Abstract
Some morphological features of solar magnetic fields in the chromosphere and corona are considered based on studying various observational data. These data are compared to the results of observation of the solar wind and interplanetary magnetic field, as well as to the data on fluxes of solar cosmic rays. New specific features are found in the solar wind structure, and new additional indications of sources of the solar wind are obtained. The properties of the active regions and coronal holes are considered. A model of the ascending stream-like plasma flow is suggested. It flows around the discrete arched magnetic field tubes in the solar atmosphere and stretches them out into interplanetary space.
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Boguslavskaya, E.Ya., Structure of the Solar Corona, in Trudy GAISh im. P.K. Shternberga (Transactions of Shternberg Astronomical Institute), 1949, vol. 19.
Vsekhsvyatskii, S.K., Nikol’skii, G.M., Ivanchuk, V.I., et al., Solnechnaya korona i korpuskulyarnoe izluchenie v mezhplanetnom prostranstve (Solar Corona and Corpuscular Radiation in the Interplanetary Space), Kiev: Izd. KGU, 1965.
Mustel, E.R., Solar Corpuscular Fluxes and Geomagnetism, Astron. Zh., 1964, vol. 41, no. 5, p. 777.
Mustel, E.R., Quasi-Stationary Outflow of Gases from Active Regions on the Sun and the Coronal Holes, Astron. Zh., 1980, vol. 57, no. 2, p. 225.
Gordon, I.M., Radar Investigations of the Sun and Acceleration of the Solar Wind above Active Regions, Preprint of Inst. of Radio Elect. of Ukr. SSR Acad. Sci., Kharkov, 1973, no. 30.
Vernov, S.N., Tverskoi, B.A., Lyubimov, G.P., et al., Variations of Cosmic Ray Intensity and the Solar Wind, Izv. Akad. Nauk SSSR, Ser. Fiz., 1975, vol. 39, no. 2, p. 340.
Lyubimov, G.P. and Pereslegina, N.V., Imprinting of the Solar Atmosphere in the Solar Wind, Astronomicheskii Tsirkulyar AN SSSR, 1984, no. 1323, p. 2.
Lyubimov, G.P. and Pereslegina, N.V., Imprinted Structure of the Solar Chromosphere and Corona in the Solar Wind and Interplanetary Magnetic Field, Astron. Zh., 1985, vol. 62, no. 4, p. 780.
King, J.H., Interplanetary Medium Data Book, NSSDC/WDC-A-R S S 77-04, Goddard Space Flight Center, Greenbelt, Maryland, 20771, 1977–1979.
Solar Geophysical Data, Boulder, Colorado, 1967–1977.
Report UAG-70, 1979.
Zombeck, M.V., Yaiana, G.S., Haggerty, R., et al., An Atlas of Soft X-Ray Images of the Solar Corona from Skylab, Astrophys. J., Supplement Series, 1978, vol. 38, p. 69.
Lyubimov, G.P., Stretching of Magnetic Loops in the Solar Atmosphere, Astronomicheskii Tsirkulyar AN SSSR, 1986, no. 1441, p. 5.
Armstrong, J.W. and Woo, R., Solar Wind Motion within 30 R: Spacecraft Radio Scintillation Observations, Astron. Astrophys., 1981, vol. 103, no. 2, p. 415.
Efimov, A.I., Yakovlev, O.I., Razmanov, V.M., and Shtrykov, V.K., Turbulence of Near-Solar Plasma and the Solar Wind Velocity according to Radio Occulation Experiment onboard the Venera-10 Spacecraft, Pis’ma Astron. Zh., 1977, vol. 3, no. 7, p. 322.
Lotova, N.A., Blums, D.F., and Vladimirskii, K.V., Interplanetary Scintillation and the Structure of the Solar Wind Transonic Region, Astron. Astrophys., 1985, vol. 150, p. 266.
Lyubimov, G.P., Traces of Coronal Holes in the Solar Wind, Astronomicheskii Tsirkulyar AN SSSR, 1986, no. 1448, p. 7.
Woo, R. and Habbal, S.R., The Origin of the Solar Wind. A Novel Way of Looking at the Solar Corona Reveals a Hidden “Imprint” of the Sun, American Societist, 2002, vol. 90, p. 532.
Lyubimov, G.P., Kontor, N.N., Pereslegina, N.V., and Ignat’ev, P.P., Anisotropy of Solar Protons and Irregularities of the Interplanetary Medium, Izv. Akad. Nauk SSSR, Ser. Fiz., 1976, vol. 40, no. 3, p. 462.
Lyubimov, G.P. and Chuchkov, E.A., A System of Loop-Like Interplanetary Traps in SCR in June 1974, Kosm. Issled., 1991, no. 6, p. 911.
Lyubimov, G.P., Deceleration of Shock Waves from Solar Flares in the Interplanetary Space, Astronomicheskii Tsirkulyar AN SSSR, 1968, no. 488, p. 4.
Lyubimov, G.P. and Pereslegina, N.V., Deceleration of the Solar Plasma Flows, Astronomicheskii Tsirkulyar AN SSSR, 1974, no. 836, p. 1.
Borrini, G., Wilcox, J.M., Gosling, J.T., et al., Solar Wind Helium and Hydrogen Structures near Heliospheric Current Sheet: A Signal of Coronal Streamers at 1 AU, J. Geophys. Res., 1981, vol. 86, p. 4564.
