Infrared absorption features for tetrahedral ammonia ice crystals

An effort has been made to ascertain how particle shape and composition affect the strength and shape of resonant absorption features at 9.4 and 26 microns. A shifting of the peak of the resonance relative to that for spherical particles is noted in the computational results obtained for the extinction cross-sections of 0.5- and 1-micron, volume-equivalent radius tetrahedral NH3 ice crystals that either possessed or lacked foreign cores. It it judged unlikely that small, (less than 5-micron) NH3 particles could be the principal component of the haze in the 300-500 mbar region of Jupiter.