Hyperspectral Imager for the Coastal Ocean

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Hyperspectral Imager for the Coastal Ocean (HICO) on the International Space Station. Hyperspectral Imager for the Coastal Ocean (HICO) on International Space Station.jpg
Hyperspectral Imager for the Coastal Ocean (HICO) on the International Space Station.

The Hyperspectral Imager for the Coastal Ocean (HICO) was a hyperspectral earth observation sensor that operated on the International Space Station (ISS) from 2009 to 2014. HICO collected hyperspectral satellite imagery of the Earth's surface from the ISS. [1] [2] [3]

Contents

HICO was a pathfinder or proof-of-concept mission for hyperspectral imaging of the oceans, particularly for optically complex coastal waters. [4] The dataset collected by HICO serves as an example dataset for future hyperspectral satellite missions such as PACE.

HICO was mounted directly on the ISS rather than on a separate unmanned satellite platform (i.e., distinct from the MODIS sensor mounted on Aqua and Terra satellites and from SeaWiFS mounted on OrbView-2 aka Seastar satellite). As such, HICO was tasked to collect images of certain regions in sync with the daytime orbit path of the ISS. Further, its data record may contain some gaps in time for operational tasks on board the ISS such as spacewalks and docking.

History

HICO was developed by the United States Office of Naval Research. The sensor was launched on September 10, 2009, from the Tanegashima Space Center in Japan as payload for the ISS on the H-2B-304 rocket (including HTV-1 transfer vehicle). It was installed on September 24, 2009, onto the Japanese Experiment Module Exposed Facility of the Kibo Laboratory (Japanese Kibo complex) of the ISS by two Expedition-20 engineers, ESA astronaut Frank De Winne and NASA astronaut Nicole Stott. HICO was installed concurrently with the RAIDS/Remote Atmospheric and Ionospheric Detection System: together these two systems are referred to as the “HICO and RAIDS Experiment Payload (HREP or HREP-RAIDS).” [5] HICO Collected over 10,000 images during its operating lifetime. [3] Financial support came from the United States Office of Naval Research, the United States Department of Defense, and later from the International Space Station Program.

In summer 2013 HICO data became publicly available [6] and remain freely accessible today.

HICO stopped collecting data in September 2014 when radiation from a solar flare damaged its computer. Attempts to restart the computer were unsuccessful. [7] The last image date and official end of operations was September 13, 2014.

After the end of its lifetime, HICO and RAIDS Experiment Payload (HREP) was removed from the ISS on August 3, 2018, on the SpaceX CRS-15 Dragon space capsule after its July–August 2018 resupply mission. The Dragon's trunk section burned up during re-entry, disposing of the HICO instrument and other contents. The flight that offloaded HICO was the fourth ever round-trip cargo flight with a reused Dragon capsule. [8]

Technical specifications and data products

Hyperspectral imagery (right) uses more spectral bands or more colors of light, providing more information to identify different types of terrain. Mono, Multi and Hyperspectral Cube and corresponding Spectral Signatures modified.svg
Hyperspectral imagery (right) uses more spectral bands or more colors of light, providing more information to identify different types of terrain.
Hyperspectral satellite sensors(right) detect light radiating from Earth's surface over the full spectrum of visible light, rather than at a few specific "bands" like RGB or multispectral sensors (left and middle). Spectral sampling RGB multispectral hyperspectral imaging.svg
Hyperspectral satellite sensors(right) detect light radiating from Earth's surface over the full spectrum of visible light, rather than at a few specific "bands" like RGB or multispectral sensors (left and middle).

