Corrected navigation filename. If marsnav was run on the input images it created a table of corrected pointing parameters. If you refer to this table using NAVTABLE it will override the pointing parameters (e.g. azimuth and elevation) in the picture labels, giving you a better registered output.
VICAR image which camera model forms a pair of almost aligned camera models with input image's camera model. If stereo_partner is not present, the program tries to find stereo partner of the input image based on mission, instrument etc. info of the input image. The presence of stereo_partner input parameter is an unconditional overwrite of that process. Note that for a generic camera, there is absolutely no way to tell what the stereo partner might be, or even if there is one. Thus using stereo_partner input parameter is the ONLY way to specify stereo pair for generic image.
Overrides size of the input image. If the input image is a subframe and the camera model in the label corresponds to the fullframe image, FULLSIZE would specify the size of the fullframe. Moreover, the presence of this input parameter would tell us that we are in the situation described above and need to deal with it accordingly.
Overrides size of the output image. (NL, NS) order.
Sets size of output image to be the minimum or maximum of each dimension in both inputs. Ignored if stereo_partner is not given.
Overrides x/y offset values for output. This offset is the distance from the camera coordinate origin to the image origin (0-based) and affects where the center of the projection falls in the output.
The BSQ input file band number. Defaults to 1
The local mars surface normal vector coordinate system specified by SURF_COORD parameter (defaults to surface fixed). For most pan/tilt cameras, if the lander is not tilted this vector would be: normal=(0,0,-1). ie: x_component=0, y_component=0, z_component=-1. This need not be a unit vector. This vector is used to define the surface plane to which image points are projected in order to minimize parallax. For SPHERE1/2 surface models, normal's first parameter is used to denote sphere's radius. Thus to describe sphere of radius R, user would specify normal=(R, 0, 0).
Any point on the surface, in coordinate system specified by SURF_COORD parameter (defaults to surface fixed). This defines where the tilted plane is in space. Although any point may be used, normally the point just "under" the origin is selected. Defaults: Mars Pathfinder: (0.0, 0.0, 0.0) (lander zero point is on the ground) Mars 98 Lander: (0.0, 0.0, 1.64) (lander zero point is on top of deck) MER : (0.0, 0.0, 0.294) For MER images taken on top of the lander, the ground is roughly at (0.0, 0.0, 0.7) For SPHERE1/2 surface models, GROUND parameter is used to denote sphere's center.
The coordinate system that surface parameters like GROUND and NORMAL are defined in. For valid values refer to COORD parameter description. The interpretation of the values is dependent on the mission. Defaults to surface fixed coordinate system. Note that no validation is done for input strings because COORD is using the same values. So user needs to be extra careful in specifying SURF_COORD value. For example COORD=local would be correctly interpreted to mean LOCAL_LEVEL because of validation process. On the other hand specifying SURF_COORD=local would lead to underlying code treating the input value as invalid and reverting to default which is FIXED frame. So the values for SURF_COORD should be spelled exactly as found in the list of valid values for COORD parameter.
Radius of surface sphere.
The type of mars surface to use. The surface is used to intercept view rays emanating from the cameras in order to model out parallax between the stereo cameras. The two options are surface=INFINITY which means no surface is used or surface=PLANE (the default case). If surface =PLANE then the plane is defined by the NORMAL parameters. If surface = SPHERE then the sphere is defined by radius and center.
Keyword parameter that turns on or off radiometric correction of the input images. RAD (the default) enables the correction (for missions/instruments which support it), while NORAD disables it.
DN scaling factor. This factor is used to convert between physical radiometric units (watts/(meter**2, steradian, micron)) and DN's for the output. The formula is: true_radiance = offset + (factor * DN) where "offset" is 0.0 in the current implementation, and "factor" is 1.0 / DNSCALE (making the formula equivalently: offset + (DN / DNSCALE)). The offset and factor (1.0/DNSCALE) are written to the output label.
A colon-separated list of directories in which to look for configuration and calibration files. Environment variables are allowed in the list (and may themselves contain colon-separated lists). The directories are searched in order for each config/cal file when it is loaded. This allows multiple projectes to be supported simultaneously, and allows the user to override any given config/cal file. Note that the directory structure below the directories specified in this path must match what the project expects. For example, Mars 98 expects flat fields to be in a subdirectory named "flat_fields" while Mars Pathfinder expects them to be directly in the directory specified by the path (i.e. no intermediate subdirectories).
