Presentation #401.03 in the session Titan: Up High, Down Low.
Ground-based observations of Titan in the millimeter/submillimeter bands have long been an important tool for understanding the physical and chemical characteristics of its stratosphere starting with the detection of upper atmospheric CO , nitriles [2-4], and isotopologues [5-6]). The development of the first mm-wave interferometers allowed for Titan to be coarsely resolved, providing crude maps and detection of winds [7-9]. In the past decade a sea change has come from the commissioning of ALMA, providing significant improvements in sensitivity and spatial resolution, leading to many detections of new species and novel isotopologues . ALMA programs leading to highly resolved maps of many species, along with vertically resolved winds from 300 km into the thermosphere above 1000km, have now been presented [11-12].
We will present new spatially resolved observations of many nitriles in Titan’s stratosphere, obtained in 2019 as a spectral line survey using the Submillimeter Array (SMA). While significantly smaller than ALMA, the SMA provided 32 GHz of continuous bandwidth at 140 kHz resolution (roughly 34 times what ALMA can provide simultaneously at the same resolution), covering many different species and transitions. While the 2019 data have lower spatial resolution, many spectral lines were imaged by SMA and can be compared to the 2016 distributions mapped by ALMA. Most nitriles show significant changes in their distributions, following seasonal changes that have been explored by Cassini CIRS, for example [13-15]. Zonal wind estimates are also possible from the data. These measurements show that the SMA can play an important role going forward in measuring stratospheric seasonal variability. Current and future SMA upgrades will significantly improve upon the capabilities demostrated by these observations, and will allow for unique and timely measurements of Titan’s atmosphere in the coming years.
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