Astrochemistry Laboratory, NASA GSFC, Code 691, Greenbelt, Maryland 20775, USA.
J Chem Phys. 2010 Feb 7;132(5):054508. doi: 10.1063/1.3308484.
We studied the effects of 100 keV proton irradiation on films of ammonia-water mixtures between 20 and 120 K. Irradiation destroys ammonia, leading to the formation and trapping of H(2), N(2), NO, and N(2)O, the formation of cavities containing radiolytic gases, and ejection of molecules by sputtering. Using infrared spectroscopy, we show that at all temperatures the destruction of ammonia is substantial, but at higher temperatures (120 K), it is nearly complete (approximately 97% destroyed) after a fluence of 10(16) ions/cm(2). Using mass spectroscopy and microbalance gravimetry, we measure the sputtering yield of our sample and the main components of the sputtered flux. We find that the sputtering yield depends on fluence. At low temperatures, the yield is very low initially and increases quadratically with fluence, while at 120 K the yield is constant and higher initially. The increase in the sputtering yield with fluence is explained by the formation and trapping of the ammonia decay products, N(2) and H(2), which are seen to be ejected from the ice at all temperatures.
我们研究了 100keV 质子辐照对 20 至 120K 氨-水混合物薄膜的影响。辐照会破坏氨,导致 H(2)、N(2)、NO 和 N(2)O 的形成和捕获、含有放射分解气体的空穴的形成以及分子的溅射喷射。我们利用红外光谱表明,在所有温度下,氨的破坏都很严重,但在较高温度(120K)下,在 10(16)离子/cm(2)的辐照剂量后,几乎完全(约 97%被破坏)。我们利用质谱和微量天平重力法测量了我们样品的溅射产额和溅射流的主要成分。我们发现,溅射产额随辐照剂量而变化。在低温下,初始时产额非常低,随辐照剂量呈二次方增加,而在 120K 时产额初始时保持不变且较高。随着辐照剂量的增加,溅射产额的增加可以用氨衰变产物 N(2)和 H(2)的形成和捕获来解释,这些产物在所有温度下都被观察到从冰中逸出。