Specifies a method for pointing corrections. Loose method matchs with pointing parameters of the image. Tight method matchs with unique id of the image.
Tolerance value for matching pointing parameters in the pointing corrections file. Used if MATCH_METHOD=LOOSE Default value is pretty arbitrary, though seems to work well so far....
Specifies a mission-specific pointing method to use. Normally this parameter is not used, in which case the "default" pointing methods are used. Some missions may have special, or alternate, pointing methods available, which are indicated by this string (for example, backlash models, using arm joint angles instead of x/y/z/az/el, etc). A substring search is used, so multiple methods (where that makes sense) can be specified by separating the keywords with commas. Note that nav files created using one pointing method will most likely not be compatible with a mosaic created using a different pointing method. The methods available vary per mission, but some methods available at the time of this writing are: CAHV_FOV: All Missions using CAHV-based camera models. Valid values are: * MIN or INTERSECT: Aligning stereo-pair cameras produces virtual camera with FOV equal to INTERSECTION area of two input cameras. (default) As a result, the output image is missing,sometimes a significant, (depending on camera geometry) part of overlap area between two cameras but there are no black areas on the side. The image data is stretched in horizontal direction. * MAX or UNION: Aligning stereo-pair cameras produces virtual camera with FOV equal to UNION area of two input cameras. The result is the opposite of the MIN option: wide black areas on the side, but the stereo-pair's intersection area is preserved. The image data is squeezed in horizontal direction. Note that the above two entries have two names each, which are equivalent and it's up to the user to decide which one is more intuitive to him/her. * LINEAR: Uses only CAHV vectors and ignores higher order terms OR(E) while aligning the cameras. As a result, this mode has advantage of best preserving horizontal aspect ratio. The features in the image look similar, scale-wise, to the original. BACKLASH : Mars 98 SSI only. Selects a backlash pointing model, which adjusts the telemetered azimuth and elevation values based on knowledge of the camera's mechanical backlash and the direction the motor was travelling when the image was taken.
Disables all label-derived parameters to the Site mechanism which underlies coordinate systems. This forces all sites to be identical, with all rotations and offsets set the same. In the case of MPF or Mars 98, this disables the lander quaternion and offset (sets them to identity and 0, respectively). This option should not be used with images taken from different vantage points (e.g. the spacecraft moved, or mixing a lander and a rover) or invalid results will be obtained. The use of this option invalidates the Fixed coordinate frame; any values reported in the Fixed frame will not correctly reflect the orientation of the lander/rover. Obviously, this option should be rarely used; it is intended for when the image labels defining the site are invalid or inconsistent.
Keyword parameter that turns on or off interpolation of the output images pixel values. INTERP (the default) enables the interpolation, while NOINTERP disables it.
The UNSUB mode will "un-subframe" the image before linearizing it. When this mode is on, the program looks up the nominal size of the camera frame (using the camera mapping file), and sets the output to be that size. It then puts the input in the right position in the output according to the subframe start (FIRST_LINE and FIRST_LINE_SAMPLE labels for most missions). From then on, it proceeds as if a full-frame image had been given. This is useful for cameras like the MSL Mastcam, where the differential zoom on both eyes causes them to often do different subframes on the two eyes. Removing the subframe puts it all back in the same geometry again, so downstream programs that need the same image size for both eyes can work.
Turns on or off parallel processing. The default is on. The main help describes some environment variables that can further control parallel processing. Note that this program uses standard OpenMP (which is built in to the gcc/g++ compilers), so further details can be found in the OpenMP documentation.
The DATA_SET_NAME typically identifies the instrument that acquired the data, the target of that instrument, and the processing level of the data. This value is copied to the output label, property IDENTIFICATION, keyword DATA_SET_NAME.
The DATA_SET_ID value for a given data set or product is constructed according to flight project naming conventions. In most cases the DATA_SET_ID is an abbreviation of the DATA_SET_NAME. This value is copied to the output label, property IDENTIFICATION, keyword DATA_SET_ID.
When a data set is released incrementally, such as every three months during a mission, the RELEASE_ID is updated each time part of the data set is released. For each mission(or host id if multiple spacecrafts), the first release of a data set should have a value of "0001". This value is copied to the output label, property IDENTIFICATION, keyword RELEASE_ID.
Specifies a permanent, unique identifier assigned to a data product by its producer. Most commonly, it is the filename minus the extension. This value is copied to the output label, property IDENTIFICATION, keyword PRODUCT_ID.
