PPT-Titan: FUV & EUV 2007-2009 Spectra Limb,

Dayglow Nightglow amp Eclipse JOSEPH AJELLO JPL MICHAEL STEVENS NRL ROBERT WEST JPL JACQUES GUSTIN LPAP GREG HOLSCLAW CU TODD BRADLEY UCF team meeting January 2011 Titan dayglow. 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. Rob Aitken. ARM . R&D. San Jose, CA. (with help from Greg Yeric, Brian Cline, Saurabh Sinha, Lucian Shifren, Imran Iqbal, Vikas Chandra and. Dave Pietromonaco). What’s Ahead?. EUV around the corner?. 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. 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 . 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. Basic Information. Discovered in 1655. Christiaan. Huygens. Moon of Saturn. Atmosphere. Mainly nitrogen and methane. The only moon to hold onto a substantial atmosphere. The orange color comes from the Sun’s ultra violet rays breaking up methane molecules. 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. Michael Campbell, Colton Colwell, Jamie Easton, Anna Scarbrough. Cassini-Huygens Mission. Previous Mission. Cassini. Flyby. Huygens: Landed on Titan. Descended through atmosphere and landed on surface.. . Fumihiro Koike, Kitasato University. Collaborators:. Izumi Murakami, NIFS (National Institute for Fusion Science). Daiji. Kato, NIFS (National Institute for Fusion Science). Hiroyuki A. . Sakaue. 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. 2. -BROADENING PARAMETERS IN THE . n. 9. BAND OF ETHANE (C. 2. H. 6. ). CURTIS P. RINSLAND. (NASA Langley Research Center, Hampton, VA, USA.). V. MALATHY DEVI & D. CHRIS BENNER. (The College of William and Mary, Williamsburg, VA, USA.).