Isis 3 Application Documentation
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Outputs a PVL file that contains camera infomation.
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Object = Caminfo
Object = Parameters
Program = caminfo
Version = 2.0
IsisVersion = "3.1.18beta | 2008-09-10"
RunDate = 2008-09-23T04:04:40
IsisId = MeSSEnGeR/MDIS-WAC/1/0108827809:757000
From = EW0108827809H_iof.cub
Lines = 1024
Samples = 1024
Bands = 1
End_Object
Object = Camstats
MinimumLatitude = -83.41440480372
MaximumLatitude = 3.7509815164171
MinimumLongitude = 130.12663958352
MaximumLongitude = 211.4118481043
MinimumResolution = 2837.9275992245
MaximumResolution = 3243.3476291415
MinimumPhase = 55.948494781205
MaximumPhase = 63.452364544485
MinimumEmission = 1.5987003275551
MaximumEmission = 89.906039419667
MinimumIncidence = 0.0061432307848179
MaximumIncidence = 84.83085856686
LocalTimeMinimum = 8.3450457249626
LocalTimeMaximum = 13.764059626348
End_Object
Object = Statistics
MeanValue = 0.027290557106805
StandardDeviation = 0.030059960910294
MinimumValue = 1.93800340639427e-04
MaximumValue = 0.13901169598103
PercentHIS = 0.0
PercentHRS = 0.0
PercentLIS = 0.0
PercentLRS = 0.0
PercentNull = 0.390625
TotalPixels = 1048576
End_Object
Object = Geometry
BandsUsed = 1
ReferenceBand = 1
OriginalBand = 1
Target = Mercury
StartTime = 2008-01-14T19:53:48.9698697
EndTime = 2008-01-14T19:53:48.9698697
CenterLatitude = -35.99699070995
CenterLongitude = 183.5425629901
CenterRadius = 2440000.0
UpperLeftLongitude = 130.629425434
UpperLeftLatitude = 2.2131023206612
LowerLeftLongitude = NULL
LowerLeftLatitude = NULL
LowerRightLongitude = NULL
LowerRightLatitude = NULL
UpperRightLongitude = NULL
UpperRightLatitude = NULL
PhaseAngle = 61.158147083403
EmissionAngle = 67.650944858113
IncidenceAngle = 36.012241921332
NorthAzimuth = 301.67928206242
OffNadir = 7.0664149700808
SolarLongitude = 251.5447380459
LocalTime = 11.906107285401
TargetCenterDistance = 2.2131023206612
SlantDistance = 17277.206903028
SampleResolution = 3082.7363142225
LineResolution = 3082.7363142225
PixelResolution = 3082.7363142225
MeanGroundResolution = 3040.5954926264
SubSolarAzimuth = 302.6826986422
SubSolarLatitude = -0.010137623850141
SubSolarLongitude = 184.95095370909
SubSpacecraftAzimuth = 220.05494431655
SubSpacecraftLatitude = -0.010137623850141
SubSpacecraftLongitude = 129.16259115677
ParallaxX = 106.67119905901
ParallaxY = -89.682221077406
ShadowX = -22.488549587781
ShadowY = -35.052794194572
HasLongitudeBoundary = FALSE
HasNorthPole = FALSE
HasSouthPole = FALSE
End_Object
Object = Polygon
CentroidLine = 444.50993729582
CentroidSample = 451.51727680485
CentroidLatitude = -29.640948990517
CentroidLongitude = 169.87095531121
CentroidRadius = 2440000.0
SurfaceArea = 8306887.6685914
GlobalCoverage = 11.103217
GisFootprint = "MULTIPOLYGON (((130.6294254340024850
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2.1768866704663559, 136.5989383173149179
2.1639614104686271, 138.6138732701137997
2.1544991617480225, 140.6479870975472579
2.1485370053737980, 142.7056447944214597
2.1461393256491279, 144.7915859682860571
2.1474007607611276, 146.9110313636781484
2.1524501894704975, 149.0698155062488013
2.1614560641171146, 151.2745557583258744
2.1746335423788317, 153.5328727459032621
2.1922540865408204, 155.8536845185811046
2.2146585384017592, 158.2476088770336560
2.2422752278895586, 160.7275286712950901
