Диссертация (1149582), страница 26
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— С. 154–169.43. Финкельштейн А. М., Топчило H. A., Петерова H. Г., Ахмедов Ш. Б.,Борисевич Т. П., Дьяков А. А., Ильин Г. Н., Ипатов А. В., Коржавин А. Н., Рахимов И. А., Смоленцев С. Г. Предварительные результаты наблюдений солнечного затмения 29.03.2006 г. на радиотелескопах РТ–32 (Светлое), РТ–32 (Зеленчукская), РТ–2,5 (Петергоф) и БПР(Пулково) // Труды ИПA РАН. — 2006.
— Вып. 14. — С. 33–42.44. Юровский Ю. Ф. Радиоизлучение невозмущенного Солнца и локальных источников на волнах 5, 10.7, 12 и 95 см по наблюдениям затмения4 января 2011 г в Крыму // Изв. Крымской Астрофиз. Обс. — 2011. —Т. 108, № 0. — С. 45–57.15145. A purely polarized S-component at 17 GHz / K. Shibasaki, S. Enome,H. Nakajima, M.
Nishio, T. Takano, Y. Hanaoka, C. Torii, H. Sekiguchi,S. Kawashima, T. Bushimata, N. Shinohara et al. // Publ. of the Astron.Soc. of Japan. — 1994. — Vol. 46, N 2. — P. L17–L20.46. Alissandrakis C. E., Kundu M. R. Polarized horseshoes around sunspotsat 6 centimeter wavelength // Astrophysical Journal. — 1982. — Vol. 253,N 2. — P. L49–L52.47. Alissandrakis C.
E., Kundu M. R. Center-to-limb variation of a sunspotassociated microwave source // Astron. and Astrophys. — 1984. — Vol. 139,N 2. — P. 271–284.48. Alissandrakis C. E., Kundu M. R., Lantos P. A model for sunspot associated emission at 6 cm wavelength // Astron. and Astrophys. — 1980. —Vol. 82, N 1-2. — P. 30–40.49. Avrett E. N., Loeser R. Models of the Solar Chromosphere and TransitionRegion from SUMER and HRTS Observations: Formation of the ExtremeUltraviolet Spectrum of Hydrogen, Carbon, and Oxygen // Astrophys.
J.Suppl. Ser. — 2008. — Vol. 175. — Iss. 1. — P. 229–276.50. Bezrukov D., Ryabov B., Peterova N., Topchilo N. Sharp Changes In theOrdinary Mode Microwave Emission from a Stable Sunspot: Model Analysis // Latv.J. of Phys. and Tech.Sciences. — 2011. — Vol. 48, N 2. — P. 56–69.51. Bogod V. M., Peterova N. G., Ryabov B. I., Topchilo N. A. Recording ofan Emission with a Reduced Brightness in the Region of a Strong SunspotMagnetic Field // Cosmic Research. — 2015. — Vol.
53, N 1. — P. 10–20.52. Brosius J. W., White S. M. Close Association of an Extreme-UltravioletSunspot Plume with Depressions in the Sunspot Radio Emission // Astrophys. J. — 2004. — Vol. 601. — Iss. 1. — P. 546–558. — doi:10.1086/380394.53. Fontenla J. M., Avrett E., Thuillier G., Harder J. Semiempirical Models of the Solar Atmosphere. I. The Quiet- and Active Sun Photosphereat Moderate Resolution // Astrophys. J. — 2006. — Vol. 639.
— Iss. 1. —P. 441–458.15254. Fontenla J. M., Curdt W., Haberreiter M., Harder J., Tian H. Semiempirical Models of the Solar Atmosphere. III. Set of Non-LTE Models forFar-Ultraviolet/Extreme-Ultraviolet Irradiance Computation // Astrophys.J. — 2009. — Vol. 707. — Iss. 1.
— P. 482–502.55. Gary D. E., G. J. Hurford G. J. Radio spectral diagnostics / Ed. by D. E.Gary, C. U. Keller. — Dordrecht: Kluver, 2004. — Vol. 314 of Astrophysicsand Space Science Library. — P. 71–87.56. Grebinskij A., Shibasaki K., Zhang H. Microwave Measurements of the Solar Magnetic Fields at Chromosphere-Corona // Solar Physics with RadioObservations. Proceedings of Nobeyama Symposium.
