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Quality of MISR Radiometric Calibration
February 5, 2009

Back to calibration uncertainty overview discussion.

Calibration Process

MISR has challenging radiometric specifications of 3% absolute, and 1% band and camera-relative calibration. The radiometric calibration is facilitated by use of an on-orbit calibrator (OBC) experiment, which is utilized at bi-monthly intervals. During these experiments a diffuse panel reflects solar light into the cameras. The intensity of this light is measured with on-board photodiode "detector standards." With the measured incident radiance and output DN, radiometric calibration coefficients are computed. Following each experiment the coefficients are packaged into a file called the Ancillary Radiometric Product (ARP). This new ARP file is used for the next two months to produce the MISR Level 1B1 radiance product, and in turn the Level 1B2 geo-located product.

Because of the challenging radiometric requirements, the calibration team at JPL has been researching various procedures for reducing the calibration data and producing coefficients. Calibration-algorithm changes have occurred over time, and thus the initial ARP time-series files have not been produced using a common algorithm. The full history of this activity is reported in Table 2 below.

It is desirable to generate all reprocessed data at a uniform quality level which reflects the most current and accurate approach available to calibrating the instrument. To this end, the ARP time-series files have been regenerated twice during the mission with fixed algorithms. The first regeneration effort, conducted in January of 2004, and described in Table 3 below, was used to produce reprocessing Collection 4 data. The second and final ARP regeneration effort, described in Table 1 below, was conducted in November of 2004. The user must pay attention to the version number portion of the ARP_INFLTCAL Filename in order to determine the uncertainty of the resulting data. Users are advised to obtain data products generated with the ARP file version specified in table 1.

Table 1. Active in-flight ARP data files (Uniform Quality.
Used in reprocessing Collections 5 and greater.)
ARP ID File Version* Radiometric uncertainty
(for uniform targets)
T002-T056 F02_0010 Same as T029, described in Table 2.
* Filename conventions:
Txxx = Time window, defined in Table 2.
Fxx = Format version
xxxx = revision number of this Time window file