Artsimovich, L.A., Elementarnaya fizika plazmy (Elementary Physics of Plasmas), Moscow: Gosatomizdat, 1963.
Lyubimov, G.P., A Stereoscopic Method of Analysis of X-Ray Images of the Sun, Astronomicheskii Tsirkulyar AN SSSR, 1985, no. 1362, p. 4.
Delone, A.B., Makarova, E.A., and Sikora, Yu., Elevation of Arches of Monochromatic Corona during the Eclipse on July 31, 1981, Pis’ma Astron. Zh., 1984, vol. 10, no. 4, p. 311.
Pereslegina, N.V., Lyubimov, G.P., and Tulupov, V.I., Quasi-Stationary Plasma Streams at the Declining Solar Activity, in Materialy VII Leningradskogo mezhdunarodnogo seminara (Proc. 7th Leningrad Intern. Seminar), Leningrad, 1975, p. 185.
Lyubimov, G.P., Solar Activity and Solar Wind, in Variatsii kosmicheskikh luchei (Variations of Cosmic Rays), IZMIR AN SSSR, 1985, p. 126.
Lyubimov, G.P., Sources of the Solar Wind, in Issledovaniya Solnechnoi Plazmy (Studies of Solar Plasma), B.V. Somov, Ed., Ashkhabad: Ylym, 1989, p. 248.
Wolfe, J.H., The Large-Scale Structure of the Solar Wind, Solar Wind, NASA, 1972.
Gosling, J.T., Asbridge, J.R., Bame, S.J., and Feldman, W.C., Solar Wind Speed Variations: 1962–1974, J. Geophys. Res., 1976, vol. 81, no. 28, p. 5061.
Stozhkov, Yu.I. and Charakhch’yan, T.N., The Role of Heliographic Latitude of Sunspots in 11-Year Modulation of Galactic Cosmic Rays, Izv. Akad. Nauk SSSR, Ser. Fiz., 1970, vol. 34, p. 2439.
Tsap, T.T. and Laba, I.S., Time Evolution of the Chromosphere Network, Izv. Krym. Astr. Observ., 1973, no. 48, p. 73.
Kotov, V.A. and Levitskii, L.S., Izv. Krym. Astr. Observ., 1983, no. 66, p. 110.
Kontor, N.N., Lyubimov, G.P., and Khotilovskaya, T.G., An Analysis of Data on Cosmic Rays in Interplanetary Space Based on the Model of Active Process in the Solar Medium, in Kosmicheskie luchi (Cosmic Rays), Moscow: Sovetskoe Radio, 1979, no. 20, p. 21.
Rickett, B.J. and Coles, W.A., Solar Wind, 1983, no. 5.
Lyubimov, G.P., Chuchkov, E.A., and Kontor, N.N., Some Features in Solar Wind and Solar Activity, in Solar Maximum Analysis. Proc. of the Int. Workshop Held in Irkutsk, USSR, 17–24 June, 1985, Novosibirsk: Nauka, 1988, p. 394.
Coronal Holes and High Speed Wind Streams, Zirker, J.B., Ed., Colorado Assoc. University Press, 1977.
Lyubimov, G.P., Some Features of the Sun’s Magnetic Field and Corona and Their Role in the solar Wind Formation, Novosibirsk: Nauka, 1989, p. 292.
Lyubimov, G.P. and Kontor, N.N., Ascending Flows in the Solar Atmosphere, Problemy fiziki solnechnykh vspyshek (Issues of Physics of Solar Flares), IZMIR AN, 1986, no. 3, p. 153.
Krasotkin, S. and Chumak, O., Quantitative Parameters of Magnetic and Velocity Fields in Solar Active Regions, Proc. 10th European Solar Physics Meeting, Solar Variability: From Core to Outer Frontiers’, Prague, Czech Republic, 9–14 September, 2002, ESA SP-506, December 2002, p. 447.
Lyubimov, G.P., Reflective Model of SCR Motion in Loop-Like Traps, Astronomicheskii Tsirkulyar AN SSSR, 1988, no. 1531, p. 19.
Lyubimov, G.P., Diagnostic Method of Studying Interplanetary Magnetic Field, Solar Wind Plasma, and Their Sources on the Sun, Izv. Akad. Nauk, Ser. Fiz., 2003, vol. 67, no. 3, p. 353.
Lyubimov, G.P., Local Radiation Belts of the Sun (Quasi-Stationary Coronal and Heliospheric Giant Traps for Solar Cosmic Rays), Kosm. Issled., 2002, vol. 40, no. 6, pp. 610–615.
Lyubimov, G.P., solar Flare Peculiarities: A Hypothesis for a New Phenomenological Model, Kosm. Issled., 2000, vol. 38, no. 6, pp. 619–623.
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Original Russian Text © G.P. Lyubimov, 2006, published in IKosmicheskie Issledovaniya, 2006, Vol. 44, No. 2, pp. 118–135.
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Lyubimov, G.P. Ascending flows in the solar atmosphere and formation of the solar wind. Cosmic Res 44, 111–127 (2006). https://doi.org/10.1134/S0010952506020043
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DOI: https://doi.org/10.1134/S0010952506020043