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ISSN: 1023-5086

ru/

ISSN: 1023-5086

Scientific and technical

Opticheskii Zhurnal

A full-text English translation of the journal is published by Optica Publishing Group under the title “Journal of Optical Technology”

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УДК: 523.9–739–355: 159.938.(202)

The Space Solar Patrol and some problems of manned flight to Mars

For Russian citation (Opticheskii Zhurnal):

Коваленок В.В., Авакян С.В., Боровкова О.К., Воронин Н.А. Космический солнечный патруль и некоторые проблемы пилотируемого полета к Марсу // Оптический журнал. 2005. Т.72. №8 С. 49-53.

 

Kovalenok V.V., Avakyan S.V., Voronin N.A., Borovkova O.K. The Space Solar Patrol and some problems of manned flight to Mars [in Russian] // Opticheskii Zhurnal. 2005. V. 72. No 8. P. 49-53.

For citation (Journal of Optical Technology):

Kovalenok V.V., Avakyan S.V., Voronin N.A., Borovkova O.K. The Space Solar Patrol and some problems of manned flight to Mars // Journal of Optical Technology. 2005. V. 72. № 8. P. 615-619. https://doi.org/10.1364/JOT.72.000615

Abstract:

In interplanetary flight, after large solar flares, the cosmonauts are subjected to the action of energetic solar protons and electrons. They have an especially strong effect during extravehicular activity or residence (in the future) on the surface of Mars when they spend an extended time there. Such particles reach the orbits of the earth and Mars with a delay of several hours relative to solar x rays and UV radiation. Therefore, there is always time to predict their appearance, in particular, by means of an x-ray-UV radiometer from the apparatus complex of the Space Solar Patrol (SSP) that is being developed by the coauthors of this article. During manned flight to Mars, the human organism will be outside the region of action of the earth's magnetic field and its pulsations for a long time, and this can, according to observations made in orbital flights, create a state of discomfort in the crew. Along with special experiments verifying these observations, it is proposed to investigate the connection between the behavior of the geomagnetic pulsations and the UV flares recorded by the SSP apparatus.

OCIS codes: 000.1430, 000.3110.