Advanced Microwave Precipitation Radar (AMPR)
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Data Access |
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(this document is based on the readme document available at NASA/Marshall's Global Hydrology web page: http://ghrc.msfc.nasa.gov/uso/readme/ampr.html
The Advanced Microwave Precipitation Radar (AMPR) data sets of Texas & Florida Underflights field experiments (TEFLUN A & B) are part of the aircraft based measurements collected in support of the TRMM ground validation efforts.AMPR instrument was flown on the NASA ER-2 aircraft over Texas from April 9 through May 6, 1998 for the TEFLUN-A experiment and over Florida from August5 through September 27, 1998 for the TEFLUN-B & CAMEX-3 field campaigns.
AMPR is a cross-track scanning total power microwave radiometer with four channels centered at 10.7, 19.35, 37.1 and 85.5 GHz. The AMPR measurements were made under the direction of the NASA/GSFC scientists Ms. Robbie Hood (Principal Investigator) and Mr.Frank LaFontaine(co-investigator). The calibrated brightness temperatures are used for the validation of TRMM TMI brightness temperatures and rain algorithms.
The TEFLUN-A data sets are archived at the Goddard Data and Information Services Center (DISC).
Sponsor
The distribution of these data sets is funded by NASA's Earth Science Enterprise. The data are not copyrighted; however, we request that when you publish data or results using these data, please acknowledge as follows:The authors wish to thank Ms. Robbie Hood and Mr.Frank LaFontaine (NASA/Marshall Space Flight Center) for the production of this AMPR data set. They also thank the Data and Information Services Center (Code 610.2) at the Goddard Space Flight Center, Greenbelt, MD, 20771, for making it available to the scientific community. Goddard's contribution to the distribution and archive of this data set was sponsored by NASA's Earth Science Enterprise.
Characteristics
The data is very preliminary, before using this data in your publication, please contact the Principal Investigator Ms.Robbie Hood .
TEFLUN-A AMPR data
Flight Date (UTC) Start-stop time UTC # 15 minute Images 5 Apr 98 1600 - 1730 6 9 Apr 98 1615 - 2000 15 15 Apr 98 0100 - 0245 7 18 Apr 98 1700 - 2045 15 21 Apr 98 0415 - 0800 15 23 Apr 98 0315 - 0500 7 27 Apr 98 0000 - 0315 13 1 May 98 0030 - 0415 15 4 May 98 2115 - 0300 13 6 May 98 1845 - 2315 18 Files Format
Data are available in binary format and each file represents one flight. The native (binary) file type is labeled "Extended Package" [EP] and filenames have this abbreviation within them. The information file associated with the data files named READ_ME_AMPR_archive.txt is provided in the ampr directory at the FTP site.
File Naming Convention
The file naming convention for AMPR data (adopted by GHRC)is:
where:
- ampr_CAMEX-3_98124_R8ntb_EPc27May99.sys
The EP (extended package) record structure is as shown in the following table. A value of -32768 is a flag indicating that the data are not useable and a value of -22222 is a flag which indicates the data calculation(s) were not executable.
- ampr = instrument name
- CAMEX-3 = experiment acronym
- 98124 = launch date (yyddd)
- R8ntb = High precision navigated brightness temperatures
- EP = Extended Package data set type
- c06Oct98 = creation date
- .sys = binary data (.sys = SGI system format option)
Data Format
Sequence Format Vals Data type Units 1 Integer*2 1 Scan number 2 Integer*2 1 Year UTC 3 Integer*2 1 Day-of-year UTC 4 Integer*2 1 Hour UTC 5 Integer*2 1 Minute UTC 6 Integer*2 1 Second UTC 7 Integer*2 1 GPS validity code 1=good 8 real*8 1 GPS Altitude meters 9 real*8 1 GPS Latitude degrees 10 real*8 1 GPS Longitude degrees 11 real*8 1 Heading (0, 360=North, clockwise) degrees 12 real*8 1 Pitch (+ is nose up) degrees 13 real*8 1 Roll (+ is right wing down) degrees 14 real*8 1 Ground Speed m/s 15 real*8 1 Air Speed m/s 16 real*8 1 Barometric Altitude meters 17 real*8 1 INS Latitude degrees 18 real*8 1 INS Longitude degrees 19-22 real*8 4 RMS noise (10, 19, 37, 85 GHz) Kelvin 23-72 real*8 50 Pixel TB's at 10.7 GHz Kelvin 73-122 real*8 50 Pixel TB's at 19.35 GHz Kelvin 123-172 real*8 50 Pixel TB's at 37.1 GHz Kelvin 173-222 real*8 50 Pixel TB's at 85.5 GHz Kelvin 223-272 real*8 50 Pixel Latitude degrees 273-322 real*8 50 Pixel Longitudes degrees Companion Software
A FORTRAN read program read_ampr_EPdata.f is provided by the data producers as an example of how to read a binary AMPR data file on a UNIX system. Source code for this FORTRAN program is available in the document directory in the anonymous FTP area.
