McIDAS Learning Guide
Version 2006
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SSEC receives satellite images from geostationary and polar orbiting satellites. Geostationary satellites remain above a fixed location on the earth's surface, appoximately 35,800 km above the equator. Because the satellites rotate with the earth, they always observe the same portion of the globe. Currently, there are geostationary satellites from the United States, the European Organisation for the Exploitation of Meteorological Satellites (EUMETSAT), and the Japan Meteorological Agency (JMA).
The United States has a satellite called GOES-East, which monitors North and South America and the western Atlantic Ocean, and one called GOES-West, which monitors North and South America and the eastern Pacific Ocean. EUMETSAT has two satellites (METEOSAT) which monitor Europe, Africa, Asia, the Indian Ocean, and the Atlantic Ocean. JMA has a satellite (MTSAT) which monitors eastern Asia, Australia, the western Pacific Ocean and the eastern Indian Ocean.
Roll your mouse over the image below to see the coverage of each geostationary satellite:
Polar orbiting satellites orbit at much lower altitudes (800-900 km). Their path is 2,400 km wide centered at the orbit path. With each orbit, the satellites observe a new path. Currently, SSEC ingests four POES satellites, NOAA-15, NOAA-16, NOAA-17, and NOAA-18. SSEC also ingests the Aqua and Terra satellites.
See the SSEC Data Center's website for a list of all current and archived satellite data available from SSEC.
IMGLIST GV4.1 FORM=ALL Image file directory listing for:GV4 Pos Satellite/ Date Time Center Res (km) Image_Size sensor Lat Lon Lat Lon --- ------------- ------------ -------- ---- ---- ----- ----- ------------ 1 GOES-7 13 MAR 93072 17:01:00 26 87 Band: 1 0.65 um Daytime cloud detection 4.39 3.64 1335 x 1608 proj: 0 created: 1993208 191703 memo: AAA-MSI TO VIS VIA ARCHIVE type:VISR cal type:BRIT offsets: data= 768 navigation= 256 calibration= 0 auxiliary= 0 doc length: 0 cal length: 0 lev length: 0 PREFIX= 4 valcod: 1104210435 zcor: 1 avg-smp: A start yyddd: 1993072 start time:170105 start scan: 56 lcor: 1121 ecor: 7585 bytes per pixel: 1 ss: 32 Resolution Factors (base=1): Line= 4.0 Element= 4.0 IMGLIST: done |
Areas use the naming convention AREAnnnn where nnnn is the four digit area number. For example, AREA0003 is the name of the file that contains area 3. Most of the older McIDAS commands use only the area number. However, you must use the AREA prefix with the DMAP command or when using Unix commands to copy, move, or delete areas.
In ADDE, sequences of AREA files are grouped together in a dataset. For example, in a previous lesson, you created the dataset MYDATA/IMAGES, which contains the AREA file numbers from 1 to 9999. Individual AREA files can be accessed with their position number within the dataset. In the case of MYDATA/IMAGES, position 3 (MYDATA/IMAGES.3) would relate to the file AREA0003. However, in the dataset MYDATA/TEST-IMAGES that was created in the previous lesson, the dataset defined the AREA files ranging from 4000 to 4004, so position 3 (MYDATA/TEST-IMAGES.3) would be AREA4002. (This would be equivalent to MYDATA/IMAGES.4002)
Navigation, as applied to satellite imagery, means the conversion between satellite image coordinates (line and element) and earth coordinates (latitude and longitude). This is usually done when the data is ingested.
If a displayed image sector is navigated, McIDAS can convert the image coordinates of a specified pixel to earth coordinates. The E command lists the earth, TV and image coordinates at the cursor center.
Image resolution is measured in kilometers and is highest at the subsatellite point. The highest available resolution depends on the satellite and image type:
Satellite Visible Infrared GOES 1 km 4 km METEOSAT 2.5 km 5 km MODIS 0.25 km 1 km MSG 1 km 3 km
MTSAT (HiRID format) 1.25 km 5 km POES 1 km 1 km
This means that a single GOES infrared pixel at the subsatellite point represents a 4km x 4km square on the earth's surface, and a single METEOSAT visible pixel at the subsatellite point represents a 2.5km x 2.5km square on the earth's surface, etc. The further a pixel is located from the subsatellite point, the lower its resolution.
You can display imagery at a resolution other than that stored in the area. Specifying a positive magnification factor in McIDAS commands (e.g., IMGDISP) enlarges or blows up the data by replicating pixel values; a negative magnification factor produces a blow down by sampling pixel values. For example, if you choose a magnification factor of 16, the value of each pixel in the area is duplicated 256 times (in a 16 x 16 box of pixels) when displayed on the frame. If you choose a magnification factor of -4, the value of every fourth element along every fourth line is displayed as one pixel on the image frame.
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