Spectral coverage and resolution

HICO uses 128 spectral bands from approximately 353 nm to 1080 nm wavelengths at 5.7 nm spectral resolution (band centers 5.7 nm apart). [3] Data from wavelengths less than 400 nm and greater than 900 nm are not recommended for analysis; 400-900 nm data are higher quality. A 10 nm smoothing filter is applied to wavelengths 400 to 745 nm and a 20 nm filter is applies to wavelengths 746 to 900 nm. [9]

Spatial coverage and resolution

HICO pixels are approximately 90 meters in spatial resolution. Each full scene covers approximately a 42 by 192 km rectangle (varying with altitude and angle). High latitude regions of the Earth are not covered. The ISS accomplishes about sixteen 90-minute orbits per day, and the location of the track for orbit moves to the west as Earth rotates. The ISS orbit tracks over the same area on the ground about every three days, including nighttime overpasses. [10] However, HICO imaging was limited to collect only one scene per orbit, resulting in about seven to eight daylight scenes per day, often spatially scattered throughout the world.

Radiometric resolution

HICO data have a signal-to-noise ratio of greater than 200-to-1 for water-penetrating wavelengths and assuming 5% albedo. The sensor had high sensitivity in the blue wavelengths and full coverage of water-penetrating wavelengths. [11]

Temporal coverage and resolution

HICO collected satellite imagery from September 25, 2009, to September 13, 2014. [12] A maximum of eight daylight scenes were collected per day. In any specific coastal region where scenes were imaged, temporal resolution is patchy. For example, over Chesapeake Bay on the United States east coast, 101 scenes were collected over the entire 5-year mission, and 16 scenes were imaged during the calendar year 2012.

Data products

HICO datasets, like other hyperspectral satellite datasets, are large in terms of data volume. For example, one HICO scene requires 120 MB to 700 MB of disk space (depending on format and compression). Data are available from NASA Ocean Color Web in HDF file format (similar to netCDF). [9]

Similar sensors

Other hyperspectral satellite sensors

(partial list)

Other Earth science instruments on the ISS

(partial list)

Applications

See also

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References

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  7. ↑ Kelly, Nina Maggi (23 March 2015). "Satellites can be vulnerable to solar storms". IGIS Informatics and GIS. Agriculture and Natural Resources, University of California. Retrieved 22 September 2021.
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  21. ↑ O'Shea, Ryan E.; Pahlevan, Nima; Smith, Brandon; Bresciani, Mariano; Egerton, Todd; Giardino, Claudia; Li, Lin; Moore, Tim; Ruiz-Verdu, Antonio; Ruberg, Steve; Simis, Stefan G.H.; Stumpf, Richard; Vaičiūtė, Diana (2021). "Advancing cyanobacteria biomass estimation from hyperspectral observations: Demonstrations with HICO and PRISMA imagery". Remote Sensing of Environment. 266. Elsevier BV: 112693. Bibcode:2021RSEnv.26612693O. doi: 10.1016/j.rse.2021.112693 . hdl: 1805/31613 . ISSN   0034-4257.
  22. ↑ Kudela, Raphael M.; Palacios, Sherry L.; Austerberry, David C.; Accorsi, Emma K.; Guild, Liane S.; Torres-Perez, Juan (2015). "Application of hyperspectral remote sensing to cyanobacterial blooms in inland waters". Remote Sensing of Environment. 167. Elsevier BV: 196–205. Bibcode:2015RSEnv.167..196K. doi: 10.1016/j.rse.2015.01.025 . ISSN   0034-4257.
  23. ↑ Dierssen, Heidi; McManus, George B.; Chlus, Adam; Qiu, Dajun; Gao, Bo-Cai; Lin, Senjie (16 November 2015). "Space station image captures a red tide ciliate bloom at high spectral and spatial resolution". Proceedings of the National Academy of Sciences. 112 (48): 14783–14787. Bibcode:2015PNAS..11214783D. doi: 10.1073/pnas.1512538112 . ISSN   0027-8424. PMC   4672822 . PMID   26627232.
  24. ↑ Garcia, Rodrigo A.; Fearns, Peter R.C.S.; McKinna, Lachlan I.W. (2014). "Detecting trend and seasonal changes in bathymetry derived from HICO imagery: A case study of Shark Bay, Western Australia". Remote Sensing of Environment. 147. Elsevier BV: 186–205. Bibcode:2014RSEnv.147..186G. doi:10.1016/j.rse.2014.03.010. hdl: 20.500.11937/24033 . ISSN   0034-4257.
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