Specifies the unique identifier of an entity associated with the production of a data set. This value is copied to the output label, property IDENTIFICATION, keyword PRODUCER_ID.
Specifies the identity of a university, research center, NASA center or other institution associated with the production of a data set. This value is copied to the output label, property IDENTIFICATION, keyword PRODUCER_INSTITUTION_NAME.
Specifies a target. The target may be a planet, satelite, ring, region, feature, asteroid or comet. This value is copied to the output label, property IDENTIFICATION, keyword TARGET_NAME.
Specifies the type of a named target. This value is copied to the output label, property IDENTIFICATION, keyword TARGET_NAME.
Rover State File. This is a list of filenames to load containing Rover State information. These files contain position and orientation information for a rover (or other mobile spacecraft) at various sites. They are in XML format. See the "Rover Motion Counter (RMC) Master File SIS " for details on these files. Rover State Files have a priority order. The files listed first have the highest priority. Environment variables may be used in the list. For MER, if a directory is specified, then that directory is searched for RMC Master files and any found are loaded. The directory structure and filename convention is covered in the RMC SIS. The directory specified is the one containing "master", so if <dir> is the name specified in the RSF parameter, the following files will be searched for: <dir>/master/
_Master.svf <dir>/master/ _Site_ _Master.rvf The name of each file loaded is printed to the stdout log for reference.
If enabled, this causes the internal database of RMC locations to be printed out to the stdout log. This is after the RSF files have been loaded and the coordinate systems read from the input label(s).
The coordinate system to use for the output camera model. Also the coordinate system used for the actual ray tracing. Note that the surface model parameters are always expressed in the Fixed site, however. The interpretation of the values is dependent on the mission. Some representative missions are listed here: Fixed - The Fixed frame (default). This is the ultimate reference frame (see also FIXED_SITE for rover missions). Instrument - The "natural" frame for the instrument (of the first input image). MPF: Lander or Rover; M98: MVACS; MER: Rover. Site - A major Site frame. For rover missions, COORD_INDEX specifies which Site frame to use. Non-rover missions treat this as Fixed. Rover - An instance of the Rover frame. For rover missions, COORD_INDEX specifies which instance of the rover frame to use. Non-rover mission use the spacecraft frame (e.g. Lander for M98). Local_Level - An instance of a Local Level frame. This is typically coincident with the Rover frame (in XYZ) but oriented toward North like the Site and Fixed frames. For MER, this is an instance of a Drive index move.
The index specifies which instance of a coordinate system to use. It is currently applicable only to rover-based missions, but could have other uses. The index is equivalent to the Rover Motion Counter (RMC) for MER and FIDO. For MER/FIDO, there are many Site frames. Each is numbered with a single index. For Site Frames, coord_index specifies which to use. Likewise, there are many Local_Level and Rover frames, corresponding to values of the RMC. The multiple instances of this frame are selected by COORD_INDEX. Generally COORD_INDEX defaults sensibly so you don't usually need to specify it. It will default to the instance used by the first input.
Specifies which major Site is the "Fixed" Site for this run. Historically, MPF and M98 had a single "Surface Fixed" frame which never moved, and which all other coordinate system frames were referenced to. With the advent of long-range rovers (such as MER and FIDO), that became insufficient. The rover traverses far enough that errors in knowledge of coordinate system offset and orientation become unacceptable. For this reason, a system of major Sites was introduced. Periodically during the mission, a Site frame is declared. This then becomes the reference frame for all activities until the next Site is declared. References are kept local, and errors don't propogate across Sites. However, if images from more than one Site are combined together, the Site's must be placed relative to each other. Therefore a single reference frame is still needed to combine different sites. The FIXED_SITE parameter controls which of the major Site frames is the reference ("fixed") site for this program run. This fixed frame can vary in different program runs, but is constant throughout one execution. If not specified, FIXED_SITE defaults to the minimum Site number (i.e. lowest numbered, or earliest chronologically) used in all input images. Normally this default is sufficient; rarely must FIXED_SITE be specified. One or more Rover State Files must usually be specified in order to combine image from more than one Site. These describe the relationship between sites. See the RSF parameter.
Specifies which solution ID to use for pointng corrections. There are potentially many different definitions for the same coordinate system. These are identified via a unique Solution ID. If this parameter is given, only the specified solution's definition is searched for.