
Photoevaporation is the process where energetic radiation ionises gas and causes it to disperse away from the ionising source. The term is typically used in an astrophysical context where ultraviolet radiation from hot stars acts on clouds of material such as molecular clouds, protoplanetary disks, or planetary atmospheres.
光致蒸發表示的是高能輻射電離氣體,並將其趨散電離源的過程。常在天文物理中,用來形容炙熱恆星的紫外線、電磁輻射對於不同雲氣(像是分子雲、原行星盤或行星大氣層等)的作用。
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Discovered by embedding cosine similarity (sentence-transformers MiniLM, 384-dim).