7 results
Analysis of quasi-periodic oscillations of position and brightness of details of the radio sources of the solar active regions based on observations made with the radio heliograph Nobeyama
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- Journal:
- Proceedings of the International Astronomical Union / Volume 2004 / Issue IAUS223 / June 2004
- Published online by Cambridge University Press:
- 14 March 2005, pp. 245-246
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- June 2004
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On the relationship between chromospheric oscillations of radio brightness at 1.76 cm with periods from minutes to hours and magnetic field changes
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- Journal:
- Proceedings of the International Astronomical Union / Volume 2004 / Issue IAUS223 / June 2004
- Published online by Cambridge University Press:
- 14 March 2005, pp. 281-282
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- June 2004
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On the microwave oscillations from active region NOAA 0139
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- Journal:
- Proceedings of the International Astronomical Union / Volume 2004 / Issue IAUS223 / June 2004
- Published online by Cambridge University Press:
- 14 March 2005, pp. 243-244
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- June 2004
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Observations of CME-related phenomena in a wide spectral range
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- Journal:
- Proceedings of the International Astronomical Union / Volume 2004 / Issue IAUS223 / June 2004
- Published online by Cambridge University Press:
- 14 March 2005, pp. 725-726
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- June 2004
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Multy octave spectral-polarization observations of solar atmosphere at radiowaves.
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- Journal:
- Proceedings of the International Astronomical Union / Volume 2004 / Issue IAUS223 / June 2004
- Published online by Cambridge University Press:
- 14 March 2005, pp. 613-614
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- June 2004
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Coronal Magnetic Fields from the Effect of the Double Inversion of Circular Polarization of Radio Emission
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- Journal:
- International Astronomical Union Colloquium / Volume 141 / 1993
- Published online by Cambridge University Press:
- 12 April 2016, pp. 302-305
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- 1993
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Diagnostics of the Solar Plasma Using Radio Observations with the RATAN-600
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- Journal:
- Symposium - International Astronomical Union / Volume 142 / 1990
- Published online by Cambridge University Press:
- 19 July 2016, pp. 483-488
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- 1990
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