VizieR Online Data Catalog: Venus mesosphere ALMA observations (Piccialli+, 2017)
Résumé
Observations of Venus were obtained using the ALMA interferometer within the project labeled 2011.0.00136.S. We observed - with a single receiver tuning setup - the CO, SO, SO2 and H2O rotational lines at frequencies of 345.795GHz, 346.528GHz, 346.652GHz and 335.395GHz, respectively. The spectral resolution (originally 61kHz) was binned to 0.35MHz in order to optimize the S/N. These observations were obtained on November 14, 2011, between 22:15 and 22:53 UT; on November 15, 2011, between 20:39 and 21:11 UT; on November 26, 2011, between 21:24 and 22:02 UT; and on November 27, 2011, between 21:07 and 21:58 UT. (23 data files).