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Millimeter Imaging Radiometer (MIR) Data from TRMM LBA


Overview
Sponsor

The Data
Characteristics

The Files
Format
Naming Convention
Companion Software

Data Access & Contacts
FTP Site
Points of Contact

The Science
Instrument

References


MIR Data from TRMM LBA

Overview

MIR is an airborne cross-track scanning radiometer that provides calibrated brightness temperatures at seven different channels in the frequency range of 89-340 GHz. It is being used aboard a NASA high-altitude (20 km) ER-2 aircraft to study atmospheric water vapor, clouds, and precipitation.

The MIR measurements were made under the direction of NASA/GSFC scientists Dr. James Wang (Principal Investigator) and Dr. Paul Racette (co-investigator)and the 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 NASA scientists James Wang and Paul Racette (Goddard Space Flight Center) for the production of this MIR 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.

The Data

Characteristics

The MIR data consist of calibrated brightness temperatures in degrees Kelvin at seven channels (89, 150, 183.3±1, 183.3±3, 183.3±7, 220, and 340 GHz).

The data is preliminary. Before using MIR data in your publication, please contact the Principal Investigator Dr. James Wang (wang@sensor.gsfc.nasa.gov).

The Files

File Formats

MIR data for each flight is contained in one file. The data are in four-byte IEEE floating point words.

Each logical record of size 2316 bytes( 4 x 579)contains one calibrated MIR scan comprising temporal, spatial and aircraft attitude information for the nadir position (beam position 29) of the scan followed by a brightness temperature value for each of 57 beam positions at all 7 MIR frequencies.

Logical Record Format
wordParameterSource/UnitsGHz
1Record Number  
2MonthReal time clock (RTC) 
3DayReal time clock (RTC) 
4HourIRIG 
5MinuteIRIG 
6SecondIRIG 
7Julian DayNavigation 
8HourNavigation 
9MinuteNavigation 
10SecondNavigation 
11LatitudeDegrees 
12LongitudeDegrees (-West, +East) 
13Air TemperatureDegrees celsius 
14AltitudeFeet 
15PitchDegrees (+ for nose down) 
16RollDegrees (+ for roll right) 
17HeadingDegrees 
18- 26 HouseKeeping Temperatures   
27Hot average temperature for this scan  
28Cold average temperature for this scan  
29 Hot temperature, 8-scan moving average  
30 Cold temperature, 8-scan moving average  
31- 39Hot average counts for this scan  
40- 48Cold average counts for this scan  
49- 57 Hot counts, 8-scan moving average  
58- 66Cold counts, 8-scan moving average  
67- 12357 brightness temperatures degrees Kelvin89
124-180150
181-237183.3 ±1
238-294183.3 ±3
295-351183.3 ±7
352-408220
409-465340
466-522 
523-578 
NOTE: The last 2 words in the record are zero-filled

File Naming Convention

The file naming convention for TRMM LBA MIR data is:
                OUT.yyddd.MIR
 where:
              yy = year
             ddd = day of year 
             MIR = instrument name

Example: File for 23 January, 1999              
                OUT99023.MIR

Companion Software

The MIR dataset was generated using a personal computer. To read it on a UNIX system requires a byte swap (see following sample read program.)

cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc
! This program reads a few records of 1998 MIR data in SGI computer
! !!!!!!!!!!!!!!!!!!!!!***  last 3 channels have zero brightness temp.

      structure /OutStruct/
      real*4   		RecNumber
      real*4   		RTCmonth, RTCDayOfMonth
      real*4   		IrigHour, IrigMin, IrigSec
      real*4   		NavJulian, NavHour,  NavMin,  NavSec
      real*4		latitude, longitude
      real*4		AirTemp, altitude, pitch, roll, heading
      real*4            HouskptTmp(9)
      real*4            HotTemp,CldTemp,HotTemp8a,CldTemp8a
      real*4            HotCnt(9) ,CldCnt(9) ,HotCnt8a(9),CldCnt8a(9)
      real*4   		BrightTemps(9,57)
      end structure

      record/OutStruct/ i
      record/OutStruct/ j

      integer   m, k
       ib=    1
       ie=11111

      open(8, file='/xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx',
     $ access='DIRECT', status='OLD', err=1999, recl=579*4)
c!!! use f77 -bytereclen !!!!

