50 MASTER Configuration for 18-657-00  20 Jun 2018  
01 01 16 0 0.032756 0.0000  0.439  0.462  0.482 0.100 2034.16
02 02 16 0 0.051224 0.0000  0.478  0.504  0.524 0.100 1930.16
03 03 16 0 0.036594 0.0000  0.522  0.544  0.566 0.100 1879.98
04 04 16 0 0.046590 0.0000  0.562  0.582  0.604 0.100 1798.90
05 05 16 0 0.051654 0.0000  0.633  0.654  0.693 0.100 1553.01
06 06 16 0 0.066837 0.0000  0.693  0.712  0.734 0.100 1397.17
07 07 16 0 0.042536 0.0000  0.732  0.752  0.773 0.100 1280.79
08 08 16 0 0.042378 0.0000  0.782  0.802  0.823 0.100 1130.94
09 09 16 0 0.034640 0.0000  0.848  0.868  0.889 0.100  976.80
10 10 16 0 0.027960 0.0000  0.888  0.908  0.929 0.100  926.07
11 11 16 0 0.026306 0.0000  0.928  0.948  0.970 0.100  848.26
12 12 16 0 0.008419 0.0000  1.574  1.604  1.630 0.018  247.88
13 13 16 0 0.007335 0.0000  1.631  1.660  1.686 0.015  230.82
14 14 16 0 0.006351 0.0000  1.689  1.716  1.741 0.015  206.00
15 15 16 0 0.006192 0.0000  1.743  1.770  1.796 0.015  179.19
16 16 16 0 0.004817 0.0000  1.797  1.830  1.847 0.010  159.47
17 17 16 0 0.004626 0.0000  1.853  1.876  1.895 0.010  140.07
18 18 16 0 0.004286 0.0000  1.902  1.928  1.952 0.010  132.41
19 19 16 0 0.004175 0.0000  1.952  1.976  2.000 0.010  124.16
20 20 16 0 0.002949 0.0000  2.054  2.078  2.102 0.010   98.07
21 21 16 0 0.003154 0.0000  2.136  2.160  2.183 0.010   81.05
22 22 16 0 0.003353 0.0000  2.185  2.210  2.233 0.010   74.38
23 23 16 0 0.003347 0.0000  2.235  2.258  2.282 0.010   69.69
24 24 16 0 0.002296 0.0000  2.293  2.318  2.364 0.010   59.88
25 25 16 0 0.002571 0.0000  2.363  2.386  2.426 0.010   57.04
26 26 16 1 0.952520 0.0000  3.984  4.065  4.131 0.100    8.12
27 27 16 1 0.964037 0.0000  3.206  3.280  3.356 0.010   17.94
28 28 16 1 0.964243 0.0000  3.356  3.450  3.516 0.010   15.09
29 29 16 1 0.961219 0.0000  3.514  3.590  3.665 0.010   12.86
30 30 16 1 0.957902 0.0000  3.669  3.750  3.808 0.010   11.06
31 31 16 1 0.954554 0.0000  3.824  3.910  3.981 0.010    9.46
32 32 16 1 0.952520 0.0000  3.984  4.065  4.131 0.010    8.12
33 33 16 1 0.950117 0.0000  4.166  4.238  4.319 0.010    6.79
34 34 16 1 0.948980 0.0000  4.300  4.372  4.453 0.001    5.97
35 35 16 1 0.946107 0.0000  4.449  4.525  4.593 0.010    5.22
36 36 16 1 0.943250 0.0000  4.599  4.685  4.748 0.010    4.53
37 37 16 1 0.942143 0.0000  4.749  4.840  4.900 0.010    3.99
38 38 16 1 0.940173 0.0000  4.901  4.985  5.043 0.010    3.54
39 39 16 1 0.937848 0.0000  5.045  5.130  5.189 0.010    3.17
40 40 16 1 0.940760 0.0000  5.197  5.260  5.335 0.010    2.83
41 41 16 1 0.973157 0.0000  7.649  7.820  7.934 0.010    0.66
42 42 16 1 0.971481 0.0000  7.928  8.190  8.373 0.010    0.54
43 43 16 1 0.968865 0.0000  8.407  8.630  8.793 0.010    0.44
44 44 16 1 0.950971 0.0000  8.828  9.050  9.256 0.010    0.36
45 45 16 1 0.944660 0.0000  9.480  9.700  9.874 0.010    0.28
46 46 16 1 0.952338 0.0000  9.901 10.100 10.277 0.010    0.23
47 47 16 1 0.954040 0.0000 10.320 10.560 10.941 0.010    0.19
48 48 16 1 0.956128 0.0000 10.987 11.290 11.698 0.010    0.15
49 49 16 1 0.958519 0.0000 11.890 12.090 12.391 0.010    0.11
50 50 16 1 0.957416 0.0000 12.641 12.840 13.113 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 124 MASTR
ExperimentName           HyspIRI_SumFall2018
AircraftPlatform         NASA ER2 (806)
NavFormatCode            POS 50Hz (C-3)
LocationCode             Global Pos (GPS)
AltitudeCode             Global Pos (GPS)
CalibrationVersion       Version 3.0 Calibration
CalibrationName          Summer18_061218-092118_1018
SRF_Dataset              /calibration/calibrat/MASTER/srf/Oct_18/
SRF_FTP                  https://asapdata.arc.nasa.gov/MASTER/srf/Oct_18/
NavDataSource            Applanix POSAV 510
NavDataPath              /archive/nav/2018/er2/bet062018
TbackBand                48, 47, 30, 273.15
GranuleVersion           2.0
MetadataVersion          2.0
GeoLocationProcess       MasterGeo (3.0-D)
MGeoControlFilePath      Control_mgeo_18657_utm10.txt
FlightComment            SARP 2018 Flight 1; Thomas Fire Scar
------------------------------------------------------------------------------
------------------------------------------------------------------------------
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 2A/2B.
Aeroglaze Z306 Flat Black installed October 2017
Emissivities used were from Simon Hook's calculation
and embedded in MASCAL.F program (mascal_master.f).
*************************
*************************

Config creation date: Nov 16, 2018