2.2756455971466307, 163.3094106296108805
2.3154614378397187, 166.0135340628912388
2.3626208040715224, 168.8664138091551763
2.4183154173570665, 171.9039685142860208
2.4841743385969286, 175.1770904293465208
2.5625157415150714, 178.7623042877256410
2.6568269305599421, 182.7846940640967830
2.7727925518573540, 187.4765775963039118
2.9209141292952903, 193.3794591608424014
3.1254813901633982, 202.8003290883544025
3.4888589890121060, 208.9133243384161744
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-40.1005881182147590, 208.1640541101386361
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-79.7808076095631549, 165.0757843694741496
-81.0881608166793910, 152.4799804246200949
-82.5308661672881669, 133.8681496681806493
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-29.3228321892930808, 130.2111932749780863
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-11.9906299772648701, 130.4162032634127115
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-2.0090910168198790, 130.5857852735746576
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1.9487429878277542, 130.6294254340024850
2.2131023206611959)))"
End_Object
End_Object
End
Output values that are not a range are calculated at the center of the image. The SubSpacecraftLatitude and SubSpacecraftLongitude make up the subspacecraft point, which is the point on a body which lies directly beneath the spacecraft. The SubSolarLatitude and SubSolarLongitude make up the subsolar point, which is the point on a body's refernce surface where a line from the body center to the sun center intersects that surface. The NorthAzimuth, SpacecraftAzimuth and SubSolarAzimuth are the values of the angle between a line from the image center to the relative point (North pole, SubSpacecraftLatitude/Longitude, SubSolar Latitude/Longitude respectively) and a reference line in the image plane. The reference line is a horizontal line from the image center to the middle right edge of the image. The angles increase in a clockwise direction. The LocalTime is the time at the current longitude relative to the subsolar longitude, which has a time of 12 o'clock. The SolarLongitude is LSubS, or the seasonal angle.
| Name | Description |
|---|---|
| FROM | Filename of a cube |
| TO | output PVL filename |
| Name | Description |
|---|---|
| GEOMETRY | Get Geometry Information |
| ISISLABEL | Write the ISIS label to the output file |
| ORIGINALLABEL | Get the Original Label |
| STATISTICS | Gather DN Statistics. |
| CAMSTATS | Get Camera Statistics Information |
| LINC | LINC for camstats |
| SINC | SINC for camstats |
| POLYGON | Creates polygon information |
| Name | Description |
|---|---|
| PIXINC | Polygon pixel increment |
| MAXEMISSION | Maximum emission angle to include in polygon |
| MAXINCIDENCE | Maximum incidence angle to include in polygon |
| Name | Description |
|---|---|
| SPICE | Run spiceinit on the input |
| Name | Description |
|---|---|
| VCAMERA | Test image center for valid camera |
Input cube with appropriate camera labels (Instrument and kernel groups). This file must be in raw camera space, which is a "level 1" cube. cube
| Type | cube |
|---|---|
| File Mode | input |
| Filter | *.cub *.CUB |
A text file in label format (PVL) which will contain the results of this program. This file can be used in conjunction with the 'getkey" program in order to pass the results to another program when developing scripts.
