Modeling thermal energy transfer in planetary regoliths involves treating four processes: visible radiative transfer, thermal radiative transfer, conductive transfer, and heat storage. We explicitly treat these processes while considering time-dependent problems, and we apply this model to the regol
β¦ LIBER β¦
Application of laboratory data to the sputtering of a planetary regolith
β Scribed by R.E. Johnson
- Publisher
- Elsevier Science
- Year
- 1989
- Tongue
- English
- Weight
- 389 KB
- Volume
- 78
- Category
- Article
- ISSN
- 0019-1035
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