Table 2. Initial Releases of in-flight ARP data files (Incremental Quality Improvements Since Launch)
ARP ID Valid For Data Acquired On/After: Time Orbit Filename* Calibration algorithm updates Radiometric uncertainty
(for uniform targets)
T056 04 Feb 2009 23:47:13 48590 T056_F02_0010 Same algorithm as T055. Same as T018
T055 21 Jan 2009 23:34:51 48386 T055_F02_0010 CALFACT, the precursor to ARPGEN which calculates the calibration factors contained in the calfactor file, was modified to remove any dependencies on goniometer movement. Calibration sequences T054 and prior computed Pin3_cal and Pin4_cal based on the goniometer movement. Due to the MISR anomaly during the T054 calibration sequence on September 30, 2008, the MISR calibration sequences were modified to exclude any goniometer movement. Therefore, the algorithm which calculates the Pin3_cal and Pin4_cal calibration factors was changed to use predictions derived from historical goniometer calibration data through T054. For Pin4_cal a south_Pin2 / north_Pin2 ratio was also used to compensate for panel variations. Calibration sequences from T055 on will use this new algorithm. Same as T018
T054 16 Oct 2008 17:54:17 46970 T054_F02_0010 Same algorithm as T031. Same as T018
T053 06 Aug 2008 22:44:45 45939 T053_F02_0010 Same algorithm as T031. Same as T018
T052 11 Jun 2008 23:34:21 45124 T052_F02_0010 Same algorithm as T031. Same as T018
T051 04 May 2008 22:32:21 44570 T051_F02_0010 Same algorithm as T031. Same as T018
T050 19 Feb 2008 22:50:44 43478 T050_F02_0010 Same algorithm as T031. Same as T018
T049 16 Dec 2007 23:46:09 42532 T049_F02_0010 Same algorithm as T031. Same as T018
T048 30 Oct 2007 22:50:45 41847 T048_F02_0010 Same algorithm as T031. Same as T018
T047 29 Aug 2007 22:38:38 40944 T047_F02_0010 Same algorithm as T031. Same as T018
T046 28 Jun 2007 01:00:34 40028 T046_F02_0010 Same algorithm as T031. Same as T018
T045 01 May 2007 00:23:28 39183 T045_F02_0010 Same algorithm as T031. Same as T018
T044 28 Feb 2007 00:11:21 38280 T044_F02_0010 Same algorithm as T031. Same as T018
T043 15 Jan 2007 01:25:13 37640 T043_F02_0010 Same algorithm as T031. Same as T018
T042 15 Nov 2006 00:16:38 36751 T042_F02_0010 Same algorithm as T031. Same as T018
T041 06 Sep 2006 00:54:00 35732 T041_F02_0010 Same algorithm as T031. Same as T018
T040 21 Jul 2006 01:37:18 35048 T040_F02_0010 Same algorithm as T031. Same as T018
T039 18 May 2006 01:36:55 33819 T039_F02_0010 Same algorithm as T031. Same as T018
T038 21 Mar 2006 00:59:46 33271 T038_F02_0010 Same algorithm as T031. Same as T018
T037 20 Jan 2006 00:34:26 32397 T037_F02_0010 Same algorithm as T031. Same as T018
T036 10 Nov 2005 00:25:18 31363 T036_F02_0010 Same algorithm as T031. Same as T018
T035 26 Sep 2005 00:56:43 30707 T035_F02_0010 Same algorithm as T031. Same as T018
T034 21 Jul 2005 00:26:35 29732 T034_F02_0010 Same algorithm as T031. Same as T018
T033 01 Jun 2005 00:39:31 29004 T033_F02_0010 Same algorithm as T031. Same as T018
T032 21 Mar 2005 01:28:20 27956 T032_F02_0010 Same algorithm as T031. Same as T018
T031 31 Jan 2005 00:47:05 27242 T031_F02_0010 Subsequent to the overall band-to-band calibration adjustments made in ARP T024, camera-by-camera radiometric calibration refinements were made based on the combined analysis of multiple calibration techniques (Diner et al., 2004; Kahn et al., 2005). They amounted to 1% or less in all cases except the near-infrared channel of the Bf camera, which was reduced by 2.5%. Same as T018
T030 19 Nov 2004 00:27:53 26237 T030_F02_0001 Same algorithm as T024. Same as T018
T029 28 Sep 2004 00:22:20 25436 T029_F02_0001 Same algorithm as T024. Same as T018
T028 29 Jul 2004 00:10:15 24533 T028_F02_0001 Same algorithm as T024. Same as T018
T027 16 Jun 2004 23:46:38 23921 T027_F02_0001 Same algorithm as T024. Same as T018
T026 30 Mar 2004 00:17:39 22771 T026_F02_0001 Same algorithm as T024. Same as T018
T025 20 Jan 2004 10:48:50 21758 T025_F02_0001 Same algorithm as T024. Same as T018
T024 5 Dec 2003 01:08:28 21023 T024_F02_0002 Band-to-Band Adjustment: The red band calibration was reduced by 3% relative to the calibration in use since the year 2000. The NIR band was reduced by 1.5% (Bruegge et al., 2004). Blue and Green band relative calibrations were not changed. Additional bug fixes amounting to roughly a 1% change include: calibrating the G1 coefficients over the slowly-changing clear atmosphere portion of the cal acquisition and fixing some minor time and angle problems in the ARP generation software. Same as T018
T023 21 Oct 2003 00:19:32 20441 T023_F02_0001 Same algorithm as T022. Same as T018
T022 20 Aug 2003 01:03:31 19524 T022_F02_0001 Minor Bug Fix to T018 algorithm. Solar Angles on the diffuse panel are computed at the correct time, removing a 1.5 degree error; and the aft-camera BRF scale factors have been adjusted appropriately. The resulting change in the calibration is less than 1%. Same as T018
T021 09 Jun 2003 00:14:54 18475 T021_F02_0001 Same algorithm as T018. Same as T018
T020 22 Apr 2003 00:15:25 17776 T020_F02_0001 Same algorithm as T018. Same as T018
T019 18 Feb 2003 01:08:38 16859 T019_F02_0001 Same algorithm as T018. Same as T018
T018 12 Jan 2003 00:41:19 16320 T018_F02_0001 Same off-axis corrected algorithm as used to generate T017, but an additional bug fix regarding sun angles on the calibration panel was made to the code which calculates BRF.

Absolute: 4%

Camera and band relative: 2%

Pixel relative: 0.5%

T017 24 Oct 2002 00:42:14 15155 T017_F02_0001 Off-axis corrected algorithm. An error in the BRF database indexing has been corrected in the code used to process MISR calibration coefficients.

Absolute: 4%

Camera and band relative: 2%

Pixel relative: 0.5%

T016 6 Sep 2002 00:42:47 14456 T016_F02_0001 Linear. A linear calibration equation is again implemented. The DN versus radiance curve is constrained to go through zero. This algorithm gives more consistent calibrations among data collected over the North and South poles. Exceptions to the 4% absolute uncertainty are: AN camera western edge is 10% too bright; AN camera eastern edge is 5% too dim. Error varies between these values for other pixels, with best radiometry at the swath center.

Relative uncertainties: Same as most recent ARP.

T015 26 Jun 2002 01:33:03 13408 T015_F02_0001 No algorithm change.
T014 25 Apr 2002 01:21:24 12505 T014_F02_0001 No algorithm change.
T013 25 Feb 2002 00:05:41 11645 T013_F02_0001 No algorithm change.
T012 22 Dec 2001 01:02:27 10699 T012_F02_0001 BRF correction algorithm. Data from the on-board goniometer have been used to update the North calibration panel reflectance data base. The D-pin photodiodes are used to calibrate all but the nadir camera; the -yn-pn photodiode was used for the An camera only. We believe this to correct an aft-to-fore camera bias; camera-relative uncertainties using this algorithm are believed to be less than 2%. Level 1 data produced using this ARP are Provisional Data Quality.

