MTSAT Australia Winds IR Satellite Imagery

This dataset contains Australia winds IR imagery from the MTSAT satellite taken during the HIPPO-4 project. The imagery are in GIF format. The imagery cover the time span from 2011-06-08 18:00:00 to 2011-07-13 15:00:00.

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  • EOL Data Support
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    UCAR/NCAR - Earth Observing Laboratory

Temporal Range

  • Begin:  2011-06-08T18:00:00Z
    End:  2011-07-13T17:59:59Z

Keywords

Resource Type dataset
Temporal Range Begin 2011-06-08T18:00:00Z
Temporal Range End 2011-07-13T17:59:59Z
Temporal Resolution N/A
Bounding Box North Lat 0.00000
Bounding Box South Lat -50.00000
Bounding Box West Long 120.00000
Bounding Box East Long 180.00000
Spatial Representation N/A
Spatial Resolution N/A
Related Links N/A
Additional Information N/A
Resource Format GIF: Graphics Interchange Format (GIF) (image/gif)
Standardized Resource Format Image
Asset Size 94 MB
Legal Constraints

none


Access Constraints none
Software Implementation Language N/A

Resource Support Name EOL Data Support
Resource Support Email datahelp@eol.ucar.edu
Resource Support Organization UCAR/NCAR - Earth Observing Laboratory
Distributor UCAR/NCAR - Earth Observing Laboratory
Metadata Contact Name EOL Data Support
Metadata Contact Email datahelp@eol.ucar.edu
Metadata Contact Organization UCAR/NCAR - Earth Observing Laboratory

Author Cooperative Institute for Meteorological Satellite Studies (CIMSS)
Publisher UCAR/NCAR - Earth Observing Laboratory
Publication Date 2013-03-18T20:44:08
Digital Object Identifier (DOI) https://doi.org/10.26023/KAZB-7156-SB07
Alternate Identifier 248.068
Resource Version 1.0
Topic Category climatologyMeteorologyAtmosphere
Progress completed
Metadata Date 2024-12-26T23:48:18Z
Metadata Record Identifier edu.ucar.eol::248.068
Metadata Language eng; USA
Suggested Citation Cooperative Institute for Meteorological Satellite Studies (CIMSS). (2013). MTSAT Australia Winds IR Satellite Imagery. 1.0. UCAR/NCAR - Earth Observing Laboratory. https://doi.org/10.26023/KAZB-7156-SB07. Accessed 28 December 2024.

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