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1.
Adv Space Res ; 14(10): 77-84, 1994 Oct.
Artigo em Inglês | MEDLINE | ID: mdl-11540023

RESUMO

The radiation environment is of special concern when the spaceship flies in deep space. The annual fluence of the galactic cosmic rays is approximately 10(8) cm-2 and the absorbed dose of the solar cosmic rays can reach 10 Gy per event behind the shielding thickness of 3-5 g cm-2 Al. For the radiation environment monitoring it is planned to place a measuring complex on the space probes "Mars" and "Spectr" flying outside the magnetosphere. This complex is to measure: cosmic rays composition, particle flux, dose equivalent, energy and LET spectra, solar X-rays spectrum. On line data transmission by the space probes permits to obtain the radiation environment data in space.


Assuntos
Radiação Cósmica , Meio Ambiente Extraterreno , Modelos Teóricos , Monitoramento de Radiação/instrumentação , Atividade Solar , Transferência Linear de Energia , Doses de Radiação , Proteção Radiológica , Voo Espacial/instrumentação , Astronave
2.
Adv Space Res ; 14(10): 771-8, 1994 Oct.
Artigo em Inglês | MEDLINE | ID: mdl-11540024

RESUMO

A possibility of a manned mission to Mars without exceeding the current radiation standards is very doubtful during the periods of minimum solar activity since the dose equivalent due to galactic cosmic rays exceeds currently recommended standards even inside a radiation shelter with an equivalent of 30 g cm-2 aluminum. The radiation situation at the time of maximum solar activity is determined by the occurrence of major solar proton events which are exceedingly difficult to forecast. This paper discusses the radiation environment during a manned mission to Mars in the years between minimum and maximum solar activity when the galactic cosmic ray intensity is considerably reduced, but the solar flare activity has not yet maximized.


Assuntos
Radiação Cósmica , Atividade Solar , Voo Espacial , Marte , Concentração Máxima Permitida , Doses de Radiação , Proteção Radiológica , Fatores de Tempo
3.
Adv Space Res ; 12(2-3): 435-9, 1992.
Artigo em Inglês | MEDLINE | ID: mdl-11537041

RESUMO

Possible manned flights toward Mars are discussed from the viewpoint of radiation hazard. A standard situation is considered for the fast two times crossing of the Earth radiation belts. The flight to Mars is shown to be practically impossible without a special system of radiation shelters, because of the effect of penetrating galactic and solar radiations which are responsible for almost maximum permissible doses. But even in case there were radiation shelters on board the spacecraft their flights are undesirable in the periods of maximum and minimum solar activity. It would obviously be worthwhile to schedule Martian flights for intervals in between minima and maxima of 11-year cycles of solar activity when primary cosmic rays levels are considerable reduced and flare activity is not yet sufficiently high. It should be mentioned that it would not be easy to select such allowed intervals. Further studies of that aspect are discussed.


Assuntos
Radiação Cósmica/efeitos adversos , Marte , Monitoramento de Radiação/normas , Proteção Radiológica/normas , Sistema Solar , Voo Espacial/normas , Astronautas , Relação Dose-Resposta à Radiação , Trajes Gravitacionais , Humanos , Doses de Radiação , Astronave , Fatores de Tempo
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