PPT-SEEM 94 Calibration to RBSA Data

Progress Report on Phase 2 Digging a Little Deeper Subcommittee Regional Technical Forum March 20 2013 Background Ran SEEM on 289 RBSA houses Full RBSA sample n 1404 whittled down due to. Block Diagram of Setup. Pure Nitrogen. CO2 . 1028 . ppm. 500 . sccm. 200 . sccm. 200 . sccm. Flow rate. MFC. TGS 4161 Figaro- co. 2. Range: 350 . ppm. -10000ppm. Atmospheric concentration: 350-400 . Sean R. Stratton. TA-All Meeting – June 2010. Motivation. We’re still trying to understand the relative energy scale differences between our FDs.. The UVLED was used to . cross-calibrate all three FD sites.. M. . Sugizaki. (RIKEN). on behalf of MAXI Team. 2010.11.30 MAXI 2010. 1. GSC Calibration and Analysis Status. Outline. In-orbit . Operation . and Performance. HV Operation History. Background, Sky Coverage,. Craig Donlon and Kenneth S. Casey on behalf of the SST-VC members. ESA and NOAA. CEOS SIT-29 Meeting. C. NES, Toulouse, France. 9. th. -10. th. April 2014. GPM/GMI. SST-VC Status and Issues. Relatively healthy space segment but:. 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. Major references. Calibration lecture is not in the book.. Kennedy, Marc C., and Anthony O'Hagan. "Bayesian calibration of computer models." . Journal of Royal Statistical Society: Series B . (2001).. George J. Bendo. and the SPIRE-ICC. Basic Equations. Derivative of flux calibration curves (from empirical analysis):. Flux calibration curve (integral of above equation):. V. 0. is a zero-point voltage that is selected to match the background in dark sky. . Purpose. Disclaimer. This presentation is . not. intended to supersede or substitute for the information found within the WSR-88D Electronic Handbooks. . The technician should always read new revisions and change packages, to better understand any changes to their system, or the maintenance procedures prior to the development of an issue.. USGS EROS. rmorfitt@usgs.gov. Work Performed by. SGT: Mike Choate, . Mark . Lubke, . Obaidul. . Haque. , . Ajit. . Sampath. , Jim . Storey. , . and . Esad. . Micijevic. SDSU: . Dennis . Helder. , and Ashish Shrestha . Purpose. Disclaimer. This presentation is . not. intended to supersede or substitute for the information found within the WSR-88D Electronic Handbooks. . The technician should always read new revisions and change packages, to better understand any changes to their system, or the maintenance procedures prior to the development of an issue.. 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), NRAO – Green Bank. November 2012. Receiver calibration sources allow us to convert the backend’s detected voltages to the intensity the signal had at the point in the system where the calibration signal is injected.. Goal. Address Areas for Recommendations: . #2 “Data Policy, Data Quality Protocols and Procedures” and . #. 4 “Data sampling rate strategy development and management ”. Specific topics:. “.