Journal Solar-Terrestrial Physics. Vol. 2, Iss. 2, 2016
Материал из ISTP SB RAS.
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| Yazev S.A., Mordvinov A.V., Dvorkina-Samarskaya A.A. Corona during the total solar eclipse on March 20, 2015, and 24 cycle development
| 3–14
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| Zhdanov D.A., Lesovoi S.V., Tokhchukova S.Kh. Sources of type III solar microwave bursts
| 15–27
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| Rybak A.L. Some peculiarities in longitude distribution of sunspot groups over last four eleven-year solar cycles
| 28–36
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| Guglielmi A.V. On the phenomenological theory of magnetic storms
| 37–45
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| Kozyreva O.V., Pilipenko V.A., Engebretson M.J., Klimushkin D.Yu., Mager P.N. Correspondence between the ULF wave power spatial distribution and auroral oval boundaries
| 46–65
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| Penzin M.S., Ilyin N.V. Modeling of Doppler frequency shift in multipath radio channels
| 66–76
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| Karpov I.V., Borchevkina O.P., Dadashev R.Z., Ilminskaya A.V. Influence of meteorological storms on ionospheric parameters in Baltic region in 2010
| 77–81
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| Skomorovsky V.I., Kushtal G.I., Lopteva L.S., Proshin V.A., Trifonov V.D., Chuprakov S.A., Khimich V.A. Chromospheric telescope of Baikal Astrophysical Observatory. New light
| 82–103
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| Savin M.G., Izrailsky Yu.G. New capabilities of Chetaev's model
| 104–114
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