| Abstrakt: |
In this work, a model for calculating the galactic cosmic rays (GCRs) radiation dose rate is developed. The model is based on a GCR modulation model, which is established by Shen and Qin, and the fluence‐dose conversion coefficients (FDCCs) published by the International Commission on Radiological Protection (ICRP). With the model, the radiation absorbed dose rate of GCRs near the lunar surface over long time periods is calculated and compared with the observation data from the Cosmic Ray Telescope for the Effects of Radiation and the Lunar Lander Neutron and Dosimetry. First, the energy spectrum of GCRs at 1 AU in the ecliptic, where the lunar orbit is located, is computed using the GCR modulation model. Then, using the FDCCs of ICRP 123, the absorbed dose rates of 15 human organs/tissues at the lunar orbit position are calculated to represent the general absorbed dose rate of the body (in water). Furthermore, considering the albedo radiation (excluding neutrons) and using the water‐silicon conversion coefficients, the total absorbed dose rates of GCRs near the lunar surface (in silicon) are calculated, it is shown that our modeling results generally agree with the observations from spacecraft. This work is useful for future manned space exploration to the Moon or other celestial bodies in the solar system. Plain Language Summary: The radiation absorbed dose rate is a fundamental quantity for evaluating the space radiation environment. In our study, we develop a time‐varying and spatial‐varying model to calculate the radiation dose rates of the galactic cosmic rays (GCRs). With the model, we calculate the radiation absorbed dose rate of GCRs near the lunar surface (excluding neutrons) over long time periods and compare it with the observation data from the Cosmic Ray Telescope for the Effects of Radiation and the Lunar Lander Neutron and Dosimetry. The results show that our modeling results generally agree with the observations from spacecraft. This research is important for evaluating the space radiation environment for future human space exploration to the Moon or other planets similar to the Moon in our solar system. Key Points: We develop a time‐varying and spatial‐varying model to calculate the radiation dose rates of cosmic raysReproduce the absorbed dose rate of galactic cosmic rays near the lunar surface (2010–2022) and compare with the observation of Cosmic Ray Telescope for the Effects of Radiation and Lunar Lander Neutron and Dosimetry [ABSTRACT FROM AUTHOR] |