1998. NRO Report479. / Ed. by T. Bastian, N. Gopalswamy, K. Shibasaki. — 1999. — P. 59–64.57. Györi L., Baranyi T., Ludmány A. Photospheric data programs at theDebrecen Observatory // The Physics of Sun and Star Spots / Ed. byD. P. Choudhary, K. G. Strassmeier. — Vol. 6 of Proceedings of the International Astronomical Union (Symposium S273). — 2011. — P. 403–407. —doi:10.1017/S174392131101564X.58. Hermans L. M., Lindsey C. Solar chromospheric modeling based on submillimeter limb brightness profile // Astrophys.
J. — 1986. — Vol. 310, N 1. —P. 907–911.59. Hildebrandt J., Seehafer N., Krüger A. An example of a solar S-componentmodel calculation using force-free magnetic field extrapolation // Astron.and Astrophys. — 1984. — Vol. 134, N 1. — P. 185–188.60. Iwai K., Koshiishi H., Shibasaki K., Nozawa S., Miyawaki S., Yoneya T.Chromospheric Sunspots in the Millimeter Range as Observed by theNobeyama Radioheliograph // Astrophys. J.
— 2016. — Vol. 816. — P. 91. —DOI:10.3847/0004-637X/816/2/91.61. Iwai K., Shimojo M. Observation of the Chromospheric Sunspot at Millimeter Range with the Nobeyama 45 m Telescope // Astrophys. J. — 2015. —Vol. 804. — P. 48. — DOI:10.1088/0004-637X/804/1/48.15362. Kakinuma T., Swarup G. A Model for the Sources of the Slowly Varying Component of Microwave Solar Radiation // Astrophys. J. — 1962. —Vol. 136. — P. 975–994.
— DOI:10.1086/147450.63. Klvana M., Kaltman T. I., Bumba V. The depths of sunspot magnetic fieldsources calculated on the basis of magnetographic measurements in twospectral lines // SOLMAG 2002. Proceedings of the Magnetic Couplingof the Solar Atmosphere Euroconference / Ed. by H. Sawaya-Lacoste.
—Vol. 505 of ESA Special Publication. — 2002. — P. 449–452.64. Korzhavin A. N., Arreola J. I., Casselin L. V., Timofeeva G. M. Radioobservations of the 24 of December 1973 solar eclipse // Boletin del Institutode Tonantzintla. — 1974. — Vol. 1, N 2. — P. 55–71.65. Korzhavin A. N., Peterova N. G., Topchilo N. A. Ring-Shaped CyclotronRadiation Source on the Example of the NOAA 11140 Active Region According to High Angular Resolution Observations // Geomagnetism andAeronomy. — 2012. — Vol. 52, N 7. — P. 867–874.66. Krüger А., Hildebrandt J., Furstenberg F.
A working model of the solarS-component radio emission // Astron. and Astrophys. — 1985. — Vol. 143,N 1. — P. 72–76.67. Kundu M. R., Alissandrakis C. E. Structure and polarization of activeregion microwave emission // Solar Phys. — 1984. — Vol. 94. — Iss. 2. —P. 249–283.68. Kundu M. R., Alissandrakis C. E., Bregman J. D. 6 centimeter observations of solar active regions with 6"resolution // Astrophysical Journal. —1977. — Vol. 213, N 1.
— P. 278–295.69. Landi E., Chiuderi Drago F. The Quiet-Sun Differential Emission Measurefrom Radio and UV Measurements // Astrophysical Journal. — 2008. —Vol. 675, N 2. — P. 1629–1636. — DOI:10.1086/527285.70. Lang K. R., Willson R. F. Polarized horseshoes around sunspots at 6 centimeter wavelength // Astrophysical Journal. — 1982. — Vol. 255, N 2. —P.
L111–L117.71. Lantos P. A model for thermal gyromagnetic radioemission from solar active regions // Ann. Astrophys. — 1968. — Vol. 31, N 1. — P. 105–113.15472. Lee J. Radio Emissions from Solar Active Regions // Space Sci. Rev. —2007. — Vol. 133. — Iss. 1–4. — P. 73–102. — DOI:10.1007/s11214-007-92062.73. Lee J. W., Gary D. E., Hurford G. J. Microwave emission from a sunspot.II - The center-to-limb variation // Solar Physics. — 1993. — Vol.
144,N 2. — P. 349–360.74. Loukitcheva M., Solanki S. K., White S. M. The chromosphere abovesunspots at millimeter wavelengths // Astron. and Astrophys. — 2014. —Vol. 561. — A133.75. Low B. C. Exact static equilibrium of vertically oriented magnetic fluxtubes. I - The Schlueter-Temesvary sunspot // Solar Phys. — 1980. —Vol. 67. — Iss. 1. — P. 57–77. — DOI:10.1007/BF00146682.76.