Absolute: Larger than current algorithm. See T016.

Camera relative: 4%

Band and pixel: Same as most recent ARP (2% and 0.5% respectively).

T011 19 Nov 2001 00:19:10 10218 T011_F02_0001 D-PIN photodiodes used to calibrate C and D cameras; HQE for all other cameras.
T010 26 Sep 2001 00:56:52 9432 T010_F02_0001 In an effort to study camera-to-camera relative calibrations, the D-PIN photodiodes were used to calibrate the C and D cameras (HQE photodiodes were used for other cameras). An evaluation of the camera-relative calibrations followed.
T009 11 Jul 2001 01:27:11 8311 T009_F02_0001 A 5% aft-to-fore camera-relative bias has been discovered. This bias is present for all data products produced through T011 (T012 has applied the final correction algorithm). For ARP T009, separate calibration coefficients have been developed for the photodiodes as they view the North panel (used for aft and AN-red, nir channels) and the South panel (used for the fore- and AN-blue, green channels). This change was expected to improve fore-aft camera biases. In practice, several additional updates were made in T010 though T012 to correct this problem. Photodiodes used for T009: D-PIN for D camera, HQE for others.

Absolute: Larger than current algorithm. See T016.

Camera relative: 5%

Band and pixel: Same as most recent ARP (2% and 0.5% respectively).

T008 17 May 2001 01:19:09 7510 T008_F02_0001 Beginning with this delivery, a quadratic calibration equation is being used to convert the sensor data from DN to radiances values. This algorithm may change the radiances reported over dark, or ocean targets, by a few percent. Radiances reported over bright scenes are believed to be invariant with algorithm. Photodiodes used: HQE only.
T007 07 Mar 2001 01:17:44 6476 T007_F02_0001 Use was made of the June 11th Vicarious Calibration experiment to validate the Blue HQE photodiode. As a result of this study all radiances computed for MISR have been adjusted upwards by a factor of 1.10, irrespective of data acquisition time. The Linear Algorithm is used both to convert DN to Radiance and to generate ARP coefficients.

Absolute: Radiances are increased to remove a 10% bias from previous data products. Errors are still larger than the current algorithm. See T016.

Camera relative: 5%

Band and pixel: Same as most recent ARP (2% and 0.5% respectively)

T006 19 Dec 2000 19:29:18 5351 T006_F02_0001
T005 01 Nov 2000 21:06:26 4653 T005_F02_0001
T004 29 Aug 2000 14:25:43 3717 T004_F02_0001
T003 12 Jun 2000 4:16:43 2575 T003_F02_0001
T002 24 Feb 2000 16:41:00 995 T002_F02_0005
* Filename convention:
F = Format version
T = Time window
xxxx = revision number of this Time window file

Table 3 below describes ARPs that were used to create MISR reprocessing collection 4. These products were widely distributed. Collection 4 products will eventually be replaced by another reprocessing collection. This set of ARPs was generated with uniform quality in January, 2004, before the camera-by-camera adjustment was available.

Table 3. Historical Group of in-flight ARP data files used for reprocessing Collection 4
ARP ID File Version* Radiometric uncertainty
(for uniform targets)
T025-T026 F02_0001 Same as T024, described in Table 2.
T024 F02_0002 Same as T024, described in Table 2.
T019, T020, T022, T023 F02_0003 Same as T024, described in Table 2.
T021, T018 F02_0004 Same as T024, described in Table 2.
T017 F02_0005 Same as T024, described in Table 2.
T015 F02_0004 Same as T024, described in Table 2.
T002-T014, T016 F02_0003 Same as T024, described in Table 2.
* Filename conventions:
Txxx = Time window, defined in Table 2.
Fxx = Format version
xxxx = revision number of this Time window file

Warning: Do not use MISR Level 1 radiance products with the version number F03_0021. Products with this version number were generated with ARP files containing an error in the band-to-band calibration. This error resulted in Red band radiances that were 6% too high and Near-Infrared band radiances that were 2% high. All data products containing this error have been removed from the Langley DAAC archive. The first ARP to include the erroneous correction was T024_F02_0001, but T017-T023 were redelivered with the error at the same time. The Langley DAAC used these bad ARPs between December 5, 2003 and January 23, 2004.


Table 4. Bad in-flight ARP data files, producing Red radiances that are 6% high and NIR radiances that are 2% high.
ARP ID File Version* Radiometric uncertainty
(for uniform targets)
T024 F02_0001 N/A
T018 F02_0003 N/A
T017, T019-T023 F02_0002 N/A
* Filename conventions:
Txxx = Time window, defined in Table 2.
Fxx = Format version
xxxx = revision number of this Time window file

Further information may be found in the following papers:

The MISR Access Data Table contains a link to the MISR Validation website for those who desire more details.


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