| Type | filename |
|---|---|
| File Mode | output |
| Internal Default | None |
| Filter | *.txt |
Get geometry information from the camera at the center of the image. These data are contained in the Geometry Object. The keyword/values contained there are:
BandsUsed
ReferenceBand
OriginalBand
Target
StartTime
EndTime
CenterLine
CenterSample
CenterLatitude
CenterLongitude
CenterRadius
RightAscension
Declination
UpperLeftLongitude
UpperLeftLatitude
LowerLeftLongitude
LowerLeftLatitude
LowerRightLongitude
LowerRightLatitude
UpperRightLongitude
UpperRightLatitude
PhaseAngle
EmissionAngle
IncidenceAngle
NorthAzimuth
OffNadir
SolarLongitude
LocalTime
TargetCenterDistance
SlantDistance
SampleResolution
LineResolution
PixelResolution
MeanGroundResolution
SubSolarAzimuth
SubSolarGroundAzimuth
SubSolarLatitude
SubSolarLongitude
SubSpacecraftAzimuth
SubSpacecraftGroundAzimuth
SubSpacecraftLatitude
SubSpacecraftLongitude
ParallaxX
ParallaxY
ShadowX
ShadowY
HasLongitudeBoundary
HasNorthPole
HasSouthPole
| Type | boolean |
|---|---|
| Default | TRUE |
This option will extract the ISIS label and write it to the output PVL file.
| Type | boolean |
|---|---|
| Default | FALSE |
Get the original label blob and add it to the PVL.
| Type | boolean |
|---|---|
| Default | FALSE |
Get DN statistics for all band within the cube. These data are contained in the Statistics object. The keyword/values contained therein are:
MeanValue
StandardDeviation
MinimumValue
MaximumValue
PercentHIS
PercentHRS
PercentLIS
PercentLRS
PercentNull
TotalPixels
| Type | boolean |
|---|---|
| Default | FALSE |
Run camstats to get camera information that can be expressed as a range. Camstats will run on the entire cube (common object), and then for each band(bandset object). The default linc and sinc for camstats will is "1", the user can select a different linc and sinc. Output values are:
Minimum Latitude
Maximum Latitude
Minimum Longitude
Maximum Longitude
Minimum Resolution
Maximum Resolution
Minimum Phase
Maximum Phase
Minimum Emission
Maximum Emission
Minimum Incidence
Maximum Incidence
Minimum Local Time
Maximum Local Time
| Type | boolean |
|---|---|
| Default | FALSE |
| Inclusions |
|
This is the line incrument used by camstats.
| Type | integer |
|---|---|
| Default | 1 |
This is the sample incrument used by camstats.
| Type | integer |
|---|---|
| Default | 1 |
use the imagePolygon class to gather ploygon information. The output polygon will be in well known text format (WKT). These data are contained within the Polygon object. The keyword/values contained therein are:
CentroidLine
CentroidSample
CentroidLatitude
CentroidLongitude
CentroidRadius
SurfaceArea
GlobalCoverage
GisFootprint
| Type | boolean |
|---|---|
| Default | FALSE |
Specifies the number of pixels skip around the perimiter of the image to compute the polygon footprint. Note that currently, an increment of 1 will not work for pushframe instruments such as THEMIS-VIS. A default of 0 will cause caminfo to aribitrarily set it to 100.
| Type | integer |
|---|---|
| Default | 0 |
Specifies the maximum emission angle that a polygon point is allowed to have. This limit is useful for eliminating limb data that cause numerous ragged spikes. Limb data will generally result in odd polygon footprints as the geometry becomes unstable at the limb due to obliqueness particularly when using a DEM for the shape model (see spiceinit). This parameter restricts the emission angle to create better behaved poygons at the limb while sacrificing some (very oblique) data.
Note the images spiceinit'ed with a DEM, the emission angle may need to shorted. The DEM at the limb will also cause additional spiking.
The default value assumes no DEM is assocaited wth movie.
| Type | double |
|---|---|
| Default | 89.5 |
Specifies the maximum incidence angle that a polygon point is allowed to have. This limit is useful for eliminating terminator data that may will typically be lost in photometric corrections. This parameter restricts the incidence angle to create more data relevant polygons at the terminator while sacrificing some (non-photometric) data.
| Type | double |
|---|---|
| Default | 120.0 |
If the user sets this to true then the spiceinit program will be run on the input file. Spiceinit will use the system SPICE kernels, so any updates to SPICE information will be lost. Spiceinit is in this program to facilitate UPC processing.
