Hawk Hyperspectral Sensor

The Hawk sensor is a short wave infra-red hyperspectral instrument manufactured by ​Specim. It operates as a separate instrument, but complimentary with, the Eagle hyperspectral instrument.

Raw data format

The Hawk data is captured as ENVI format BIL files (a pair of .hdr and .raw), with an associated nav file per line. The .hdr files are ASCII text files where as the .raw and .nav are binary data files.

The Hawk .raw data files contain 14-bit data (values of 0-16383) stored as 16-bit integer. The first pixel of the first band of each raw file is the frame counter pixel, which is essentially a frame id tag that increments by 1 through out the file. At the end of the raw file, after data capture for this flight line, a number of lines of data are captured with the shutter closed. These lines are referred to as "dark lines" and give sensor ccd values for when no light is present.

The .nav files are a collection of different 'messages'. These contain the real-time position and attitude of the aircraft as well as periodic time stamps marking the start of the flight line capture.

Specifications

Detector size	320x256
Bit depth (of sensor analog to digital converter)	12 bit
Spatial pixels	320 (unbinned)
Spectral pixels	256 typically ~220 in use
Spectral resolution	12 nm
Nominal spectral range (prior to calibration)	970-2500nm
Central pixel number	160 (unconfirmed)
Focal length	22.8mm (manufacturer supplied) (22.5mm on manufacturer datasheet retrieved 20090817 - ​http://www.specim.fi/products/aisa-airborne-hyperspectral-systems/aisa-series.html
Field of View (FOV)	24.0 degrees (from manufacturer datasheet retrieved 20090817 - ​http://www.specim.fi/products/aisa-airborne-hyperspectral-systems/aisa-series.html
Pixel size	30 micrometers (unbinned)
IFOV	0.075 degrees (from manufacturer datasheet retrieved 20090817 - ​http://www.specim.fi/products/aisa-airborne-hyperspectral-systems/aisa-series.html

The smile and keystone are <5 microns, according to the datasheet.

Note that the field of view and focal length parameters are not measured but are quoted from specifications or mathematically calculated by the manufacturer, so there will be some error.

Bad pixels

Jukka @ Specim sent email (25/July/2008) detailing some properties of the Hawk sensor. A summary is:

• the detector is a mercury cadmium telluride (MCT) sensor
  • this is sealed in a vacuum, which may gradually leak and increasingly cause more bad pixels to appear
  • the leaking process takes 6 months to several years according to the manufacturer, and the sensor can be restored by a factory process (at Specim?)
  • if we see an increase in bad pixels, we may wish to have the instrument serviced, but recalibrations will save some of the pixels anyway
• bad pixel specification: "if the pixel peak responsivity differs more than +/- 30% from average responsivity, it is considered to be bad. According to specification less than 2% of pixels should be bad. In practice that is from 0.3 to 1.0 %."