Results 21 to 30 of about 182,344 (339)
Splitting and Reconstruction of a Solar Filament Caused by Magnetic Emergence and Reconnection
The Astrophysical Journal, 2023 We present observations and interpretation of a nonerupting filament in NOAA active region (AR) 12827 that undergoes splitting and restructuring on 2021 June 4, using the high-resolution data obtained by the New Vacuum Solar Telescope, the Solar Dynamics
Zhike Xue +6 more
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The solar magnetic field [PDF]
Reports on Progress in Physics, 2006 The magnetic field of the Sun is the underlying cause of the many diverse phenomena combined under the heading of solar activity. Here we describe the magnetic field as it threads its way from the bottom of the convection zone, where it is built up by the solar dynamo, to the solar surface, where it manifests itself in the form of sunspots and faculae,
Solanki, S. +2 more
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The Magnetic Field in the Solar Atmosphere [PDF]
, 2014 This publication provides an overview of magnetic fields in the solar atmosphere with the focus lying on the corona. The solar magnetic field couples the solar interior with the visible surface of the Sun and with its atmosphere.
Solanki, Sami K. +2 more
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Association Between Magnetic Pressure Difference and the Movement of Solar Pores
The Astrophysical Journal, 2023 Solar pores are closely related to the concentration, dissipation, and transportation of solar magnetic flux. Their observable characteristics can provide constraints on models and simulations of magnetic flux emergence and formation.
Merlin M. Mendoza, Chia-Hsien Lin
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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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KamLAND, solar antineutrinos, and the solar magnetic field [PDF]
Physical Review D, 2003 In this work the possibility of detecting solar electron antineutrinos produced by a solar core magnetic field from the KamLAND recent observations is investigated. We find a scaling of the antineutrino probability with respect to the magnetic field profile in the sense that the same probability function can be reproduced by any profile with a suitable
Chauhan, Bhag C. +2 more
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A Statistical Study on Force-Freeness of Solar Magnetic Fields in the Photosphere
, 2012 It is an indisputable fact that solar magnetic fields are force-free in the corona, where force free fields means that current and magnetic fields are parallel and there is no Lorentz force in the fields.
Ai +34 more
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Diagnostics of Coronal Magnetic Fields Through the Hanle Effect in UV and IR Lines [PDF]
, 2016 The plasma thermodynamics in the solar upper atmosphere, particularly in the corona, are dominated by the magnetic field, which controls the flow and dissipation of energy.
Fineschi, S. +4 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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Measurements of Photospheric and Chromospheric Magnetic Fields
, 2015 The Sun is replete with magnetic fields, with sunspots, pores and plage regions being their most prominent representatives on the solar surface. But even far away from these active regions, magnetic fields are ubiquitous.
Centeno, Rebecca +4 more
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