Influence of Magnetically Conjugate Fragments of Auroral Emission Images on the Accuracy of Determining Eav of Precipitating Electrons


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Abstract

Results of magnetic conjugation of image fragments of auroral emissions at different altitudes along the magnetic field lines and preliminary results of evaluation of their influence on the accuracy of remote mapping of energy characteristics of precipitating electrons are presented. The results are obtained using the code of tracing being an integral part of the software Vector M intended for calculation of accompanying, geophysical, and astronomical information for the center of mass of a space vehicle (SV) and remote observation of aurora by means of Aurovisor-VIS/MP imager onboard the SV Meteor-MP to be launched.

About the authors

M. A. Banshchikova

National Research Tomsk State University

Author for correspondence.
Email: mba-tomsk@mail.ru
Russian Federation, Tomsk

I. N. Chuvashov

National Research Tomsk State University

Email: mba-tomsk@mail.ru
Russian Federation, Tomsk

A. K. Kuzmin

Space Research Institute of the Russian Academy of Sciences

Email: mba-tomsk@mail.ru
Russian Federation, Moscow

G. M. Kruchenitskii

Central Aerological Observatory of the Russian Federal Hydrometeorology and Environmental Monitoring Service, Moscow Institute of Physics and Technology (State University)

Email: mba-tomsk@mail.ru
Russian Federation, Moscow

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