Results 71 to 80 of about 21,013 (198)
We address the problem of calculating the transverse magnetic field in the solar wind outside of the hypothetical sphere called the source surface where the solar wind originates.
Tran, Tham, Ulrich, Roger K.
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Proton Temperature and Density Variations in Linear Magnetic Holes in the Solar Wind
Linear magnetic holes (LMHs) are pressure-balanced structures characterized by reduced magnetic pressure and compensatory thermal pressure enhancements, driven by proton temperature and/or density variations.
RuiHui Yu, Xin Wang, Hua Zhang, Yu Zhang
doaj +1 more source
The interplanetary magnetic field: Radial and latitudinal dependences [PDF]
29 pages, 10 figures, Astronomy Reports, 2013, V.
openaire +2 more sources
A model of interplanetary and coronal magnetic fields [PDF]
Model of interplanetary and solar magnetic field structure above photosphere using Green function solution to Maxwell ...
Ness, N. F. +2 more
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We analyze the well observed flare-CME event from October 1, 2011 (SOL2011-10-01T09:18) covering the complete chain of action - from Sun to Earth - for a better understanding of the dynamic evolution of the CME and its embedded magnetic field.
Dissauer, K. +6 more
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The Parker Solar Probe (PSP) mission has revealed frequent occurrences of switchbacks (SBs) and small-scale magnetic flux ropes (SMFRs) as prominent structures within the solar wind. These mesoscale features are observed across all heliocentric distances,
Kyung-Eun Choi +7 more
doaj +1 more source
The large-scale electric fields in Earth's inner magnetosphere are generated by the interaction between the solar wind and Earth's magnetic field.
Zhao Zhang, Dianjun Zhang, Wenlong Liu
doaj +1 more source
Unipolar induction in the magnetosphere [PDF]
A theory is described for the production of electric currents in the magnetosphere and for the transfer of energy from the solar wind to the magnetosphere.
Stern, D. P.
core +1 more source
Connecting speeds, directions and arrival times of 22 coronal mass ejections from the Sun to 1 AU
Forecasting the in situ properties of coronal mass ejections (CMEs) from remote images is expected to strongly enhance predictions of space weather, and is of general interest for studying the interaction of CMEs with planetary environments. We study the
Amla, K. +17 more
core +1 more source
In space plasmas, the rarity of collisions leads to complex structures in the velocity space where a turbulent cascade of the velocity distribution function (VDF) fluctuations is thought to occur.
A. Larosa +13 more
doaj +1 more source

