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Level1_VIMS
Level1 VIMS ¶
VIMS Radiometric Calibration ¶
The application vimscal applies the dark current and flatfield correction to the input VIMS cube. vimscal requires ingestion into ISIS3 (vims2isis) and spiceinit (Level 0 processing)
Notes:
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By default, the output calibrated image cube will be in I/F Units and 32-bit for precision.
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All ISIS3 applications default to 'Tile' for output, regardless of the input file format
Example:
vimscal from=v1514302573_1_ir.cub to=C1514302573_1_ir.cub
vimscal from=v1514302573_1_vis.cub to=C1514302573_1_vis.cub
Sample image (v1514302573_1) is a VIMS observation of Titan [Sequence_Id=S17; Observation_Id=VIMS_019TI_HDAC001]
IR Portion: Samples=64 x Lines=64 x Bands=256
VIS Portion: Samples=64 x Lines=64 x Bands=96
Raw Camera Geometry ¶
Camera geometry for a Level 1 VIMS observation can be accessed following
a successful spiceinit (Level 0 Processing).
See Raw Camera Geometry
Display a VIMS cube ¶
Qview Plot ¶
Load and display a Multi-Band Cube ¶
- Qview will load an entire multi-band cube into memory.
Display Single Band in Black and White
Each Band can be selected to view as follows:
Display a Red, Green, Blue color composite
- Building
- Writing Tests
- Test Data
- Start Contributing
- Public Release Process
- Continuous Integration
- Updating Application Documentation
- Deprecating Functionality
- LTS Release Process and Support
- RFC1 - Documentation Delivery
- RFC2 - ISIS3 Release Policy
- RFC3 - SPICE Modularization
- RFC3 - Impact on Application Users
- RFC4 - Migration of ISIS Data to GitHub - Updated Information 2020-03-16
- RFC5 - Remove old LRO LOLA/GRAIL SPK files
- RFC6 - BLOB Redesign
- Introduction to ISIS
- Locating and Ingesting Image Data
- ISIS Cube Format
- Understanding Bit Types
- Core Base and Multiplier
- Special Pixels
- FAQ