CCC   do m=   1, 11111
      do m=1,2
         read(8, rec=m, end=500, err=400) j
          call FLIP(j,i,579*4)


ccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc
       if( m.ge.ib.and.m.le.ie) then
       write(*,1)i.RecNumber,i.RTCmonth,i.RTCDayOfMonth
     @,i.IrigHour, i.IrigMin,i.IrigSec
     @  ,i.latitude,i.longitude,i.altitude ,i.pitch,i.roll,
     @i.heading,(i.BrightTemps(k,29)   ,k= 1,6)     


       endif
ccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc
      end do
      stop 'Done!'
 400  call perror('Error reading record')
      stop 3
 500  call perror('Hit EOF reading record')
      stop 4
 1999 call perror('Error opening input file!')
      stop 5
  1    format( f6.0,1x,2f3.0,f3.0,f4.0,f4.0,2f6.1,f7.0,12f6.1)
  4    format( 3x ,2f6.1,f9.0,9f6.1)
  2    format(   (10f6.1))                         
  3    format(1x,'NavJulian, hr,min,sec' ,8x,4f5.1)
      end
CCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCC
      subroutine flip(ib,jb,n)
      character*1 ib(n),jb(n)
       do k=1,n-3,4
        jb(k  )=ib(k+3)
        jb(k+1)=ib(k+2)
        jb(k+2)=ib(k+1)
        jb(k+3)=ib(k  )
       end do
      return
      end
ccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc

Data Access and Contacts

FTP Site

The MIR data from TRMM LBA resides on DISC anonymous FTP. You may access the files from this document,

FTP
GIFMIR Calibrated Brightness Temperatures(Binary files)

or directly via FTP at

ftp disc2.nascom.nasa.gov
login: anonymous
password: < your internet address >
cd data/trmm-lba/aircraft/er-2/mir/

Points of Contact

Technical Inquiries about this Data should be addressed to:

Principal Investigator:

James R. Wang
Code 975
NASA Goddard Space Flight Center
Greenbelt, MD 20771
Internet: wang@sensor.gsfc.nasa.gov
(301) 614-5655 (voice)
(301) 614-5558 (fax)

Co-Investigator:

Paul Racette
Code 975
NASA Goddard Space Flight Center
Greenbelt, MD 20771
email:per@meneg.gsfc.nasa.gov
(301) 614-5655 (voice)
(301) 614-5558 (fax)

For additional information, please contact the GES DISC User Services:

GES DISC User Services
Code 610.2
NASA Goddard Space Flight Center
Greenbelt, MD 20771
301-614-5224
Email: help-disc@listserv.gsfc.nasa.gov

The Science

The instrument was first flown in May, 1992, and has accumulated more than 800 flight hours since. It has been involved in a number of field experiments e,g, TOGA/COARE - Tropical ocean Global Atmosphere/Coupled Ocean Atmosphere Response Experiment; CAMEX - Convection and Atmospheric Moisture Experiment, SUCCESS - Subsonic aircraft: Contrail and Cloud Effect Special Studies, WINCE - WINter Cloud Experiment, as well as the calibration/validation work for the SSM/T-2 - Special Sensor Microwave/Temperature-2 aboard the Defense Meterological Satellite Project DMSP, F11 and F12 satellites. Excellent data sets were acquired in all of these flights.

