Master index of OBPG MODIS Terra L1b LUTs
created by Gerhard Meister for the Ocean Biology Processing Group
(click
here for Aqua)
(click
here for m1 and RVS trending plots, comparing V6.1.6.3_OC2a and V6.1.6.3_OC3a)
Collection 6 (final format):
- V6.1.12.3b: 9/24/12, C6 LUT in new format. Identical to LUT used for R2010.0 up to 2010, identical to operational since April 2012, and very similar to operational in between. Used for testing only.
- V6.1.14.2a: 9/21/12, C6 LUT in new format. Contains V6.1.12.0a values until April 2012; V6.1.12.3a from then until September 2012; then values from V5.0.46.46. Submitted to swdev1 for operational processing
- V6.1.14.2: 9/21/12, MCST update to V6.1.14.1 (update to end of mission only)
- V6.1.14.1: August 2012, MCST LUT in new format. Designated as final for C6 by MCST. Used for TT24.
- V6.1.12.4: 05/15/12, MCST LUT in new format, not officially designated as final for C6 by MCST, but expectation is that there will be no change; used for TT23 (no reprocessing so far)
- V6.1.12.3a: April 2012, contains values from MCST LUT V5.0.46.38 in new C6 format (no merging with V6 LUTs was done, only format was changed; therefore, historic values are different); used for operational processing
- V6.1.12.0a.hdf: 12/27/11, contains values from operational LUT (V6.1.6.3_OC3a) in new C6 format (this LUT is identical to MOD02_Reflective_LUTs.V6.1.6.3_OC3a.hdf.finalC6; original MCST file: V6.1.12)
Collection 6 (preliminary format):
- V6.1.6.3_OC3a: 09/21/11, same method as below, submitted to swdev1 for production
- V6.1.6.3_OC2a: 06/13/11, merged V6.1.6.2 and V6.1.6.3_OC2 (replacing data in V6.1.6.3_OC2 (MCST calibration method for V6.1.6.3_OC2 is identical to that used in V6.1.6.2, but e.g. band 9 shows a larger than 1 percent transition)) up to end of 2010 with V6.1.6.2), submitted to swdev1 for production
- V6.1.6.3_OCa: 04/19/11, merged V6.1.6.2 and V6.1.6.3_OC (replacing data in V6.1.6.3_OC (MCST calibration method for V6.1.6.3_OC is identical to that used in V6.1.6.2, but e.g. band 9 shows a larger than 1 percent transition)) up to end of 2010 with V6.1.6.2), submitted to swdev1 for production
- V6.1.6.3a: 03/25/11, merged V6.1.6.2 and V6.1.6.3 (replacing data in V6.1.6.3 (even though MCST calibration methodology for V6.1.6.3 not identical to that used in V6.1.6.2) up to end of 2010 with V6.1.6.2), submitted to swdev1 for production
- V6.1.6.3: 12/08/10, MCST LUT for Collection 6 (different historical data relative to V6.1.6.2, not used)
- V6.1.6.2a: 07/20/10, applied detector correction to V6.1.6.2, problems with new detector dependent RVS, not used for production
- V6.1.6.2: 08/12/10, final MCST LUT for collection 6, submitted to swdev1 var/EVAL directory (e.g. for TXC07 update); LUT used for R2010.0
- V6.1.6.1: 04/15/10, MCST LUT for collection 6, submitted to swdev1, used e.g. for TT17
Collection 5:
- V5.0.46.6a: 09/13/10
applied TOA detector destriping correction to V5.0.46.6 (both ocean and land bands), submitted to swdev1 var/OPER directory (i.e. automatically applied for production the following day)
- V5.0.46.5a: 08/12/10
applied TOA detector destriping correction to V5.0.46.5 (both ocean and land bands), submitted to swdev1 var/OPER directory (i.e. automatically applied for production the following day)
- V5.0.46.2a: 06/11/10
applied TOA detector destriping correction to V5.0.46.2 (both ocean and land bands), submitted to swdev, installed into production on 6/11/10
- V5.0.44.13a: May 2010
applied TOA detector destriping correction to V5.0.44.12 (both ocean and land bands), submitted to swdev, installed into production on 5/19/10
- V5.0.44.12a: 04/05/10
applied TOA detector destriping correction to V5.0.44.12 (both ocean and land bands), submitted to swdev, installed into production on ??
