Overview of the main radiation transport codes

被引：3

作者：

Schetakis, Nikolaos ^{[1
]}

Crespo, Rodrigo ^{[2
]}

Luis Vazquez-Poletti, Jose ^{[2
]}

Sastre, Mariano ^{[1
,3
]}

Vazquez, Luis ^{[2
,4
]}

Di Iorio, Alessio ^{[1
]}

机构：

[1] ALMA Sistemi Srl, I-00012 Rome, Italy

[2] Univ Complutense Madrid, Fac Informat, Madrid 28040, Spain

[3] Univ Complutense Madrid, Dept Fis Tierra & Astrofis, Madrid 28040, Spain

[4] Univ Complutense Madrid, Inst Matemat Interdisciplinar IMI, Madrid 28040, Spain

来源：

GEOSCIENTIFIC INSTRUMENTATION METHODS AND DATA SYSTEMS | 2020年 / 9卷 / 02期

基金：

欧盟地平线“2020”;

关键词：

HETC-HEDS; HZETRN; FLUKA; NEUTRONS; SPECTRA; SHIELD;

D O I：

10.5194/gi-9-407-2020

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

Accurate predictions of expected radiation dose levels on Mars are often provided by specific radiation transport codes that have been adapted to space conditions. Unsurprisingly, several of the main space agencies and institutions involved in space research and technology tend to work with their own in-house radiation codes. We present the codes that are related to the simulation of the radiation on Mars' surface under different scenarios. All of these codes have similar fields of application, but they differ with respect to several aspects, including the energy range and types of projectiles considered as well as the models of nuclear reactions considered.

引用

页码：407 / 415

页数：9

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