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GEOSTATIONARY METEOROLOGICAL SATELLITE - VIS/IR IMAGERY (MCIDAS FORMAT)C. Velden (University of Wisconsin, USA)Announced availability: 1 October 1994 Data AccessThe Bureau of Meteorology (BoM)/Wisconsin reprocessed Geostationary Meteorological Satellite (GMS) images are available from the National Center for Atmospheric Research (NCAR) in Boulder, CO (http://dss.ucar.edu/datasets/ds745.0/). Also available from NCAR are the data originally identified as 'missing' (see Appendix 2, below), in preprocessed form. The BoM/Wisconsin reprocessed data have also been archived at NOAA's National Climatic Data Center (NCDC) in Asheville, NC (http://www.ncdc.noaa.gov).
BackgroundGMS-4 is a Japanese satellite in geostationary orbit over the equator at approximately 140E. The satellite is equipped with the Visible and Infrared Spin Scan Radiometer (VISSR) imaging sensor, which uses the spin motion of the satellite to scan the earth in the East-West direction. GMS begins a North-South scan every hour on the half hour, with four additional scans daily for wind estimation. At the satellite subpoint, the visible (0.5-0.75 um) channel has a resolution of 1.25 km and the infrared (10.5-12.5 um) channel has a resolution of 5 km. This gives approximately 10,000 visible and 2,500 infrared lines and samples for each full-globe image. The visible channel is digitized at 6 bits and the infrared channel at 8 bits. The S-VISSR telemetry is transmitted digitally at 1.7 GHz with a bit rate of 660 kbps. Detailed documentation on the GMS satellite and the VISSR can be found in the GMS User's Guide.GMS satellite data were obtained from the Australian Bureau of Meteorology (BoM, Melbourne) for the entire TOGA COARE Intensive Observing Period (IOP) from 1 November 1992 to 28 February 1993. Data were reprocessed in McIDAS-X file format by the University of Wisconsin.
Data File InformationThe data include 5-km full-disk IR and 1.25-km (full resolution) visible imagery over the 15 N-15 S domain at hourly intervals. The images have been carefully checked and renavigated when necessary. Eighty-two percent of all the hourly images for this period have been recovered. Other images were either missing or corrupted in the BoM dataset.A software package, called MERLIN, available through the University of Wisconsin, allows basic functions of the McIDAS software. A "TOGA COARE" subroutine added to the standard MERLIN package allows conversion of McIDAS files to raster-type files for more general use. For information on MERLIN, see Appendix.
For more information, please contact:
Chris Velden
email:chrisv@ssecmail.ssec.wisc.edu
Appendices1. MERLIN SOFTWAREMERLIN and the "TOGA COARE" Sidecar are available for distribution via http://www.ssec.wisc.edu/software/ams94.htmlBelow is a copy of the readme file that is included in the FTP directory. The package will work on HP, IBM, SGI and SUN.
Title: This software is the property of the University of Wisconsin-Madison, Space Science and Engineering Center (SSEC). It is intended for the free use of the scientific community. It is not to be decompiled or remarketed or sold without the express written permission of the SSEC.
Purpose:
Developer:
System Requirements:
HP/Apollo 9000 series 700
IBM RISC System/6000
SGI
Sun SPARC Or:
Operating System Solaris version 2.3
Installation: After you obtain the MERLIN package, use the three steps below to install it on your workstation. The MERLIN package contains the following files: merlin1.0.tar.Z, merlin1.0.sh and merlin1.0.readme. MERLIN is distributed in binary form. 1. Change the file permissions of the installation script. Type:
Additional data is available on the Internet via anonymous FTP to pathfinder.arc.nasa.gov (128.102.128.10), the Pathfinder Vernal Equinox Sampler. Data located in the /pub/GOES.ssec.wisc and /pub/SSMI.AntennaTemps.msfc directories can also be used with MERLIN. Other Pathfinder data types will be supported in the future. Data is also available on the University of Wisconsin-Madison SSEC Gopher. 2. GMS IMAGERY INVENTORYThe following GMS data are missing in the U. of Wisconsin/BoM/Taiwan GMS imagery collection. (April 1997 UPDATE: Tetsuo Nakazawa has provided data, now archived at NCAR in their original format, which fill some of these gaps.)The number in the brackets after the time means as follows.