The source code of the FORTRAN program (read_ampr_EPdata.f) (which includes an example for use in extracting AMPR data from the EP binary file) is also given below.
=============== beginning of source code ===========
program read_ampr_EPdata c c Data reader for the *R8ntb_EP* type of public AMPR data. c Frank LaFontaine (Raytheon ITSS) Sep 98 --- New. c implicit real*8 (a-h,o-z), integer*4 (i-n) parameter maxrec=10000 logical exist, done character file_format*12, file_name*80 integer*4 iscan(maxrec), itime(5,maxrec), igps(maxrec) real*8 rmsN(4,maxrec), er2nav(11,maxrec), tbs10(50,maxrec), tbs19(50,maxrec), tbs37(50,maxrec), tbs85(50,maxrec), xlat(50,maxrec), xlon(50,maxrec) c Get command input. if (iargc() .eq. 2) then call getarg (1, file_format) call getarg (2, file_name) else print* print*,' Usage: read_ampr_EPdata file_format file_name' print* print*,' file_format: formatted, system, '// 'unformatted, or binary' print* print*,' file_name: enter the AMPR "EP" file name' print* stop endif c Check for input file existance. inquire (file=file_name, exist=exist) if (.not. exist) then print* print*,' Invalid input file name: ',file_name print* stop ' ' endif c Open and read all the data from the file. open (11, file=file_name, form=file_format, readonly) i = 0 done = .false. do while (.not. done) i = i + 1 if (file_format .eq. 'formatted') then read (11, 1100, err=101, end=101) iscan(i), (itime(j,i), j=1,5), igps(i), (er2nav(j,i), j=1,11), (rmsN(j,i), j=1,4), (tbs10(j,i), j=1,50), (tbs19(j,i), j=1,50), (tbs37(j,i), j=1,50), (tbs85(j,i), j=1,50), (xlat(j,i), j=1,50), (xlon(j,i), j=1,50) else read (11, err=101, end=101) iscan(i), (itime(j,i), j=1,5), igps(i), (er2nav(j,i), j=1,11), (rmsN(j,i), j=1,4), (tbs10(j,i), j=1,50), (tbs19(j,i), j=1,50), (tbs37(j,i), j=1,50), (tbs85(j,i), j=1,50), (xlat(j,i), j=1,50), (xlon(j,i), j=1,50) endif enddo 1100 format ( 6i8, i8,f10.2,2f14.6,5f12.4,f10.2,2f14.6, 4f12.4, 200f12.4, 100f14.6) 101 continue nscans = i - 1 close (11) print* print*,'All data read...' print* c FOR EXAMPLE: c Print to the screen the scan#, date, time, and element 25 of each c frequency, with latitude and longitude at that point. Pause every 100 scans. do i= 1, nscans write (6, 6001) iscan(i), (itime(j,i), j=1,5), tbs10(25,i), tbs19(25,i), tbs37(25,i), tbs85(25,i), xlat(25,i), xlon(25,i) if (mod(i,100) .eq. 0) pause enddo 6001 format ('Scan: ',i4,2x,'Date: ',i4,i3,2x, 'Time(UTC): ',i2,':',i2,':',i2,3x,'Tb10: ',f6.2,2x, 'Tb19: ',f6.2,2x,'Tb37: ',f6.2,2x,'Tb85: ',f6.2,3x, 'Lat: ',f9.5,2x,'Lon: ',f10.5) print* print*,' ******* read_ampr_EPdata is done *******' stop end=================== End of source code==========
Data Access and Contacts
Data Access
FTP Site
The TEFLUN aircraft data resides on DISC anonymous FTP. You may access the files from this document,AMPR Calibrated Brightness Temperatures(Binary files)
AMPR Browse Images
- or directly via FTP at
- ftp disc2.nascom.nasa.gov
- login: anonymous
- password: < your internet address >
- cd data/TEFLUNA/aircraft/nasa_er2/ampr
Points of Contact
For Information about TEFLUN data at Goddard DISC, please contactHydrology Data Support Team
NASA Goddard Space Flight Center
Greenbelt, MD 20771
email: hydrology@disc.gsfc.nasa.govTechnical Inquiries about this Data should be addressed to:
Principal Investigator:
Ms. Robbie Hood
Global Hydrology and Climate Center
977 Explorer Blvd.
Huntsville, Alabama 35806
Phone: 256-922-5959
Fax: 256-922-5723
E-mail: robbie.hood@msfc.nasa.govor
Co-investigator:
Mr. Frank LaFontaine
Global Hydrology and Climate Center
977 Explorer Blvd.
Huntsville, Alabama 35806
Phone: 256-922-5796
Fax: 256-922-5723
E-mail: frank.lafontaine@msfc.nasa.gov
Instrument Characteristics
The AMPR is a total power scanning multifrequency passive radiometer which collects data at 10.7, 19.35, 37.1, and 85.5 GHz. The AMPR radiometer is designed to fly on a NASA ER-2 high altitude aircraft which has an approximate cruising altitude of 20 km.The radiometer and accompanying data system are mounted behind the cockpit in the Q-bay section of the fuselage. The radiometer is positioned in the lower Q-bay with the scanning mirror extending below the body of the aircraft into a hatch with a porthole open to the ambient atmosphere. The data system is mounted above the radiometer in the upper Q-bay section.
