Terrestrial Space Radiation and Its Biological Effects 1988
DOI: 10.1007/978-1-4613-1567-4_51
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Space Radiation Dosimetry on U.S. and Soviet Manned Missions

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Cited by 13 publications
(4 citation statements)
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“…Radiation hazards posed by solar energetic particles (SEP), protons and highly charged energetic particles (HZE) of galactic cosmic rays (GCR) are worrisome for exploration missions, when the chances of solar flares increase. Passive dosimetry recorded levels from 10-87 mrad/day in low Earth orbit (200-500 km altitudes) to 44-1 27 mrad/day on the moon (3). GCR predominate at the lowest altitudes; dose-rates increase tenfold at higher altitudes (mostly trapped protons); secondary radiation, mostly neutrons, arises from HZE interacting with spacecraft material.…”
Section: What Is the Spaceflight Environment?mentioning
confidence: 99%
“…Radiation hazards posed by solar energetic particles (SEP), protons and highly charged energetic particles (HZE) of galactic cosmic rays (GCR) are worrisome for exploration missions, when the chances of solar flares increase. Passive dosimetry recorded levels from 10-87 mrad/day in low Earth orbit (200-500 km altitudes) to 44-1 27 mrad/day on the moon (3). GCR predominate at the lowest altitudes; dose-rates increase tenfold at higher altitudes (mostly trapped protons); secondary radiation, mostly neutrons, arises from HZE interacting with spacecraft material.…”
Section: What Is the Spaceflight Environment?mentioning
confidence: 99%
“…Such an experiment -again using the rad54-3 mutant of yeastwas flown on STS-84; the results will be reported elsewhere. The special radiation field in space [1,2] has also to be taken into account. It consists mainly of charged particles and their secondaries created by interaction with spacecraft material and the human body.…”
Section: Discussionmentioning
confidence: 99%
“…Estimation of radiation risk in space is a complicated matter, and one cannot simply rely on terrestrial radiation protection standards. The radiation field is in fact quite different; it consists essentially of protons, alpha-particles, and heavier ions up to iron [2]. These particles interact with spacecraft material, giving rise to secondary radiation, e.g., neutrons.…”
Section: Introductionmentioning
confidence: 98%
“…For the US Shuttle, e.g. average crew dose rates range from 36 mGy/day to 1.1 mGy/day [2]. SEP events are currently not predictable neither in time of their occurrence nor in the maximum flux expected.…”
Section: Sources Of Protons and Ions In Outer Space And On Earthmentioning
confidence: 98%