UVIS Occultation Geometry Summary

Slides:

Advertisements

Similar presentations

Francesco Trotta YERAC, Manchester Using mm observations to constrain variations of dust properties in circumstellar disks Advised by: Leonardo.

Advertisements

Revised tholin profile for the atmosphere of Titan Mao-Chang Liang 1, J. A. Kammer, X. Zhang 3, D. Shemansky 4, Y. L. Yung 2 1 Research Center for Environmental.

CIRS Ring Observations: Submm, Temp and Stellar Occultations Linda Spilker, Scott Edgington, Rich Achterberg, Stuart Pilorz, Shawn Brooks April 26, 2004.

Wavelike Structure in Saturn’s Rings

Toshimichi Otsubo Mihoko Kobayashi Hitotsubashi University 1 Optical Response Simulation for ASTRO-G Laser Reflector Array Hiroo Kunimori National Institute.

Halfway Around the World for 5 Minutes of data

Dust Envelopes around Oxygen-rich AGB stars Kyung-Won Suh Dept. of Astronomy & Space Science Chungbuk National University, Korea

The planetary nebula M2-9: Balmer line profiles of the nuclear region Silvia Torres-Peimbert 1 Anabel Arrieta 2 Leonid Georgiev 1 1 Instituto de Astronomía,

Essam Marouf & Richard French Cassini CHARM Presentation

1 The Organic Aerosols of Titan’s Atmosphere Christophe Sotin, Patricia M. Beauchamp and Wayne Zimmerman Jet Propulsion Laboratory, California Institute.

Global seismic tomography and its CIDER applications Adam M. Dziewonski KITP, July 14, 2008.

CP violation in B decays: prospects for LHCb Werner Ruckstuhl, NIKHEF, 3 July 1998.

Neutron Detection in JLab’s Hall B Michael Braverman Tel-Aviv University Data Mining Meeting, MIT, August 9th 2014 In Collaboration With : E. Piasetzky.

Nitrogen Chemistry in Titan’s Upper Atmosphere J. A. Kammer †, D. E. Shemansky ‡, X. Zhang †, and Y. L. Yung † † California Institute of Technology, Pasadena,

Rutherford Appleton Laboratory Requirements Consolidation of the Near-Infrared Channel of the GMES-Sentinel-5 UVNS Instrument: Initial trade-off: Height-resolved.

Rev 131 Enceladus’ Plume Solar Occultation LW Esposito and UVIS Team 14 June 2010.

Lingling Ma IHEP China Measurement of Cosmic rays with LHAASO at 10PeV~100PeV 4th Workshop on Air Shower Detection at High Altitude Institute of High Energy.

Micro-structural size properties of Saturn’s rings determined from ultraviolet measurements made by the Cassini Ultraviolet Imaging Spectrograph Todd Bradley.

The Composition and Structure of Enceladus’ Plume from the Cassini UVIS Solar Occultation C. J. Hansen, L. Esposito, D. Shemansky, A. I. F. Stewart, A.

Enceladus Plume Update C. J. Hansen, I. Stewart, L. Esposito, A. Hendrix June 2009.

Methane Distribution in Titan’s Atmosphere Spica + Shaula Occultations. Candidate Observations Symmetrical Methane Distribution Flatfield Issues Asymmetrical.

Rev 51 Enceladus Zeta Orionis Occultation Analysis Status 9 January 2008.

Observations of Enceladus ’ Plume from Cassini ’ s UltraViolet Imaging Spectrograph (UVIS) C. Hansen, L. Esposito, J. Colwell, A. Hendrix, B. Meinke, I.

Cassini UVIS Results on the Enceladus Plume and Spacecraft Safety Larry W. Esposito 5 June 2007 Athens PSG.

UVIS calibration update Greg Holsclaw Bill McClintock Jan 8,

Cassini Observations and the History of Saturn’s Rings Larry W. Esposito 12 October 2006.

Cassini UVIS Observations and the History of Saturn’s Rings Larry W. Esposito, Joshua E. Colwell, Glen R. Stewart LASP, University of Colorado 24 August.

Ring Spectroscopy and Photometry Todd Bradley January 9, 2014.

U.A. Dyudina, A.P. Ingersoll, California Institute of Technology Pasadena, CA, Objectives We study lightning on Jupiter using spatially resolved.

Unraveling the Twists and Turns of Saturn’s Rings

Enceladus Dual Star Occultation

UVIS spectrometry of Saturn’s rings

Icy Moon Occultations: the Search for Volatiles

C. J. Hansen, L. Esposito, D. Shemansky, B. Lewis, A. I. F. Stewart, J

Enceladus Report C. J. Hansen January 2013.

