Four Subjects in Solar Physics from the Point of View of the Electric Current Approach
coronal temperature solar wind sunspots solar flares
Abstract
Four major subjects in solar physics, the heating of the corona, the cause of the solar wind, the formation of sunspots and the cause of solar flares, are discussed on the basis of the electric current approach, a sequence of processes consisting of power supply(dynamo), transmission (currents/circuits) and dissipation(high coronal temperature, solar wind, sunspots and solar flares). This is because the four subjects have hardly been considered in terms of the electric current approach in the past, in spite of the fact that these subjects are various manifestations of electromagnetic processes. It is shown that this approach provides a new systematic way of considering each subject; (1) the long-standing issue of the coronal temperature, (2) the long-standing problem on the cause of the solar wind, (3)the presence of single spots(forgotten or dismissed in the past) and its relation to unipolar magnetic regions and (4) the crucial power/energy source and subsequent explosive processes of solar flares. The four subjects are obviously extremely complicated and difficult subjects, but it is hoped that the electric current approach might provide a new insight in considering the four subjects.
Downloads
How to Cite
References
S.-I Akasofu (2015) Single spots, unipolar magnetic regions, and pairs of spots. 41(11), 3698-3700.
S.-I Akasofu (2021) A morphological study of unipolar regions and the relationship with sunspots. 218, 105625.
S-I Akasofu, P Gray, L Lee (1980) A model of the heliospheric magnetic field configuration. 28(6), 609-615.
S.-I Akasofu, L.-C Lee (2019) On the explosive nature of auroral substorms and solar flares: The electric current approach. 186, 104-115.
H Alfven (1967) The secondapproach to cosmicalelectrodynamics.
A By, J Egeland, Holtet (1985) The Polar Cusp. 439-444.
H Alfven (1977) Electric currents in cosmic plasmas. 15(3), 271-284.
H Alfven (1981) Cosmic Plasma.
Hannes Alfven (1986) Double Layers and Circuits in Astrophysics. 14(6), 779-793.
M Aschwanden (2005) Physics of the Solar Corona.
H Babcock (1961) The Topology of the Sun's Magnetic Field and the 22-YEAR Cycle.. 133, 572.
R Bray, R Loughheard (1964) Sunspots.
James Chen, Jonathan Krall (2003) Acceleration of coronal mass ejections. 108(A11).
G Choe, L Lee ; A (1996) Evolution solar magnetic arches I. Ideal MHD evolution under footpoint shearing. 472, 360-388.
Alfred Clark, H Johnson (1967) Magnetic-field accumulation in supergranules. 2(4), 433-440.
Steven Cranmer (2009) Coronal Holes. 6.
L Fletcher, B Dennis, H Hadson, S Krucker, K Phollips, V Veronig, M Batterglia, L Bone, A Caspi, Q Chen, P Gallagher, P Grigis, H Ji, W Liu, R Milligan, M Temmer (2011) An observational review of solar flares. 159, 19-106.
R Howard, B Labonte (1980) The sun is observed to be a torsional oscillator with a period of 11 years. 239, L33.
Hiroki Kurokawa, Yoichiro Hanaoka, Kazunari Shibata, Yutaka Uchida (1987) Rotating eruption of an untwisting filament triggered by the 3B flare of 25 April, 1984. 108(2), 251-264.
T Karlsson (2012) The Acceleration Region of Stable Auroral Arcs. 227-240.
Ed, A Keiling, E Donovan, F Bagenal, T Karlsson (2012) Auroral Phenomenology and Magnetospheric Processes: Earth and Other Planets. 197.
V Kotov (1970) IAU Symposium No.43. 213-219.
Lou‐chuang Lee, Syun‐ichi Akasofu (2021) On the Causes of the Slow Solar Wind: 1. The Solar Unipolar Induction Currents. 126(7), 1-8.
T Li, J Drake, M Swisdak (2013) CORONAL ELECTRON CONFINEMENT BY DOUBLE LAYERS. 778(2), 144.
T Li, J Drake, M Swisdak (2014) DYNAMICS OF DOUBLE LAYERS, ION ACCELERATION, AND HEAT FLUX SUPPRESSION DURING SOLAR FLARES. 793(1), 7.
Robert Leighton (1969) A Magneto-Kinematic Model of the Solar Cycle. 156, 1.
D Mccomas, N Angold, H Elliott, G Livadiotis, N Schwadron, R Skoug, C Smith (2013) WEAKEST SOLAR WIND OF THE SPACE AGE AND THE CURRENT "MINI" SOLAR MAXIMUM. 779(1), 2.
P Mcintosh (1981) The Physics of Sunspots. 7, 7-54.
Min, S, J Chae (2009) The rotating sunspot in AR 10930. 258, 203-217.
E Parker (1958) Dynamics of the Interplanetary Gas and Magnetic Fields.. 128, 664.
E Parker (1992) Vortex attraction and the formation of sunspots. 390, 290.
Kan Yang, Liz Matson, Michael Choi, David Steinfeld, Brian Ottens, Patrick Coronado, Scott Applebaum (1963) Thermal Design for the New Era of Lunar Instruments: Lessons Learned from NASA Goddard Space Flight Center's Instrument Design Laboratory.
W Hess (1968) 4/68-2R NASA thesaurus: Subject terms for indexing scientific and technical information. Preliminary edition. NASA SP‐7030. December 1967. Scientific and Technical Information Division, Office of Technology Utilization. National Aeronautics and Space Administration, Washington, D.C. 3 volumes Sold by Superintendent of Documents: 1968 price, $8.50.. 19(2), 208-209.
M Rempel (2011) PENUMBRAL FINE STRUCTURE AND DRIVING MECHANISMS OF LARGE-SCALE FLOWS IN SIMULATED SUNSPOTS. 729(1), 5.
M Rees (1989) Physics and Chemistry of the Upper Atmosphere.
N Sheeley (1976) Energy released by the interaction of coronal magnetic fields. 47(1), 173-180.
S Solanki (2003) Sunspots: Anoverview. 11, 153-286.
M Stix (2002) Tagebuch.
Z Svestka (1976) Solar flares.
P Sweet (1958) 14. The neutral point theory of solar flares. 6, 123-134.
T Van Doorsselaere, A Srivasttava, P Antolin, N Magyare, S Farahanni (2020) Coronal heating by MHD waves. 216-140.
H Van De Hulst (1953) The chromosphere and the corona. 207-321.
V Vasyliunas (1975) Theoretical models of magnetic fiel line merging. 13, 303-336.
Nicholeen Viall, Joseph Borovsky (2018) Nine Outstanding Questions of Solar Wind Physics. 125(7), 26005.
Haimin Wang, M Ewell, H Zirin, Guoxiang Ai (1994) Vector magnetic field changes associated with X-class flares. 424, 436.
G Young, Y Xu, W Cao, H Wang, C Denker, T Rimmele (2004) Photospheric shear flows along the magnetic neutral line of active region 10486. 617, 151-154.
W Zhao, A Kosovichev, T Duvall (2001) Investigation of mass flows beneath a sunspot by time-distance helioseismology. 557, 384-388.
H Zirin (1988) Astrophysics of the Sun.
Daniel Verscharen, Kristopher Klein, Bennett Maruca (2019) The multi-scale nature of the solar wind. 16(1).
Published
2021-09-22
Issue
Section
License
Copyright (c) 2021 Authors and Global Journals Private Limited

This work is licensed under a Creative Commons Attribution 4.0 International License.