Computer Science
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..587i&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, July-Aug. 1985, p. 587-591. In Russian.
Computer Science
Auroral Electrojets, Interplanetary Medium, Longitude, Magnetic Storms, Magnetospheric Instability, Space Plasmas, Convective Flow, Magnetoactivity, Rarefied Plasmas
Scientific paper
A comparison of data of five interplanetary and magnetospheric flare disturbances shows that dense and rarefied interplanetary clouds generate magnetospheric storms from the western auroral electrojet situated at the morning and night meridians, respectively. This result can be explained by the presence of two branches of magnetospheric convection and their different dependences on the concentration of interplanetary plasma. Of decisive significance are deceleration (acceleration) of the main convection branch with increase (decrease) in density, the formation of slow (fast) convection waves in the reverse flow, their entrainment (lack of entrainment) by the earth's rotation, and the intensification (reduction) of convection on closed field lines with increase (decrease) in concentration.
Ivanov K. G.
Mikerina N. V.
Zaitsev Alexander N.
No associations
LandOfFree
Longitudinal position of the western auroral electrojet and the density of interplanetary hydromagnetic clouds does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Longitudinal position of the western auroral electrojet and the density of interplanetary hydromagnetic clouds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Longitudinal position of the western auroral electrojet and the density of interplanetary hydromagnetic clouds will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-753290