McConnel D., Kundu M. R. VLA observations of fine structures in a solar active region at 6 centimeter wavelength // Astrophysical Journal. —1984. — Vol. 279, N 1. — P. 421–426.77. Neupert W. M., Brosius J. W., Thomas R. J., Thompson W. T. Evidencefor mass outflow in the low solar corona over a large sunspot // Astrophysical Journal. — 1992. — Vol. 392, N 2.
— P. L95–L98. — DOI:10.1086/186434.78. Nindos A., Kundu M. R., White S. M., Shibasaki K., Gopalswamy N. SoftX-Ray and Gyroresonance Emission above Sunspots // Astroph. J. Suppl.Ser. — 2000. — Vol. 130. — Iss. 2. — P. 485–499. — DOI:10.1086/317355.79. Nitta N. V., DeRosa M. L. A Comparison of Solar Open Field RegionsFound by Type III Radio Bursts and the Potential Field Source SurfaceModel // Astrophysical Journal. — 2008. — Vol. 673.
— Iss. 2. — P. L207–L210. — DOI:10.1086/527548.80. Obridko V. N., Staude J. A two-component working model for the atmosphere of a large sunspot umbra // Astron. and Astrophys. — 1988. —Vol. 189, N 1–2. — P. 232–242.81. Peterova N. G., Topchilo N. A., Opeikina L. V., Agalakov B. V., Borisevich T.
P., Lubyshev B. I. Anomalous Polarization Features of the Cyclotron Radiation Source in the NOAA 7123 Active Region: The Structure,155Dynamics, and Reasons of Occurrence // Geomagnetism and Aeronomy. —2013. — Vol. 53, N 8. — P. 1000–1006.82. Ryabov B. I., Gary D. E., Peterova N. G., Shibasaki K., Topchilo N. A. Reduced Coronal Emission Above Large Isolated Sunspots // Solar Physics. —2015. — Vol. 290. — Iss. 1. — P. 21–35.83. Socas-Navarro H. Semiempirical Models of Solar Magnetic Structures //Astrophys. J.
Suppl. Ser. — 2007. — Vol. 169. — Iss. 2. — P. 439–457.84. Solanki S. K. Sunspots: An overview // Astron. and Astrophys. Rev. —2003. — Vol. 11. — P. 153–286.85. Solov’ev A. A., Kirichek E. A. Analytical Model of an Asymmetric Sunspotwith a Steady Plasma Flow in its Penumbra // Solar Phys. — 2016. —Vol. 291.
— Iss. 6. — P. 1647–1663.86. Vernazza J. E., Avrett E. H., Loeser R. Structure of the solar chromosphere. III. Models of the EVU brightness components of the quiet sun //Astroph. J. Suppl. Ser. — 1981. — Vol. 45, N 2. — P. 635–725.87. Vourlidas A., Bastian T. S. Multiband VLA Observations of Solar ActiveRegions: Implications for the Distribution of Coronal Plasma // Astrophysical Journal. — 1996. — Vol.
466, N 2. — P. 1039–1053.88. Vourlidas A., Bastian T. S., Aschwanden M. J. The Structure of the SolarCorona above Sunspots as Inferred from Radio, X-Ray, and Magnetic FieldObservations // Astrophysical Journal. — 1997. — Vol. 489. — Iss. 2. —P. 403–425.89. Vourlidas A., Bastian T. S., Nitta N., Aschwanden M. J. Joint Radioand Soft X-Ray Imaging of an ‘Anemone’ Active Region // Solar Phys. —1996. — Vol. 163. — Iss.
1. — P. 99–120.90. White S. M. Coronal Magnetic Field Measurements through GyroresonanceEmission / Ed. by D. E. Gary, C. U. Keller. — Dordrecht: Kluver, 2004. —Vol. 314 of Astrophysics and Space Science Library. — P. 89–113.91. White S. M., Kundu M. R., Gopalswamy N. Strong magnetic fields andinhomogeneity in the solar corona // Astrophysical Journal. — 1991. —Vol. 366.
— Iss. 2. — P. L43–L46. — DOI:10.1086/185905.15692. Zhivanovich I., Solov’ev A. A., Smirnova V. V., Riehokainen A., Nagnibeda V. G. Radial profile of sunspot magnetic field on the SDO data // Astrophys. Space Sci. — 2016. — Vol. 361. — Iss. 3:102. — P. 1–6. —DOI:10.1007/s10509-016-2681-8.93. Zirin H., Baumert B. M., Hurford G. J. The microwave brightness temperature spectrum of the quiet sun // Astrophysical Journal. — 1991. —Vol. 370.
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