PPT-UVIS calibration update

Greg Holsclaw Bill McClintock June 18 2012 Braunschweig Germany Extended source vs point source An extended source appears to exhibit flat field effects The total signal from a point source as a function of position on the detector does not. GSICS Executive Panel Meeting 12. Fuzhong Weng and Fangfang Yu. GSICS Coordination Center . Outline. Staff change in GCC team. GCC . Progress Since . April 2011. Support to the establishment of GSICS correction algorithm: diurnal calibration Evaluation. Kozhurina-Platais. Ω. Cen observed with the . WFC3/UVIS and IR . F606W & F160W filters. Wide . Range PA_V3 . and Large . POSTARG ±40. ”. Observations. L_Flat. and Distortion Cal Programs:. Outline. 1.) Step 1 – TV3 Calibration. 2.) Step 2 – SMOV4 (+ Cycle 17 Calibration). 3.) Step 3 – Final Calibration (present analysis). - More data. - New flat fields. - Astrodrizzle. - Precise calibration. -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 . Greg Holsclaw. Jan 8, 2014. 1. Outline. Calibrations since the last . meeting. Future calibrations. Calibration update. Status . of new calibration . routine. Website updates. A restructured calibration routine. 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. Auroral. Movies. As of June 2008. Wayne Pryor, Central Arizona College/Space Environment Technologies. 8. . UVIS Polar Movies in Hand!. -2007 day 96. (April 6) – only 1 with disturbed solar wind conditions. 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.. 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 . JOSEPH AJELLO. JPL. MICHAEL STEVENS. NRL. ROBERT WEST. JPL. JACQUES GUSTIN. LPAP. GREG HOLSCLAW. CU. TODD BRADLEY. UCF. Team meeting: Jan20112. TITAN PROTON PLASMA (0.1 keV-4 . MeV. ) & SOLAR XUV GENERATES . Landsat Cal/Val Team. Landsat Calibration Meeting, May 2018. Topics. TIRS. Noise. Stability. Vicarious calibration comparison. OLI. Noise. Stability. Relative Calibration. Comparison to Sentinel 2 MSIs. GOES-R Program Calibration and Validation Robert A. Iacovazzi, Jr .* (1) , Edward C. Grigsby (1), Steve Goodman (2), Changyong Cao (3), Jaime Daniels (3), and Kathleen McIntyre (1) NASA (1), MODIS/VIIRS Calibration Workshop 26 February 2021VIIRS Observations of the MoonSNPP and NOAA20 execute roll maneuvers each month to capture the Moon in the Earthview sector at phase angle 51before Ful Add 12 event classes for SVX detector. .  . Done. Generate calibration parameters for Q-vector and flattening run by run .  . on-going. Status of centrality calibration. The calibrations for run-343031-347349 are good to use..