coronal magnetic field expansion in the heliosphere well established. On the other hand, only a few, sporadic, in situ field observations were available at heliocentric distances significantly inside the terrestrial orbit.
Franco Mariani, Fritz M. Neubauer
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Active Regions and the Interplanetary Magnetic Field [PDF]
The relation of solar active regions to the large-scale sector structure of the interplanetary field is discussed. In the winter of 1963–64 (observed by the satellite IMP-1) the plage density was greatest in the leading portion of the sectors and lesser in the trailing portion of the sectors. The boundaries of the sectors (places at which the direction
John M. Wilcox +2 more
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PUZZLES OF THE INTERPLANETARY MAGNETIC FIELD IN THE INNER HELIOSPHERE [PDF]
10 pages, 8 figures, 2 tables, Preprint IZMIRAN, Published in the Astrophysical Journal ...
Khabarova, Olga, Obridko, Vladimir
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Existence of interplanetary magnetic fields other than<br />the geomagnetic field is now well established. They travel as frozen-in<br />fields inside the solar plasma clouds: magnetic fields on the Sun are then<br />discussed ...
F. Molina, F. Mariani
doaj +1 more source
The physics of space weather/solar-terrestrial physics (STP): what we know now and what the current and future challenges are [PDF]
Major geomagnetic storms are caused by unusually intense solar wind southward magnetic fields that impinge upon the Earth's magnetosphere (Dungey, 1961). How can we predict the occurrence of future interplanetary events?
B. T. Tsurutani +3 more
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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.
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EULERIAN DECORRELATION OF FLUCTUATIONS IN THE INTERPLANETARY MAGNETIC FIELD [PDF]
A method is devised for estimating the two-time correlation function and the associated Eulerian decorrelation timescale in turbulence. With the assumptions of a single decorrelation time and a frozen-in flow approximation for the single-point analysis, the method compares two-point correlation measurements with single-point correlation measurements at
Matthaeus, W.H. +4 more
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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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The Structure and Origin of Switchbacks: Parker Solar Probe Observations
Switchbacks are rapid magnetic field reversals that last from seconds to hours. Current Parker Solar Probe (PSP) observations pose many open questions in regard to the nature of switchbacks.
Jia Huang +27 more
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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
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