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Summary:
The Pathfinder Program, sponsored by the National Oceanic and
Atmospheric Administration (NOAA) and the National
Aeronautics and Space Administration (NASA), is
tasked to produce long-term research quality data
sets for global change research. The SSM/I
Pathfinder Precipitation Rate data set has been
generated using the Goddard Scattering Algorithm,
Version 2 (known as GSCAT2). The algorithm was
applied to antenna temperature data generated from
the
Special Sensor Microwave/ Imager (SSM/I)
instrument flown aboard the Defense
Meteorological Satellite Program (DMSP) F-8
platform. The antenna temperatures in the lower
frequency channels at each location (pixel) are
screened for a precipitation signature. The antenna
temperatures in the 85.5 gigahertz (GHz) horizontal
polarization channel are used in a linear equation
to derive instantaneous precipitation rates. The
Level 2 Precipitation Rate data are in swath
format. Coverage is global, and covers the period
from 1 August 1987 through 31 December 1988.
The SSM/I Pathfinder Level 3 Precipitation Rate
data set has been generated using the the Level 2
data, described above. The Level 2 data were
interpolated to a longitude-latitude grid with a
resolution of 1 degree. The data were weighted
using a pixel weighting scheme to account for pixel
overlap, which is dependant upon the location of
the pixel within the scan and orbit. This weighting
scheme was supplied by the algorithm developers.
Once the weighting was done, the pixels were
averaged over a period of time. The data were
averaged over a period of either 5 days (a pentad)
or an entire month. The data set, including both
pentad and monthly grids, covers the period from 1
August 1987 through 31 December 1988.
Table of Contents:
-
-
-
- NOAA-NASA Pathfinder Level 2 and Level 3
Preciptation Rate from DMSP F-8.
-
-
The NOAA-NASA SSM/I Pathfinder Level 2
Precipitation Rate data set is created
using the NOAA-NASA Pathfinder SSM/I data
set which contain antenna temperature data
as input. Each SSM/I Pathfinder
Precipitation Rate file begins with the
first scan after 00:00:00 UTC and contains
all data up to 23:59:59 UTC. The files are
in Hierarchical Data Format (HDF). The file
size for an uncompressed SSM/I Pathfinder
daily precipitation rate file is 50
megabytes.
-
The NOAA-NASA SSM/I Pathfinder Level 3
Precipitation Rate data set is created
using the NOAA-NASA Pathfinder SSM/I Level
2 Precipitation Rate data set, which
contain full-resolution precipitation rate
data, as input. Each SSM/I Pathfinder
Precipitation Rate file begins with the
first scan after 00:00:00 UTC of the first
day of the gridding period and contains all
data up to 23:59:59 UTC of the last day of
the gridding period. The gridding period
may be either a calendar month or a
pre-determined group of 5 days within the
year, known as a pentad. The files are in
Hierarchical Data Format (HDF). The file
size for an uncompressed SSM/I Pathfinder
gridded precipitation rate file is about
0.8 megabytes.
-
- The objective of producing the NOAA-NASA
SSM/I Pathfinder Level 2 and Level 3
Precipitation Rate data set is to provide
long-term research quality global data for
global change research.
-
- The parameters for the Level 2
Precipitation Rate data set are:
-
- 12.5-km resolution, swath format
Precipitation Rates
- Confidence Flag/Surface Type
- File Description
- Latitude Values
- Longitude Values
- Scan Start Times
- Orbit Parameters
- Precipitation Rate Image.
-
- The parameters for the Level 3
Precipitation Rate data set are:
-
- Precipitation Rate grid, 1 degree
longitude-latitude format
- The Sum of the Squares grid
- The Number of Pixels grid
-
-
- A complete discussion of the Level 2 data
sets is available from the
NOAA/NASA Special Sensor Microwave/ Imager (SSM/I) Pathfinder Daily Precipitation Rate Data (Level 2) and for the Level 3
Precipitation Rate is available from
NOAA/NASA SSM/I Pathfinder Pentad and Monthly Precipitation Rate Data Sets .
-
-
The following related data sets are
available from the Goddard Space Flight
Center (GSFC) Distributed Active Archive
Center (DAAC):
Chang SSM/I Derived Ocean Monthly Rain
Indices
GPCP Combined Precipitation
Arkin & Janowiak GPCP Satellite Derived
Monthly Rainfall
Jaeger Monthly Mean Global
Precipitation
Legates Surface and Ship Observation of
Precipitation
GPCC Rain Gauge Analysis for GPCP
-
-
-
-
-
Data Investigators:
Dr. Robert Adler
Code 912
NASA Goddard Space Flight Center
Greenbelt, MD 20771 USA
Internet: adler@agnes.gsfc.nasa.gov
301-286-9086 (voice)
301-286-1762(fax)
and
Dr. George Huffman
Code 912
NASA Goddard Space Flight Center
Greenbelt, MD 20771 USA
Internet: huffman@agnes.gsfc.nasa.gov
301-286-9785 (voice)
301-286-1762(fax)
Data Producer
Mr. Michael Goodman
Global Hydrology and Climate Center
ES 44
NASA Marshall Space Flight Center
977 Explorer Blvd
Huntsville, AL 35806 USA
Telephone Numbers:(205) 922-5890
Internet: michael.goodman@msfc.nasa.gov
-
- NOAA-NASA Pathfinder Special Sensor
Microwave / Imager (SSM/I) Level 2 and Level
3 Precipitation Rate Data Set.
-
-
Please direct all queries to Goddard Space
Flight Center (GSFC) DAAC Help Desk.
