50 MASTER Configuration for 23-912-00  12 Sep 2023  San Joaquin Valley CA
01 01 16 0 0.019127 0.0000  0.438  0.460  0.481 0.100 1991.20
02 02 16 0 0.027976 0.0000  0.476  0.500  0.521 0.100 1961.63
03 03 16 0 0.022479 0.0000  0.520  0.542  0.563 0.100 1888.51
04 04 16 0 0.026974 0.0000  0.560  0.580  0.601 0.100 1825.00
05 05 16 0 0.031882 0.0000  0.631  0.654  0.691 0.100 1548.34
06 06 16 0 0.039771 0.0000  0.690  0.712  0.732 0.100 1387.78
07 07 16 0 0.027348 0.0000  0.730  0.750  0.771 0.100 1263.00
08 08 16 0 0.025699 0.0000  0.779  0.800  0.820 0.100 1128.53
09 09 16 0 0.022811 0.0000  0.845  0.866  0.887 0.100  953.87
10 10 16 0 0.017258 0.0000  0.886  0.906  0.927 0.100  882.56
11 11 16 0 0.017378 0.0000  0.926  0.946  0.968 0.100  805.44
12 12 16 0 0.005729 0.0000  1.573  1.602  1.630 0.018  242.20
13 13 16 0 0.005048 0.0000  1.631  1.660  1.687 0.015  219.73
14 14 16 0 0.004461 0.0000  1.688  1.714  1.740 0.015  196.76
15 15 16 0 0.004440 0.0000  1.743  1.768  1.795 0.015  175.80
16 16 16 0 0.003353 0.0000  1.797  1.818  1.847 0.010  156.63
17 17 16 0 0.003153 0.0000  1.854  1.876  1.894 0.010  141.04
18 18 16 0 0.003165 0.0000  1.901  1.932  1.953 0.010  129.29
19 19 16 0 0.003063 0.0000  1.953  1.976  2.001 0.010  118.56
20 20 16 0 0.002129 0.0000  2.056  2.080  2.103 0.010   99.80
21 21 16 0 0.002244 0.0000  2.138  2.162  2.185 0.010   86.00
22 22 16 0 0.002397 0.0000  2.188  2.212  2.236 0.010   79.87
23 23 16 0 0.002287 0.0000  2.239  2.262  2.285 0.010   73.47
24 24 16 0 0.001564 0.0000  2.297  2.344  2.367 0.010   65.50
25 25 16 0 0.001688 0.0000  2.367  2.390  2.431 0.010   59.18
26 26 16 1 0.999470 0.0000  3.980  4.055  4.123 0.010    8.16
27 27 16 1 0.997730 0.0000  3.209  3.295  3.351 0.010   17.89
28 28 16 1 0.997831 0.0000  3.360  3.455  3.509 0.010   15.08
29 29 16 1 0.998505 0.0000  3.518  3.605  3.667 0.010   12.79
30 30 16 1 0.999180 0.0000  3.672  3.760  3.809 0.010   11.01
31 31 16 1 0.999511 0.0000  3.821  3.920  3.981 0.010    9.44
32 32 16 1 0.999470 0.0000  3.980  4.055  4.123 0.010    8.16
33 33 16 1 0.998927 0.0000  4.168  4.240  4.321 0.001    6.77
34 34 16 1 0.998469 0.0000  4.302  4.374  4.455 0.001    5.96
35 35 16 1 0.997917 0.0000  4.442  4.515  4.581 0.001    5.25
36 36 16 1 0.997364 0.0000  4.591  4.680  4.734 0.010    4.58
37 37 16 1 0.997070 0.0000  4.741  4.825  4.891 0.010    4.02
38 38 16 1 0.996969 0.0000  4.892  4.980  5.031 0.010    3.57
39 39 16 1 0.996969 0.0000  5.035  5.110  5.173 0.010    3.19
40 40 16 1 0.997285 0.0000  5.186  5.260  5.321 0.010    2.85
41 41 16 1 0.997554 0.0000  7.669  7.830  7.948 0.010    0.65
42 42 16 1 0.996341 0.0000  7.962  8.250  8.400 0.010    0.53
43 43 16 1 0.995117 0.0000  8.433  8.650  8.804 0.010    0.44
44 44 16 1 0.994270 0.0000  8.875  9.090  9.269 0.010    0.36
45 45 16 1 0.993840 0.0000  9.511  9.720  9.894 0.010    0.27
46 46 16 1 0.994097 0.0000  9.918 10.120 10.295 0.010    0.23
47 47 16 1 0.994214 0.0000 10.338 10.600 10.943 0.010    0.19
48 48 16 1 0.994845 0.0000 10.984 11.250 11.680 0.010    0.15
49 49 16 1 0.995844 0.0000 11.877 12.090 12.379 0.010    0.11
50 50 16 1 0.996807 0.0000 12.630 12.860 13.100 0.010    0.09
|  |  |  | |        |       |      |      |     |        |
|  |  |  | |        |       |      |      |     |        =(!)
|  |  |  | |        |       |      |      |     =-Scale Factor
|  |  |  | |        |       |      |      =- Right 50% spectral response
|  |  |  | |        |       |      =-Peak 100% spectral response (microns)
|  |  |  | |        |       =-Left 50% spectral response (microns)
|  |  |  | |        =-Calibration intercept (only used for visible bands)
|  |  |  | =--------Calibration slope (only used for visible bands 1-25)
|  |  |  |          Blackbody emmissivity (only used for IR bands 26-50)
|  |  |  =----------0 => visible band, 1 => thermal infrared band
|  |  =-------------Number of bits in this channel (8 or 16)
|  =----------------Spectral band assigned to this channel
=------------------------- Channel number                
(!) Sensor weighted solar spectral irradiance (Watts/meter2/micron)
at mean Earth-Sun distance                               
                                                         
