PPT-Titan Airglow: FUV & EUV 2009 UVIS Spectra of Airglow

JOSEPH AJELLO JPL MICHAEL STEVENS NRL ROBERT WEST JPL JACQUES GUSTIN LPAP GREG HOLSCLAW CU TODD BRADLEY UCF agu dEC 2011 TITAN PROTON PLASMA 01 keV4 MeV amp SOLAR XUV GENERATES . Life in the Outer Solar System. How does life begin?. The general idea for chemical evolution is:. Organic matter + Liquid water + Energy = Life…Maybe. When looking for life…. Follow the Water. This is Europa. Approach. :. Collaborators. :. Accomplishments. :. Development of high reflectivity coatings to increase system throughput, particularly in the far-UV . (FUV) spectral . range. Study other dielectric fluoride coatings and other deposition technologies such as Ion Beam Sputtering (IBS) that is expected to produce the nearest to ideal morphology optical thin film coatings and thus low scatter.. Triton and Pluto. Vladimir Krasnopolsky. Initial data: N. 2. and CH. 4. densities near the surface. Products: vertical profiles of 83 neutral species and 33 ions from 0 to 1600 km. Main Features. The only after-Cassini model of coupled neutral and ion chemistry. Alessandra Aloisi . for the COS/STIS . team. (with input from . D.Massa. , . S.Penton. , . C.Proffitt. , . C.Oliveira. , . R.Osten. , . S.Osterman. , . D.Sahnow. ). 17 November 2011. SPACE. TELESCOPE. Life in the Outer Solar System. How does life begin?. The general idea for chemical evolution is:. Organic matter + Liquid water + Energy = Life…Maybe. When looking for life…. Follow the Water. This is Europa. -Contributed to . Kurth. et al., Saturn chapter on “auroral processes”. -Mitchell et al. 2009 paper compared UVIS auroras to INCA ring current data. -. Gustin. et al., 2009 FUSE/UVIS auroral spectroscopy . JOSEPH AJELLO. JPL. MICHAEL STEVENS. NRL. JACQUES GUSTIN. LPAP. GREG HOLSCLAW. CU. TODD BRADLEY. UCF. team meeting: . january. 2010. T. b. LIMB MODEL, RECENT LAB ANALYSIS & UVIS OBSERVATIONS . SUBMITTED FUV LIMB PAPER (T. detecting . flares, dimmings, and EUV waves . in near real-time on SDO/AIA images. Emil Kraaikamp. . (p), Cis Verbeeck – Royal Observatory of Belgium. 12. th. European Space Weather Week, Oostende, Belgium . Tritium. Studies in TITAN for. Lead Lithium Eutectic Blankets. P. . Calderoni. - . Idaho National Laboratory. S. . Fukada. - . Kyushu University. Y. . Hatano. - . Toyama University. S. . Konishi. 1/5/12. 1. UVIS Team Meeting. Problem description. No match between the FUV data and the minimum ray high from geometer.. several seconds discrepancy.. Good match of the HSP data with geometer.. We were expecting 379 integrations and only 371 could be found in DAPS.. Name that Character. The Basics. The Titans. Who Said It?. The Walls. 200. 200. 200. 200. 200. 400. 400. 400. 400. 400. 600. 600. 600. 600. 600. 800. 800. 800. 800. 800. 1000. 1000. 1000. 1000. 1000. By Grant Morgan. The “Benchmark”. 20 Years in developing a Successor. Spectra was Highly rated & very successful. . We’ve developed a close “RELATIONSHIP” . Converting to Spectra Optia is daunting. Yang Xia (Carl). Titan was discovered in 1655 by Christiaan Huygens, a Dutchman. Titan Overview. 2nd largest satellite in solar system (2575 km in radius). Orbits Saturn at about 21 Saturn radii. Rotation is tidally locked to Saturn: period--16 earth days. Jeffrey . Linsky. JILA and APAS. Solar Focus Group. April 12, 2019. Why are the Lyman-α and EUV fluxes important?. Lyman-α is the brightest line in the solar UV spectrum.. Lyman-α is as bright as the entire UV spectra of M dwarf stars..