DAAC Help Desk:
- The DAAC Help Desk also provides
additional information on the Goddard
DAAC system capabilities, and other
supported datasets. The Help Desk can be
reached at:
- EOS Distributed Active Archive Center
(DAAC)
- Code 610.2
- NASA Goddard Space Flight Center
- Greenbelt, Maryland 20771
- Internet:daacuso@daac.gsfc.nasa.gov
- 301-614-5224 (voice)
- 301-614-5268 (fax)
-
-
The GSCAT2 algorithm uses the natural
properties of microwave energy to determine
instantaneous precipitation rates within the
area defined by the pixel. Upwelling microwave
energy is scattered by ice crystals which are
usually present during different phases of the
lifetime of convection and other precipitating
systems. The GSCAT2 uses the various operating
channels of the SSM/I to first mask off pixels
as "no rain" which do not meet the criteria to
be labelled as "rain". This masking includes
surface features such as melting snowpack, cold
ocean, desert sand and land-water interfaces.
The remaining pixels (which are unmasked) are
then converted to instantaneous precipitation
rates. The precipitation rate (in mm/hr) is
inversly proportional to the brightness
temperature; therefore, a cutoff value of 247 K
(which equals 1 mm/hr) is used as the maximum
temperature (minimum intensity) in the
equation. Some unmasked pixels have a lower
confidence than others; these are called
"ambiguous" and are flagged as such in the
Confidence/Surface Type object.
-
The GSCAT2 algorithm output is used to create
pentad and monthly grids of precipitation rate.
The full-resolution output is weighted using a
pixel weighting scheme supplied by the GSCAT2
algorithm developers. This weighting scheme is
used to account for the varying amount of pixel
overlap which is dependant upon the location
within the scan and orbit. Once the data has
been weighted, it is interpolated to a 1 degree
by 1 degree longitude-latitude grid. This grid
is aligned such that the left side of the grid
corresponds to 180 degrees longitude. Thus, the
grid location (1,1) corresponds 180-179 degrees
west longitude, 90-89 degrees north latitude.
-
No flagged values are used in computing any of
the gridded values. In fact, counts of the
ambiguous and cold surface pixels are kept for
each grid box. If the percentage of the sum of
these pixels exceeds a preset threshold, then
the grid box is flagged as having bad or low
confidence data, and no average is given. Grid
boxes with no data are also flagged.
-
-
-
The information marked with an asterisk
(*) in Section 5: Equipment, is quoted
from:
-
Hollinger, J. P., J. L. Peirce, and G. A.
Poe, 1990: SSM/I instrument evaluation.
IEEE Transactions on Geoscience and
Remote Sensing,
28(5), 781-790.
The SSM/I consists of an offset
parabolic reflector illuminated by a
corrugated broad-band, seven port horn
antenna. The reflector and feed-horn
antenna are mounted on a drum which
contains the radiometers, digital data
subsystem, mechanical scanning subsystem,
and power subsystem. The entire reflector,
feed horn, and drum assembly is rotated
about the axis of the drum by a coaxially
mounted bearing and power transfer assembly
(BAPTA). All data, commands, timing and
telemetry signals, and power pass through
it on slip ring connectors to the rotating
assembly.
-
- The SSM/I is a passive microwave
sensor aboard the operational DMSP F-8
polar orbiting satellite.
-
- The DMSP Block 5D-2 F-8 spacecraft
flies in a near polar sun-synchronous
orbit. Launched on 18 June 1987, the
satellite completes 14.1 revolutions per
day, the subsatellite ground track
repeats approximately every 16 days.
-
- The mission of the DMSP is to provide
global, visual and infrared cloud data
and other specialized near real-time
meteorological, oceanographic and
solar-geophysical data required to
support worldwide Department of Defense
operations and high-priority programs.
Timely data are supplied to Air Force
Global Weather Central (AFGWC), the Navy
Fleet Numerical Meteorology and
Oceanography Center (FNMOC) and to
deployed tactical receiving terminals
worldwide.
-
-
Operational parameters include the
following orbital elements:
- Nominal altitude: 833 km
- Inclination: 98.8 degrees
- Nodal period: 102 minutes
- Equator crossing: 0612 (ascending
local time)
-
-
The SSM/I is a seven-channel,
four-frequency linearly polarized
passive microwave radiometric system.
