Stratospheric Aerosol and Gas Experiment III on the International Space Station (SAGE III/ISS) Newly Released V5.2 Validation of Ozone and Water Vapor Data

<p>The Stratospheric Aerosol and Gas Experiment III (SAGE III) instrument installed on the International Space Station (ISS) has completed over three and a half years of data collection and production of science data products. The SAGE III/ISS is a solar and lunar occultation instrument that scans the light from the Sun and Moon through the limb of the Earth’s atmosphere to produce vertical profiles of aerosol, ozone, water vapor, and other trace gases. It continues the legacy of previous SAGE instruments dating back to the 1970s to provide data continuity of stratospheric constituents critical for assessing trends in the ozone layer. This presentation shows the validation results of comparing SAGE III/ISS ozone and water vapor vertical profiles from the newly released v5.2 science product with those of in situ and satellite data .</p>

Further milliarcsecond resolution results on cool giants and binary stars from lunar occultations at Devashtal

ABSTRACT We report on 26 lunar occultation events observed in the context of a programme started at Devasthal in 2017. In addition to the customary observations with the 1.3-m telescope, we report here also the first attempts performed with the TIRCAM2 camera at the 3.6-m Devasthal Optical Telescope in the near-infrared (near-IR). The results consist in the first-time angular diameters for two late-type giants, in a measurement of the well-known asymptotic giant branch pulsating variable SW Vir, and in the measurement of eight small separation binaries one of which is detected for the first time (HR 1860). We also measured the wider binaries SAO 94431 and 55 Tau (twice). The remaining sources were found to be unresolved with upper limits as small as 1 mas. We plan to develop further the high-speed capability of the TIRCAM2 instrument, so as to include in our programme also more near-IR, highly extincted sources.