2: both northern and southern data available
1: only northern data available
0: entire data missing
Missing IR DATA
Julian Day Calendar date Time Missing
305 31 Oct 0330(1), 0730(2)
306 1 Nov 0330(1)
307 2 Nov 0330(1)
308 3 Nov 0330(1), 1130(2), 1430(2),
1530(2), 1630(2)
309 4 Nov 0130(2), 0330(1)
310 5 Nov 0330(1), 0430(2)
311 6 Nov 0330(1)
312 7 Nov 0330(1)
315 10 Nov 0030(0), 0130(0)
316 11 Nov 0030(0), 0130(0), 0230(2)
319 14 Nov 0330(1)
320 15 Nov 0230(2), 0330(1)
321 16 Nov 0330(1)
322 17 Nov 0330(1)
323 18 Nov 0330(1)
324 19 Nov 0330(1)
325 20 Nov 0330(1)
326 21 Nov 0330(1)
327 22 Nov 0330(1)
328 23 Nov 0330(1)
329 24 Nov 0330(1)
330 25 Nov 0330(1)
331 26 Nov 0330(1)
332 27 Nov 0330(1)
333 28 Nov 0330(1)
334 29 Nov 0330(1)
335 30 Nov 0330(1)
337 2 Dec 0130(1)
339 4 Dec 0030(0), 0130(0), 0230(0),
0330(0), 0430(0)
342 7 Dec 0130(1)
343 8 Dec 0030(0), 0130(0), 2130(2)
349 14 Dec 0130(1)
350 15 Dec 0030(0), 0130(0), 0230(0),
0330(0), 0430(0)
355 20 Dec 0730(2)
356 21 Dec 0030(0), 0130(0)
361 26 Dec 0630(2), 2330(2)
362 27 Dec 0030(2), 0530(2), 0830(2)
2 2 Jan 0330(2)
6 6 Jan 0030(0), 0130(0), 0230(0),
0330(0)
7 7 Jan 0030(0), 0130(0), 0230(0),
0330(0), 0830(2)
8 8 Jan 0130(0), 0230(0), 0330(0),
0430(0)
11 11 Jan 0030(0), 0230(2), 0430(2),
0530(2), 0730(2),
0930(2),1130(2), 1330(2), 1530(2), 1630(2),
1730(2), 1930(2), 2130(2), 2230(2)
12 12 Jan 0030(2), 0230(0), 0330(0),
0530(2), 0730(2),
0930(2), 1130(2), 1330(2), 2030(2), 2230(2)
13 13 Jan 0030(2), 0130(2), 0230(2),
0330(2), 0430(2),
0530(2), 0630(2), 0730(2), 0930(2), 1030(2),
1130(2), 1330(2), 1730(2), 1930(2), 2030(2),
2230(2), 2330(2)
14 14 Jan 0030(2), 0130(2), 0230(2),
0430(2), 0630(2),
1030(2), 1130(2), 1330(2), 1830(2), 2330(2)
15 15 Jan 0030(2), 0330(2), 0730(2),
0930(2), 1530(2),
1830(2), 2030(2), 2330(2)
16 16 Jan 0330(2), 0530(2), 0730(2),
1630(2), 2330(2)
17 17 Jan 0830(2), 1330(2), 1730(2),
2130(2), 2330(2)
18 18 Jan 1330(2)
19 19 Jan 0030(0), 0130(0), 0230(0),
0330(0)
21 21 Jan 1130(2)
22 22 Jan 0030(2), 0130(2)
23 23 Jan 0030(2), 0130(2), 0830(2),
2130(2)
24 24 Jan 0430(2), 1030(2), 1930(2),
2030(2), 2130(2)
25 25 Jan 0230(2), 0330(2), 0730(2),
26 26 Jan 0330(2), 0930(2), 1030(2)
27 27 Jan 0030(2), 0130(2), 0230(2),
0430(2), 0630(2),
0830(2), 1330(2)
29 29 Jan 0330(2)
30 30 Jan 1130(2), 1530(2), 1630(2),
2030(2)
31 31 Jan 1230(2), 1330(2), 1430(2)
32 1 Feb 0630(2)
41 10 Feb 0130(0), 1130(2)
42 11 Feb 0530(2)
43 12 Feb 0130(0), 1130(2)
45 14 Feb 1630(2)
46 15 Feb 0130(0), 0430(2), 1330(2),
2330(2)
47 16 Feb 0030(0), 0130(0),
48 17 Feb 1630(2)
49 18 Feb 0030(0), 0330(0), 0530(2)
50 19 Feb 0130(2)
51 20 Feb 0530(2)
52 21 Feb 0530(2)
53 22 Feb 0030(0), 0330(0)
54 23 Feb 0130(1)
55 24 Feb 1730(2)
56 25 Feb 0030(2), 0130(0), 0330(2),
0430(2), 0630(0),
0730(2), 0930(2), 1130(2), 1330(0), 1430(0),
1530(2), 1630(2)
57 26 Feb 1330(0), 1430(0)
58 27 Feb 0030(2), 1330(0), 1430(0)
59 28 Feb 1330(0), 1430(0)
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