The ground spatial resolution of the nadir footprint from the nominal aircraft altitude of 20 km is 0.6 km for the 85.5 GHz channel, 1.5 km for 37.1 GHz, and 2.8 km for both the 19.35 and 10.7 channels The AMPR calibrates with external cold and warm loads after every fourth data scan. A total calibration sequence or a total data scan are each performed in a three second time period.
The AMPR scanner sweeps through a total 90o (+/- 45o from nadir) data scan collecting a sample for each channel every 1.8o for a total of 50 samples per channel. Based upon an aircraft altitude of 20 km and an aircraft speed of 200 ms-1, this scan rate will yield contiguous footprints for the 85.5 GHz channel within a 40 km wide swath. The other three channels will be oversampled by the factors given in the Table given below which also lists other performance characteristics of the radiometer. The alignment of the feedhorns has been adjusted such that vertical polarization is received 45o to the left of nadir and horizontal is received 45o to the right of nadir. An equal mixture of vertical and horizontal polarizations is received at nadir.
The following table lists several of the AMPR performance characteristics:
AMPR Performance Characteristics
Characteristic 85.5GHz 37.1GHz 19.35GHz 10.7GHz Bandwidth (MHz) 1400 900 240 100 Integration Time (ms) 50 50 50 50 Horn Type SSM/I SSM/I SSM/I GTRI Lens Diameter (inches) 5.3 5.3 5.3 9.7 Beam width (degrees) 1.8 4.2 8.0 8.0 Footprint (km) [@20 km ER-2 alt. 500kts] 0.64 1.48 2.78 2.78 Beam Efficiency (%) N/A 98.8 98.7 97.8 Cross Polarization (%) N/A 0.4 1.6 0.2 Algorithm & Calibration Issues
The data has been calibrated, and while they are useful for many research purposes, the brightness temperatures are not yet fully quality assured. The final revised dataset processed with better calibration coefficients will be made available as soon as it it is made available by AMPR data producers.
Some AMPR flight data are missing navigation information that is normally generated by the AMPR instrument. These datasets without navigation may be recoverable at some time in the future using navigation data provided by auxillary navigation systems.
Spencer, R.W., Hood, R.E., LaFontaine, F.J., Smith, E.A., Platt, R., Galliano, J., Griffin, V.L., and E. Lobl, 1994: High Resolution Imaging of Rain Systems with the Advanced Microwave Precipitation Radiometer, Journal of Atmospheric and Oceanic Technology, Vol. 11, No. 4, pp.849-857.
Hood, R.E., Spencer, R.W., LaFontaine, F.J., and E.A. Smith, 1994: Simulation of Future Microwave Satellite Instruments Using High Resolution AMPR Aircraft Data, Preprints: Seventh Conference on Satellite Meteorology and Oceanography, Section 3.10, pp.160-163, American Meteorological Society, 6-10 June 1994, Monterrey, CA.
Smith, E.A., Xiang, X., Mugnai, A., Hood, R.E., and R.W. Spencer, 1994: Behavior of an Inversion-based Precipitation Retrieval Algorithm with High Resolution AMPR Measurements Including a Low Frequency 10.7 GHz Channel, Journal of Atmospheric and Oceanic Technology, Vol. 11, No. 4, pp.857-.
Turk, J., Vivekanandan, J., Marzano, F.S., Hood, R.E., Spencer, R.W., and F.J. LaFontaine, 1994: Active and Passive Microwave Remote Sensing of Precipitating Storms During CaPE. Part I: Advanced Microwave Precipitation Radiometer and Polarimetric Radar Measurements and Models, Meteorology and Atmospheric Physics, Special Issue on Retrieval of Hydrological Variables from Space-based Microwave Instruments, Volume 54, pp.3-27.
Marzano, J., Mugnai, A., Smith, E.A., Xiang, X., Turk, J., and J. Vivekanandan, 1994: Active and Passive Microwave Remote Sensing of Precipitating Storms During CaPE. Part II: Intercomparison of Precipitation Retrievals Over Land from AMPR Radiometer and CP-2 Radar, Meteorology and Atmospheric Physics, Special Issue on Retrieval of Hydrological Variables from Space-based Microwave Instruments, Volume 54, pp.29-51.
Evans, K.F., Turk, J., Wong, T., and G.L. Stephens, 1995: A Bayesein Approach to Microwave Precipitation Profile Retrieval, Journal of Applied Meteorology, Volume 34, Number 1, pp.260-279.
Griffin, V. L., A.R. Guillory, M. Susko, and J. E. Arnold, Operations Summary for the Convection and Moisture Experiment (CAMEX), NASA Technical Memorandum, NASA TM-108445, March 1994.
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