Working_with_Cassini_ISS_Data

Working with Cassini ISS Data ¶

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• Working with Cassini ISS Data
  • About Cassini ISS (Imaging Science SubSystem)
    • Instrument Overview
    • Technical Details
    • References & Related Resources
  • Cartographic Processing ISS Data
    • Level 0 Processing
    • Level 1 Processing
    • Level 2 Processing

About Cassini ISS (Imaging Science SubSystem) ¶

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Instrument Overview ¶

The Imaging Science SubSystem (ISS) is used for multispectral imaging of Saturn, Titan, rings, and the icy satellites to observe their properties.

See: The Cassini Mission

Technical Details ¶

The ISS consists of two framing cameras. The narrow angle camera (ISS-NAC) is a reflecting telescope with a field of view of 0.35 degrees. The wide angle camera (ISS-WAC) is a refractor with a field of view of 0.35 degrees. Each camera is outfitted with a large number of spectral filters: 23 different filters for the NAC and 17 for the WAC spanning wavelengths of light from ultraviolet to the near-infrared. Each camera is a charged coupled device (CCD) detector consisting of a 1024 square array of pixels. The data system allows many options for data collection, including choices for on-chip summing and data compression.

References & Related Resources ¶

• ISS

Cartographic Processing ISS Data ¶

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Level 0 Processing ¶

1. Data Acquisition
2. Ingestion
3. SPICE
4. Raw Camera Geometry

Level 1 Processing ¶

1. Radiometric Calibration
2. Noise Removal

Level 2 Processing ¶

1. Map Projecting