NOTE: Factor in column 10 is used to scale radiances in  
      calibrated data by the following method:           
      value_stored = int( radiance / factor ) for each channel
------------------------------------------------------------------------------
------------------------------------------------------------------------------
Title                    MODIS/ASTER Airborne Simulator (MASTER) Level-1B Data
Sensor_ID_Code           MS 178 MASTR
ExperimentName           GEMx
CampaignName             Summer2023
AircraftPlatform         NASA ER2 (809)
NavFormatCode            POS Standard (C-3)
LocationCode             Global Pos (GPS)
AltitudeCode             Global Pos (GPS)
CalibrationVersion       Version 1.0 Calibration
CalibrationName          Summer2023_081123_000000
SRF_Dataset              /calibration/calibrat/MASTER/srf/Jul_23/
SRF_FTP                  https://asapdata.arc.nasa.gov/sensors/master/data/srf/Jul_23_srf.html
NavDataSource            Applanix POSAV 510
NavDataPath              /archive/nav/2023/er2/bet230912
TbackBand                48, 273.15
GranuleVersion           1.0
MetadataVersion          1.0
GeoLocationProcess       MasterGeo (3.0-D)
MGeoControlFilePath      Control_23912_30m_utm11.txt
FlightComment            Modified PreAmp Ch31 (3.9um)
------------------------------------------------------------------------------
------------------------------------------------------------------------------
Conversion from counts to radiance in VIS and NIR channels

rad = (count - (cbb_avg)) * slope

where,
rad         = radiance
cbb_avg     = cold black body counts (running average)
slope       = from column 7 in above table
count       = count value
There was no instrument temperature correction performed.

***********************************
IR Emissivity Correction (for MAS-50{adopted for MASTER})
>From Chris Moeller (UWisc) and Simon Hook (JPL)
***********************************
This is done in 2 steps:
1. Get the 11um scan head count and convert it to a 
brightness temperature using UWisc subroutine TEMBCK.F
(from Liam Gumley (UWisc))
2. Call subroutine MASCAL.F (from Liam Gumley (UWisc)) which
uses the 11um band scan head temperature and the cold 
and warm black body counts/temperatures for computing
the corrected slope and intercept for all IR bands.

Revised emissivities are representative of BB plates.
Vanta Black plates installed Dec 2019
Emissivities used were from Simon Hook's calculation
and embedded in MASCAL.F program (mascal_master.f).
*************************
*************************
Config creation date: Oct 03, 2023