Melkonian G, Bourrieau J
Dassault Aviation, Saint-Cloud, France.
Acta Astronaut. 1994 Nov;32(11):721-30. doi: 10.1016/0094-5765(94)90166-x.
This paper presents the doses levels expected in orbits in chart form, covering the range 300-800 km of altitude and 0-90 degrees of inclination behind shieldings similar to the Hermes spacecraft and the EVA spacesuit matter distributions. These charts allow users to rapidly find the radiobiological dose received in the most critical organs of the human body either in normal situations or during a large solar event. Outside the magnetosphere, during interplanetary or lunar missions, when the dose received during crossing of the radiation belts become negligible, the dose is due to galactic cosmic rays (GCR) and solar flares. The correct radiobiological assessment of the components of this radiation field becomes a major problem. On the Moon a permanent ground-based station can be shielded by lunar materials against meteoroids and radiations. The radiobiological hazard, essentially linked to the solar flare risk during the transfer phase and the extra-station activities, may be solved by mission planning. For interplanetary flights the problem comes from both increased risk of solar events and from the continuous exposure to GCR. These energetic particles cannot be easily stopped by shieldings; cost considerations imply that more effective materials must be used. Impact on the vehicle design and the mission planning is important.
本文以图表形式展示了在轨道上预期的剂量水平,涵盖了300 - 800千米的高度范围以及与赫尔墨斯飞船和舱外活动航天服物质分布类似的屏蔽物后0 - 90度的倾角范围。这些图表能让用户快速找到在正常情况或大型太阳事件期间人体最关键器官所接受的放射生物学剂量。在磁层之外,进行行星际或月球任务时,当穿越辐射带期间所接受的剂量可忽略不计时,剂量源于银河宇宙射线(GCR)和太阳耀斑。对该辐射场各成分进行正确的放射生物学评估成为一个主要问题。在月球上,一个永久性的地面站可以被月球物质屏蔽,免受流星体和辐射的影响。放射生物学危害主要与转移阶段和站外活动期间的太阳耀斑风险相关,可通过任务规划来解决。对于行星际飞行,问题既来自太阳事件风险的增加,也来自对银河宇宙射线的持续暴露。这些高能粒子不容易被屏蔽物阻挡;出于成本考虑,意味着必须使用更有效的材料。对飞行器设计和任务规划的影响很重要。