Buffer gas cooled ice chemistry. I. Buffer gas cell and mm-wave spectrometer

Abstract

A new instrument is described that will employ buffer gas cooling with mm-wave rotational spectroscopy (60–90 GHz) to probe molecules desorbed from astrochemical ices prepared in an ultrahigh vacuum environment. Here the design and performance of the buffer gas cell, mm-wave spectrometer and data acquisition system are reported, while application to molecules desorbed from ice surfaces will be described in a future publication. The effective temperature of the neon-cooled buffer gas cell is determined by monitoring a range of rotational lines of propyl cyanide introduced into the cell. Its number density is estimated from comparison to room temperature measurements and the effective collision cross section with neon is estimated by monitoring the free induction decay (FID) lifetimes. The spectrometer and data acquisition system described are capable of acquiring and time–domain averaging the FIDs at 10 Gs/s, 10 bit vertical resolution and 98% duty cycle.