Results 11 to 20 of about 4,306,191 (296)
The investigation of quasi-separatrix layers in solar magnetic fields [PDF]
, 2011 The structure of the magnetic field is often an important factor in many energetic processes in the solar corona. To determine the topology of the magnetic field features such as null points, separatrix surfaces, and separators must be found.
Restante, Anna Lisa
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Small-Scale Solar Magnetic Fields [PDF]
Space Science Reviews, 2008 43 pages, 18 ...
de Wijn, A. +3 more
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VECTOR MAGNETIC FIELDS OF SOLAR GRANULATION [PDF]
The Astrophysical Journal, 2008 24 pages in total, 9 ...
Jin, Chunlan, Wang, Jingxiu, Zhao, Meng
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Solar mean magnetic field of the chromosphere
Journal of Astrophysics and Astronomy, 2023 The Solar Mean Magnetic Field (SMMF) is the mean value of the line of sight (LOS) component of the solar vector magnetic field averaged over the visible hemisphere of the Sun. So far, the studies on SMMF have mostly been confined to the magnetic field measurements at the photosphere. In this study, we calculate and analyse the SMMF using magnetic field
M. Vishnu, K. Nagaraju, Harsh Mathur
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On the fractal nature of the magnetic field energy density in the solar wind [PDF]
, 2007 The solar wind exhibits scaling typical of intermittent turbulence in the statistics of in situ fluctuations in both the magnetic and velocity fields.
Chapman, S.C. +6 more
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Development and application of a global magnetic field evolution model for the solar corona [PDF]
, 2009 Magnetic fields are fundamental to the structure and dynamics of the Sun’s corona. Observations show them to be locally complex, with highly sheared and twisted fields visible in solar filaments/prominences.
Yeates, Anthony Robinson
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Temporal Behaviors of Magnetic Helicity Injections by Self and Mutual Sunspot Rotations
The Astrophysical Journal, 2023 Magnetic helicity is a physical parameter used to quantify the complexity of magnetic fields, providing an indication of the energy state in the coronal magnetic structure.
Takahiro Hasegawa, Toshifumi Shimizu
doaj +1 more source
TANGLED MAGNETIC FIELDS IN SOLAR PROMINENCES [PDF]
The Astrophysical Journal, 2010 Solar prominences are an important tool for studying the structure and evolution of the coronal magnetic field. Here we consider so-called "hedgerow" prominences, which consist of thin vertical threads. We explore the possibility that such prominences are supported by tangled magnetic fields. A variety of different approaches are used.
van Ballegooijen, A. A., Cranmer, S. R.
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The evolution of a spot–spot-type solar active region which produced a major solar eruption
Frontiers in Astronomy and Space Sciences, 2023 Solar active regions are the main sources of large solar flares and coronal mass ejections. It is found that the active regions producing large eruptions usually show compact, highly sheared polarity inversion lines.
Lijuan Liu, Lijuan Liu, Lijuan Liu
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Interactions between solar neutrinos and solar magnetic fields [PDF]
Astroparticle Physics, 1997 17 pages, (+ 5 ps figs + aasms4.sty attached, uuencoded) Submitted to ...
Oakley, D. S., Snodgrass, Herschel B.
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