1 / 15

Detector dependency of MODIS Polarization Sensitivity derived from on-orbit characterization

Detector dependency of MODIS Polarization Sensitivity derived from on-orbit characterization. Gerhard Meister a,b , Bryan A. Franz b,c , Ewa J. Kwiatkoska d , Robert E. Eplee e,b , Charles R. McClain b,c a: Futuretech Corp. b: OBPG (Ocean Biology Processing Group)

velvet
Download Presentation

Detector dependency of MODIS Polarization Sensitivity derived from on-orbit characterization

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Detector dependency of MODIS Polarization Sensitivity derived from on-orbit characterization Gerhard Meistera,b, Bryan A. Franzb,c, Ewa J. Kwiatkoskad, Robert E. Epleee,b, Charles R. McClainb,c a: Futuretech Corp. b: OBPG (Ocean Biology Processing Group) c: NASA Goddard Space Flight Center, Code 614.2 d: TEC-EEP, ESTEC, ESA e: SAIC 8/03/09 Earth Observing Systems XIV, SPIE Optics and Photonics 2009, San Diego

  2. Optimization process Lm: MODIS measured TOA radiance (without polarization corr.) LTOA: modeled (nLw from SeaWiFS, aerosols from MODIS NIR bands) Q, U: Stokes vector parameters (modeled from Rayleigh) Lm = M11LTOA + M12Q + M13U • find best M11, M12, M13 per band, detector, and mirror-side • M11, M12, M13 = f (scan angle), cubic (M11) and linear (M12) • do this for one day per month over the mission lifespan • optimize over global distribution of path geometries

  3. M12: MODIS Terrablue band temporal trends Mirror side 1 Mirror side 2 M12 acts on the Q component 412 Detector 4 443 Space View (lunar) frame Nadir frame Solar Diffuser frame 488

  4. Blue band RVS & polarization sensitivity MS1, Detector 4 M13 fixed to pre-launch 412 443 488

  5. More microwave sensitivities: to rain

  6. Aerosol sensitivity to surface albedo A “critical surface albedo” exists for which sensitivity to aerosol completely disappears! ϖ0 Seidel & Popp, AMT, 2012

  7. Aerosol sensitivity to surface albedo A “critical surface albedo” exists for which sensitivity to aerosol completely disappears! AOD retrieval error at 550 nm. Plus (minus) signs denote an overestimate of surface albedo by 0.01 (-0.01). Seidel & Popp, AMT, 2012

  8. Sensitivity studies: useful for lots of things • Impact of instrument errors on retrievals • Best channels to retrieve certain variables • Qualitative picture of retrieval errors vs. different quantities (e.g. aerosol vs. surface albedo) • Impact of uncertainties in other variables on retrievals: e.g. cloud temperatures on cloud water path from Vis/NIR.

  9. 2D Gaussian

More Related