- V5.0.44.10a: 02/22/10
applied TOA detector destriping correction to V5.0.44.10 (both ocean and land bands), submitted to swdev, installed into production on 02/23/10
- V5.0.40.25e: 07/22/09
applied TOA detector destriping correction to V5.0.40.25a, submitted to swdev, installed into production on 07/28/09
- V5.0.40.25a: 06/25/09
merged MCST operational LUT V5.0.40.25 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on 07/21/09
- V5.0.40.14a: 12/16/08
merged MCST operational LUT V5.0.40.14 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on 12/16/08
- V5.0.40.13a: 11/26/08
merged MCST operational LUT V5.0.40.13 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on 11/26/08
- V5.0.40.6a-12a: same procedure as 5a
- V5.0.40.5a: 5/09/08
merged MCST operational LUT V5.0.40.5 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on ??/??/08
- V5.0.40.4a: 4/08/08
merged MCST operational LUT V5.0.40.4 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on 4/17/08
- V5.0.40.3a: 3/13/08
merged MCST operational LUT V5.0.40.3 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on 3/14/08
- V5.0.38.1c: 3/06/08
same as V5.0.38.1b, except NIR detector residual corrections from Ewa were included, used by Ewa for crosscalibration to SeaWiFS
- V5.0.40.2a: 2/29/08
merged MCST operational LUT V5.0.40.2 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on ??/08
- V5.0.38.1b: 2/26/08
same as V5.0.38.1_OC2, except NIR RVS temporal trend is derived by wavelength interpolation from non-saturated bands, never used in production
- V5.0.38.1_OC2: 2/19/08
updated MCST 'best available' LUT with 2nd half of 2007 updated for new solar diffuser degradation, NIR RVS temporal trend from non-saturated lunar pixels, never used in production
- V5.0.40.1a: 2/7/08
merged MCST operational LUT V5.0.40.1 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on 2/11/08
- V5.0.38.3a: 12/14/07
merged MCST operational LUT V5.0.38.3 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on 12/17/07
- V5.0.38.2a: 11/08/07
merged MCST operational LUT V5.0.38.2 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on 11/09/07
- V5.0.38.1a: 10/25/07
merged MCST operational LUT V5.0.38.1 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on ???
- V5.0.6.33a: 08/17/07
merged MCST operational LUT V5.0.6.33 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on ???
- V5.0.6.32a: 07/20/07
merged MCST operational LUT V5.0.6.32 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on ???
- V5.0.6.31a: 06/21/07
merged MCST operational LUT V5.0.6.31 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on 6/21/07
- V5.0.7.27a: 5/22/07
same as 27_OC2, dependency of RVS for NIR bands from bands 1,2,17 linearly interpolated
- V5.0.6.30a (05/14/07, merged MCST operational LUT V5.0.6.30 with MCST 'best available' V5.0.6.27_OC2, submitted to swdev, installed into production on 5/15/07)
- V5.0.6.27_OC2: 3/22/07
original MCST LUT, same as 20_OC, extended to beginning of mission
- V5.0.6.20f (03/20/07, same as 20d, corrected by Ewa's TOA derived detector residuals)
- V5.0.6.20e (01/31/07, time dependency of RVS for NIR bands from bands 1,2,17 linearly interpolated)
- V5.0.6.20d (01/17/07, time dependency of RVS for NIR bands from bands 1,2)
- V5.0.6.20b (11/06/06, time dependency of RVS for NIR bands from bands 1,2,17)
- V5.0.6.20_OC (9/13/06, original MCST LUT, new method for fitting SD degradation (exponential quadratic))
- V5.0.6.15b (8/4/06, RVS for NIR bands from bands 1,2,17)
- V5.0.6.15a (8/2/06, RVS for NIR bands from bands 1,2,17; modified extrapolation for frames >1000)
- V5.0.6.15_OC (05/10/06, delivered by MCST, valid for days 2004366 to 2006124)
- V4.3.0.9_OC (06/14/04)
- V4.1.2.6M (August 2003)
For further information, please contact:
Gerhard Meister
Ocean Biology Processing Group, NASA/GSFC Code 614.2
Building 28, Room W119, Greenbelt, MD 20771 USA
Tel #: (301) 286 - 0758, FAX #: (301) 286 - 0268
email: meister@simbios.gsfc.nasa.gov