scholarly journals Geomagnetic Pulsations, Blackout and Low-Latitude Aurorae Associated with Power Magnetic Storm

2021 ◽  
Vol 3 (4) ◽  
pp. 279-289
Author(s):  
Vladimir Parkhomov ◽  
Aleksandr Mikhalev ◽  
Konstantin Ratovskyi
Keyword(s):  
Solar Flare ◽  
Magnetic Storm ◽  
Geomagnetic Pulsation ◽  
Spectral Lines ◽  
Geomagnetic Pulsations ◽  
Radio Waves ◽  
Frequency Range ◽  
Low Latitude ◽  
Ionospheric Absorption ◽  
Solar Filament

The research analyzed the regularities of the dynamics of geomagnetic pulsation regimes in the frequency range 0.002–5 Hz, the generation of which reflects the interaction with the Earth's magnetosphere of the solar filament ejected by a powerful solar flare of 3B. We compared the dynamics of the change in the types and modes of geomagnetic pulsations with the dynamics of the atmosphere glow in two spectral lines and the total ionospheric absorption of radio waves. The study developed a possible model of the observed phenomenon.

A review of the October 21, 1989 red aurora seen in Japan and from the AKEBONO (EXOS-D) satellite

1992 ◽  
Vol 70 (7) ◽  
pp. 488-499 ◽  
Author(s):  
T. Oguti
Keyword(s):  
Electric Field ◽  
Magnetic Storm ◽  
Auroral Oval ◽  
Low Latitude ◽  
Terrestrial Environment ◽  
Acceleration Mechanism ◽  
Auroral Substorm ◽  
Field Fluctuations ◽  
The Difference ◽  
Auroral Expansion

Observations of the October 21, 1989 red aurora from the ground and AKEBONO satellite are reviewed mainly on the topics presented at the workshop on the aurora, held in Solar Terrestrial Environment Laboratory on January 17–18, 1991. Electric-field fluctuations associated with the auroral oval during the observation, together with auroral green-rayed structures embedded in the red veil strongly suggest that some electron acceleration mechanism was operative in the particle precipitation. Therefore this was not a typical stable auroral red (SAR) arc. This red aurora was most likely located at a low-latitude portion of an expansion aurora during an auroral substorm. The geomagnetic conditions at the time of the aurora were quite similar to those during the occurrence of a SAR arc. It occurred during a susbtorm that broke out at the maximum Dst (disturbance with storm time) phase of a magnetic storm, with an auroral expansion initiated from low latitude on a well-expanded auroral oval. The difference in conditions between a typical SAR arc and this red aurora with green-ray structures is to be studied further.

Long-period geomagnetic pulsations in the quasi-conjugate arctic and antarctic regions during the magnetic storm of April 16–17, 1999

2006 ◽  
Vol 46 (5) ◽  
pp. 622-634 ◽  
Author(s):  
O. V. Kozyreva ◽  
N. G. Kleimenova ◽  
A. E. Levitin ◽  
J. Watermann
Keyword(s):  
Magnetic Storm ◽  
Geomagnetic Pulsations ◽  
Long Period
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