Ice sublimation below artificial crusts: Results from comet simulation experiments
Dust mantles or non-volatile mineral crusts most probably exist on large parts of the surface of many cometary nuclei. Even when such a layer is only a few millimetres thick and porous, its existence reduces substantially the gas emission rate of the underlying ice. In the present paper we report th...
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Veröffentlicht in: | Planetary and space science 1991-03, Vol.39 (3), p.515-524 |
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