Instrument Characteristics

MIR is a total power cross-track scanning radiometer that measures millimeter-wave radiation at 7 channels: 89, 150, 183.3±1, 183.3±3, 183,3±7, 220, and 340 GHz. It utilizes the strong water vapor line at 183.3 Ghz to provide estimation of atmospheric water vapor profiles. As radiation in this frequency range also responds strongly to absorption and scattering by clouds and hydrometeors, the instrument could provide a measure of cloud and rain-associated parameters.

The MIR is nadir-oriented in the forward compartment of the right wing pod of the ER-2 aircraft. It scans in a plane perpendicular to the direction of flight with a swath of ± 50 degrees from nadir. At the ER-2 aircraft cruising altitude of about 20 km, the footprint at nadir is about 1km. The speed of aircraft is about 200 m/sec. With a scanning cycle of about 3 seconds, MIR produces continuos images at all nine channels with a ground swath of about 42 km. Each scan takes 3 seconds and produces 57 brightness temperature values for all nine channels.

              
                      
                    Accuracy   : ±2 Kelvin
                                      
                    Precision  : 0.5 Kelvin
                                      
               Angular Swath   : ±50 
                                      
                   Beamwidth   : ~ 3 dB (independent of frequencies)
                                      
               Response Time   :  ~40 msec
                                     
                      Weight   : ~180 lbs
                                      
                       Power   : ~400 watts
                                      
                     Platform  : ER-2 aircraft (at ~20 km altitude)
                                      
                     Location  : Right front wing pod
                                      

Data Quality Assessment

The data are geo-referenced based on the ER-2's Inertial Navigation System (INS). Absolute calibration is performed every scan cycle by consecutively pointing the scan mirror at the hot (at 330 K) and cold (at ambient air cooled) external calibration targets which are closely monitored to within ±0.1 K.

References

Racette, P., R.F. Adler, A.J. Gasiewski, D.M. Jackson, J.R. Wang and D.S. Zacharias; An airborne millimeter-wave imaging radiometer for cloud, precipitation and water vapor studies, J. Atmos.Ocean.Tech., 13(3), 610-619, 1996.

Wang, J.R., S.H. Melfi, P. Racette, D.N. Whitemen, L.A. Chang, R.A. Ferrare, K.D. Evans and F.J. Schmidlin; Simultaneous measurements of atmosperic water vapor with MIR, Raman lidar and rawinsondes., J.Appl.Meteor., 34(7) 1595-1607, 1995.

Wang, J. R., S. H. Melfi, P. Racette, D. N. Whiteman, R. A. Kakar, R. A. Ferrare, K. D. Evans and F. J. Schmidlin, 1993: Simultaneous measurements of atmospheric water vapor with MIR, Raman Lidar and rawinsondes. IGARSS'93.

Falcone, V. J., K. Griffin, R. G. Isaacs, J. D. Pickle, J. F. Morrissey, A. J. Jackson, A. Bussey, R. Kakar, J. Wang, P. Racette, D. J. Boucher, B. H. Thomas, and A. M. Kishi, 1993: SSM/T-2 calibration and validation data analysis. Environ. Res. Papers, No. 1111, PL-TR-92-2293, Phillips Laboratory, Hanscom Air Force Base, MA 01731-5000.

Racette, P., L. R. Dod, J. C. Shiue, R. F. Adler, D. M. Jackson, A. J. Gasiewski, and D. S. Zacharias, 1992: Millimeter-wave imaging radiometer for cloud, precipitation, and atmospheric water vapor studies. IGARSS'92, Houston, Texas, 1426-1428.

Wang, J. R. and L. A. Chang, 1990: Retrieval of water vapor profiles from microwave radiometric measurements near 90 and 183 GHz. J. Appl. Meteor., 29(10), 1005-1013.


Last update:Wed Dec 24 08:27:26 EST 2003
Page Author: Hydrology Data Support Team -- hydrology-disc@listserv.gsfc.nasa.gov
Web Curator: -- Website Curator: Anthony Drake
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