| Type | boolean |
|---|---|
| Default | FALSE |
If the user sets this parameter to true, a test will determain if a valid camera can be created at the center of the image band. if a valid camera cannot be created the program will end. The default is to not test the camera and output any available information.
| Type | boolean |
|---|---|
| Default | FALSE |
| Robert Sucharski | 2007-04-10 | Original version |
| Steven Lambright | 2007-08-10 | Added an application test |
| Steven Koechle | 2007-11-01 | Fixed WKT calls |
| Tracie Sucharski | 2007-11-09 | Remove ToWKT calls and PolygonTools.h inclusion. The geos package now has a method to return a WKT string, so the ToWKT method has been removed from the PolygonTools class. |
| Kris Becker | 2007-12-07 | Made the following modifications: fixed typo in PercentNull and MaximumLongitude keywords; use the base file name for generation of temporary files to further ensure uniqueness; run camstats once if there is only one band - doubles execution speed for single band images when CAMSTATS option is used; substitute the NULL string for all special pixel values; added corner pixel keywords for PDS compatability; added phase, emission, incidence angles and line and sample pixel resolution at the center pixel; added test for intersection of longitude domain, north and south poles and keywords that report them; added option to output ISIS cube labels; corrected computations for parallax and shadow keywords. |
| Kris Becker | 2007-12-19 | Renamed the HasLongitudeDomain keyword to HasLongitudeBoundary. Makes more sense. |
| Kris Becker | 2008-02-27 | Corrected method call to compute polygon with proper parameters as well as correct band number. Added code to better honor specific cube attributes (such as band numbers) in computations. Also will produce NULL valued keywords where NULLs are a produced instead of the real value for the ISIS NULL pixel value. |
| Steven Lambright | 2008-05-12 | Removed references to CubeInfo |
| Bob Sucharski | 2008-07-31 | Added Camera Test option to test for a valid camera at center of image and return an error and end if a valid camera cannot be created. |
| Kris Becker | 2008-09-22 | Reworked the output PVL format; added more keywords to the Common object that indicate versions and dates; added more values to Geometry and Polygon object. |
| Kris Becker | 2008-10-22 | Corrected generation of polygon for multi-band data. It created a POLYGON union instead of the required MULTIPOLYGON. |
| Kris Becker | 2008-10-30 | The target center distance and subspacecraft latitude were not properly propagated to the output PVL file and consequently were invalid. This has been corrected. |
| Kris Becker | 2008-12-29 | Added RightAscension, Declination, SubSolarGroundAzimuth, and SubSpacecraftGroundAzimuth computations; added center line/sample image coordinate used to compute center geometry; added check of valid image line/sample coordinates when testing for north/south poles (some camera models return valid states when coordinates are outside of image boundaries). |
| Kris Becker | 2009-02-26 | Modified to actually exclude the unconditional computation of the image polygon to assist in some geometry values. It is no longer computed if the user does not select the POLYGON option. The implications of this are that some of the keywords in the output Geometry group are no longer ever relevant. These keywords were all moved to the Polygon group. These keywords are: CentroidLine, CentroidSample, CentroidLatitude, CentroidLongitude, CentroidRadius and SurfaceArea. User will no longer see these values if the POLYGON option is not selected. Also the Radius keyword in the Polygon group has been removed as it is redundant with CentroidRadius. |
| Kris Becker | 2009-05-29 | Added PIXINC parameter to allow user to specify number of pixels to skip around the perimiter of the image to compute the polygon. |
| Kris Becker | 2009-05-29 | Fixed bug where image was a 0 longitude boundary crosser. It would typically fail when determining centroid information unless converted to 180 domain. This will also be used at the poles as it seems to work better in the 180 domain as well. (This process projects the footprint to a Sinusoidal projection to determine area which requires an equal area projection, such as Sinusoidal.) |
| Kris Becker | 2009-07-08 | Added the MAXEMISSION and MAXINCIDENCE limit parameters to better control limb and terminator polygon generation. |
| Kris Becker | 2009-08-24 | Allow disabling of shape model use when constructing polygons that contain limbs. |