Analysis of Density Waves in UVIS Ring Stellar Occultations

Titan UVIS Airglow Spectra: Modeling and Laboratory Studies

UVIS Calibration Update

XM Status and Plans, XXM Activities Icy Satellite Science

XXM Status, Priorities, Plans, and Activities Icy Satellite Science

Saturn’s Auroras from the Cassini Ultraviolet Imaging Spectrograph

XXM Status, Priorities, Plans, and Activities Icy Satellite Science

RTWT and Science Planning Report

Titan tholin properties from occultation and emission observations

UVIS Performance Status

HDAC status and analysis: Photometric observations by HDAC onboard Cassini Yuri Skorov, Horst Uwe Keller, Ralf Reulke, Karl-Heinz Glassmeier, Vlad.

Photometric observations by HDAC onboard Cassini: sensitivity and first comparison with models Yuri Skorov, Horst Uwe Keller, Ralf Reulke, Karl-Heinz.

Saturn Ring Results from the Cassini Composite Infrared Spectrometer

Iapetus as measured by Cassini UVIS

XXM Status, Priorities, Plans, and Activities Icy Satellite Science

XM Status, Priorities and Plans, XXM Activities Icy Satellite Science

UVIS Calibration Update

HyCal Energy Calibration using dedicated Compton runs

Summary of Asteroidal Occultations in North America

XM Status, Priorities and Plans, XXM Activities Icy Satellite Science

UVIS Calibration Update

UVIS results and ring evolution

UVIS Calibration Update

Retinal Function: Coupling Cones Clarifies Vision

Upcoming Events Cassini Equinox Mission

UVIS Saturn EUVFUV Data Analysis

Clumps and Moonlets in Saturn’s F Ring

Bottom view of top of cage 1 - mark on other cage half explains which half we’re looking at 2 - Dents travel along a line of latitude of the ball spin,

Dione’s O2 Exosphere C. J. Hansen January 2013.

GEOMETER Update Get new version of GEOMETER from Team web site after August 8. Some new parameters now computed (illum angles for “near point” of non-intersecting.

Revised tholin profile for the atmosphere of Titan

Kristopher Larsen July 26, 2005

Observed (symbols) and predicted (solid lines, eq

Adjustment of the 3 reference tables at building 180 AT960 measurement

Presentation transcript:

UVIS Occultation Geometry Summary July 11, 2006 UVIS Team Meeting - Colwell

A Ring Azimuthal Transparency Asymmetry July 11, 2006 UVIS Team Meeting - Colwell

A Ring Azimuthal Transparency Asymmetry Opacity variations with azimuthal view angle. July 11, 2006 UVIS Team Meeting - Colwell

Self-Gravity “Wake” Model July 11, 2006 UVIS Team Meeting - Colwell

Sig Sgr at 50 km Resolution July 11, 2006 UVIS Team Meeting - Colwell

UVIS Team Meeting - Colwell 26 Tau Rev 8 July 11, 2006 UVIS Team Meeting - Colwell

FUV Observation of 26 Tau (8) July 11, 2006 UVIS Team Meeting - Colwell

FUV Observation of Del Aqr Occultation July 11, 2006 UVIS Team Meeting - Colwell

FUV Observation of Alp Leo July 11, 2006 UVIS Team Meeting - Colwell

Inner B Ring Optical Depths July 11, 2006 UVIS Team Meeting - Colwell

Central B Ring Optical Depths July 11, 2006 UVIS Team Meeting - Colwell

Outer B Ring Optical Depths July 11, 2006 UVIS Team Meeting - Colwell

UVIS Team Meeting - Colwell Model Fit at 113,625 km July 11, 2006 UVIS Team Meeting - Colwell

UVIS Team Meeting - Colwell Thin B Ring July 11, 2006 UVIS Team Meeting - Colwell

B Ring Wake Separations July 11, 2006 UVIS Team Meeting - Colwell

Sensitivity of Model Fit July 11, 2006 UVIS Team Meeting - Colwell

Self-Gravity Wake Orientation July 11, 2006 UVIS Team Meeting - Colwell

UVIS Team Meeting - Colwell Inner vs Outer B Ring July 11, 2006 UVIS Team Meeting - Colwell

UVIS Team Meeting - Colwell Inner vs Outer B Ring (2) July 11, 2006 UVIS Team Meeting - Colwell

Predicted B Ring Normal Optical Depth July 11, 2006 UVIS Team Meeting - Colwell

Ratio of True Tau to Max Observed July 11, 2006 UVIS Team Meeting - Colwell

UVIS Team Meeting - Colwell Alp Leo Turnaround July 11, 2006 UVIS Team Meeting - Colwell

Spatial FFT of Alp Leo Turnaround Blue: Ingress Red: Egress July 11, 2006 UVIS Team Meeting - Colwell

Model Fit to Data at Alp Leo Turnaround July 11, 2006 UVIS Team Meeting - Colwell