PPT-Titan: FUV Limb Spectra From 2004 and EUV Laboratory Cross

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 amp UVIS OBSERVATIONS SUBMITTED FUV LIMB PAPER T. 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. Natalia Alvarez • . Kelsey . Bertamus. •. . Michael Morgan • Talia Strait • . Natalie Taylor. Bulk Characteristics of Titan. Diameter: . 5,150 . km. Average Density: 1.88 . g/cm. 3. . Surface Temperature: 97K. 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.. Must have for all the TITAN Clans. Rules for TITAN EMPIRE. Respect the Leader and Co-Leaders. (Racer250>=3, . RaptorTheTitan. ). Do not use inappropriate language on the chat.. Donate before Receiving.. Abstract. We observed a filament eruption, whose shape is like a dandelion, associated with the solar flare that occurred on 2011 February 16 at the active region NOAA 11158. The H. a. . full disk images of the flare were taken by FMT. 2-D Magnetosphere. -Ionosphere-Thermosphere coupling model. Chihiro Tao. 1,2. , . Michel . Blanc. 1. 1. IRAP, Univ. de Toulouse/UPS-OMP/CNRS. 2. now at NICT (chihiro.tao@nict.go.jp). Journée scientifique . and beyond. ASTR 1420. Lecture . 14. Sections 9.3. Saturn’s Moons. 62 Moons, 53 named (18 above). Mostly icy, some with rocky cores. . Titan is the 2. nd. largest moon in our Solar System & only one with a “real” atmosphere with N. Tritium. Studies in TITAN for. Lead Lithium Eutectic Blankets. P. . Calderoni. - . Idaho National Laboratory. S. . Fukada. - . Kyushu University. Y. . Hatano. - . Toyama University. S. . Konishi. JOSEPH AJELLO. JPL. MICHAEL STEVENS. NRL. ROBERT WEST. JPL. JACQUES GUSTIN. LPAP. GREG HOLSCLAW. CU. TODD BRADLEY. UCF. agu. : . dEC. 2011. TITAN PROTON PLASMA (0.1 keV-4 . MeV. ) & SOLAR XUV GENERATES . Enceladus. Enceladus. is a moon of Saturn, 1000 times . smalller. than . Europa. , with jets emanating from hot crevasses. The jets are icy particles frozen from salty water.. Titan. 2nd largest moon in the sol sys. Sam Schonfeld. Advisors: Paola . Testa. and Steve Saar . Contents. Motivation. Cross calibrating solar measurements. Methods: Finding Targets. Tracking targets. Modeling stellar emission. Estimating Signal . 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. . Fumihiro Koike, Kitasato University. Collaborators:. Izumi Murakami, NIFS (National Institute for Fusion Science). Daiji. Kato, NIFS (National Institute for Fusion Science). Hiroyuki A. . Sakaue. 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..