Search Results - "Prosovetsky, D. V."
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A Tiny Eruptive Filament as a Flux-Rope Progenitor and Driver of a Large-Scale CME and Wave
Published in Solar physics (01-04-2016)“…A solar eruptive event SOL2010-06-13 observed with the Atmospheric Imaging Assembly (AIA) of the Solar Dynamics Observatory (SDO) has been extensively…”
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2
The Connection of Solar Wind Parameters with Radio and UV Emission from Coronal Holes
Published in Solar physics (01-11-2011)“…This paper presents the results of a comparison between observations of coronal holes in UV (SOHO EIT) and radio emission (17, 5.7 GHz, 327 and 150.9 MHz, from…”
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Observations and modeling of the spatial distribution and microwave radiation spectrum of the active region NOAA 11734
Published in Geomagnetism and Aeronomy (01-12-2015)“…Microwave observations of the solar active region NOAA 11734 were done on April 28–May 8, 2013 with SSRT and the RATAN-600 radio telescopes. As a result of…”
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Spectral characteristics of large-scale radio emission areas in coronal holes
Published in Geomagnetism and Aeronomy (01-12-2013)“…The spectra of the coronal hole radio emission in solar cycles 23 and 24 have been studied based on RATAN-600 data in the 4–16.5 GHz range at frequencies of…”
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5
The correlation between geomagnetic disturbances and topology of quasi-open structures in the solar magnetic field
Published in Geomagnetism and Aeronomy (01-12-2011)“…Results of photospheric magnetic field extrapolation in a potential approximation and of the technique for separating the open part of magnetic flux have…”
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6
Finding of low-contrast formations in the solar corona using a low contrast method
Published in Geomagnetism and Aeronomy (01-12-2009)“…Coronal holes, bright coronal points, filaments, and prominences are among the initial factors responsible for variability of the space weather conditions…”
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On the amplitude of the radio response of the active region magnetosphere to long-period natural oscillations of sunspots
Published in Geomagnetism and Aeronomy (01-12-2009)“…The following has been indicated for the cyclotron emission of microwave sources based on a simple modeling of a unipolar sunspot magnetosphere by the magnetic…”
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White-light polar jets on rising phase of solar cycle 24
Published in Journal of atmospheric and solar-terrestrial physics (15-10-2019)“…We studied coronal white-light jets in the polar regions of solar corona in 2009–2014. Jets were tracked on data producing by coronographs COR2/STEREO with the…”
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Spectral Characteristics of Large-Scale Radio Emission Areas in Coronal Holes
Published 13-12-2013“…Geomagnetism and Aeronomy, 2013, Vol. 53, No. 7, pp. 867-870. ISSN 0016-7932 The spectra of the coronal hole radio emission in solar cycles 23 and 24 have been…”
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10
A Tiny Eruptive Filament as a Flux-Rope Progenitor and Driver of a Large-Scale CME and Wave
Published 04-04-2016“…A solar eruptive event SOL2010-06-13 observed with SDO/AIA has been discussed in the contexts of the CME gebesis and an associated EUV transient in terms of a…”
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11
On the Relation of Brightness Temperatures in Coronal Holes at 5.7 and 17 GHz
Published in Publications of the Astronomical Society of Japan (25-02-2006)“…From the analysis of simultaneous observations with the Siberian Solar Radio Telescope and Nobeyama Radioheliograph we show that coronal holes are not uniform…”
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Fast-moving radio sources in the solar atmosphere
Published in Radiophysics and quantum electronics (01-11-1996)Get full text
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Some Features of Manifestations of Coronal Holes in Microwave Emission
Published in Publications of the Astronomical Society of Japan (2000)“…Abstract Using observational data from the SSRT, we have investigated the behavior of four mid- and low-latitude coronal holes. The coronal holes under study…”
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14
Fast-moving radio sources in the solar atmosphere
Published in Radiophysics and quantum electronics (1996)Get full text
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