Works matching IS 00167932 AND DT 2011 AND VI 51 AND IP 8
Results: 22
Observations of the dust radial velocity field in the F-corona on March 29, 2006.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1054, doi. 10.1134/S0016793211080287
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Studying ionospheric responses to magnetic storms depending on the local time of the storm main phase onset.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1105, doi. 10.1134/S0016793211080202
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Role of atmospheric circulation in the baric field response to the Earth's crossing of the interplanetary magnetic field sector boundaries.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1155, doi. 10.1134/S0016793211080214
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Structural and dynamic features of geoeffective coronal ejections.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1058, doi. 10.1134/S0016793211080238
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Formation of accelerated ion flows in Alfvén disturbances of the magnetotail.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1160, doi. 10.1134/S0016793211080032
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Solar faculae and waves propagating in the solar atmosphere.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1041, doi. 10.1134/S0016793211080263
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Magnetic declination measurements over European Russia and Siberia in the 18th century.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1146, doi. 10.1134/S0016793211080275
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Moreton wave, 'EIT wave', and type II radio burst as manifestations of a single wave front.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1045, doi. 10.1134/S0016793211080226
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Studying large-scale traveling ionospheric disturbances according to the data of oblique-incidence sounding.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1101, doi. 10.1134/S0016793211080196
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A study of the effect of different solar wind streams on spacecraft functioning.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1095, doi. 10.1134/S0016793211080172
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Coronal plasma heating problem.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1024, doi. 10.1134/S0016793211080317
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The correlation between geomagnetic disturbances and topology of quasi-open structures in the solar magnetic field.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1078, doi. 10.1134/S0016793211080342
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Transformation and absorption of MHD oscillations in plane-stratified models of the Earth's magnetosphere.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1165, doi. 10.1134/S0016793211080068
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Generation of a burst of geomagnetic pulsations in the 1-3 Hz frequency range in the daytime sector as a result of dramatic increases in the solar wind dynamic pressure.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1138, doi. 10.1134/S0016793211080305
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Long-period oscillation processes in sunspot groups (ground-based and exoatmospheric observations).
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1049, doi. 10.1134/S001679321108024X
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Electron concentration variations in the F1-region during magnetic storms in a low solar activity period.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1121, doi. 10.1134/S0016793211080251
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Using the nonlinear geometrical acoustics method in the problem of moreton and EUV wave propagation in the solar corona.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1015, doi. 10.1134/S0016793211080159
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Seasonal changes in the amplitude and phase of diurnal and semidiurnal variations in parameters of the midlatitude F2 layer under minimum solar activity conditions according to the data of an ionospheric station in Irkutsk (52.5°N, 104.0°E).
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1130, doi. 10.1134/S0016793211080330
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The solar corona during the eclipse of August 1, 2008.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1063, doi. 10.1134/S0016793211080299
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On the formation mechanism of the sporadic solar wind.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1083, doi. 10.1134/S0016793211080184
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Effect of a self-induced electric field on the electron beam kinetics and resulting hard X-ray and microwave emissions in flares.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1029, doi. 10.1134/S0016793211080329
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Results of Russian experiments dealing with the impact of powerful HF radiowaves on the high-latitude ionosphere using the EISCAT facilities.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1109, doi. 10.1134/S0016793211080160
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