The instrument measures atmospheric,
land and ocean surface brightness
temperatures at 19.3, 22.2, 37.0 and
85.5 GigaHertz (GHz).
-
-
The SSM/I rotates at a uniform rate
making one revolution in 1.9 seconds,
during which time the satellite
advances 12.5 km. The antenna beams are
at an angle near 45 degrees to the
BAPTA rotational axis, which is normal
to the earth's surface. Thus, as the
antenna rotates, the beams define the
surface of a cone and, from the orbital
altitude of 833 km, make an angle of
incidence of 53.1 degrees at the
earth's surface.
The scene is viewed over a scan
angle of 102.4 degrees centered on the
ground track aft of the satellite,
resulting in a scene swath width of
1394 km.
For a discussion of channel sampling
methods, please refer to Sensor Measurement Geometry.
-
- The SSM/I was built by Hughes
Aircraft Company under the direction of
the Naval Space Systems Activity and the
Air Force Space Division.
-
A small mirror and hot reference
absorber are mounted on the BAPTA and do
not rotate with the drum assembly. They are
positioned off-axis such that they pass
between the feed horn and the parabolic
reflector, occulting the feed once each
scan. The mirror reflects cold sky
radiation into the feed thus serving, along
with the hot reference absorber, as
calibration references for the SSM/I.*
This scheme provides an overall absolute
calibration which includes the feed horn.
Corrections for spillover and antenna
pattern effects from the parabolic
reflector are incorporated in the data
processing algorithms.
For a complete discussion of the SSM/I
calibration, please refer to
SSM/I Instrument Evaluation (Hollinger
et al. 1990).
-
-
The Antenna Temperature (Ta) data used for the
SSM/I Pathfinder Project are provided by Remote
Sensing Systems of Santa Rosa, California and
are originally derived from the Temperature
Data Records (TDR) processed at the FNMOC in
Monterey, California. This data is processed at
MSFC into the NOAA-NASA SSM/I Pathfinder Ta
data set, which is then used as input to create
the NOAA-NASA SSM/I Pathfinder Level 2
Precipitation Rate data set, using the GSCAT2
algorithm.
- The SSM/I Pathfinder Level 2 Precipitation
Rate data set is then used to generate the
NOAA-NASA SSM/I Pathfinder Level 3 Precipitation
Rate data set. The Level 2 output is binned,
averaged, and flagged as describe in Section 3. Theory of Measurements
. For details on the processing of the Level 2
data sets, see the
NOAA/NASA Special Sensor Microwave/ Imager (SSM/I) Pathfinder Daily Precipitation Rate Data (Level 2) and for the Level 3 data sets, see
NOAA/NASA SSM/I Pathfinder Pentad and Monthly Precipitation Rate Data Sets.
-
-
-
- No notes at this time.
-
- No field notes.
-
-
-
-
-
- Coverage of the Pathfinder Level 2
and Level 3 Precipitation Rate data sets
is global.
-
-
For the spatial coverage map, blue
indicates areas where good data can
occur within the grid, black indicates
where good data can not occur within
the grid, and gold indicates the
coastal outlines.

-
-
The Pathfinder Level 2 Precipitation
Rate data set has been produced at full
resolution (12.5 km).
The Pathfinder Level 3 Precipitation
Rate data set has been produced at a
resolution of 1 degree in latitude and
longitude.
-
-
The Pathfinder Level 2 Precipitation
Rate data set has been produced in
swath format.
The Pathfinder Level 3 Precipitation
Rate data set has been produced in a
equirectangular cylindrical
projection.
-
- The Pathfinder Level 3 Precipitation
Rate data set uses an equal-angle
(longitude-latitude) grid with each grid
box corresponds to an equal interval of
latitude and longitude.
-
-
-
- Both data sets cover the period from
1 August 1987 to 31 December 1988, which
includes the Pathfinder Benchmark Period
(1 August 1987 to 30 November 1988). On
December 3, 1987, the F-8 SSM/I
instrument was turned off due to
overheating. It was turned on again on
January 13, 1988. No data was taken
during this period, and thus neither data
set contains products from this period.
Several other small gaps are also in the
data. for more information
about gaps in the data.
-
-
This map provides the temporal
distribution of the available SSM/I
data used to derive the precipitaiton
rate products.

-
-
The Level 2 data set is available at a
resolution of one day.
The Level 3 Pentad data set is
available at a resolution of 5
days.
The Level 3 Monthly data set is
available at a resolution of one
month.
-
-
-
- Average precipitation rate, in mm/day
(for the Level 3 data) or in mm/hr (for
the Level 2 data).
-
- The variable measured is an
instantaneous precipitation rate, in
mm/hr for the Pathfinder Level 2 data set
(the precipitation rates are averaged and
then converted to mm/day for the Level 3
data set). Instantaneous precipitation
rate refers to the fact that the variable
is a rate of accumulation of
precipitation, measured at the exact
moment that the instrument samples the
area in question.
-
-
For the Level 2 Precipitation Rate data
set, the units are average
precipitation rate in mm/hr * 10.0
-
For the Level 3 Precipitation Rate data
set, the units are average
precipitation rate in mm/day * 100.0
-
- The data from which the Pathfinder
Level 2 Precipitation Rate data are
generated come from the DMSP F-8 SSM/I
instrument.
-
-
For the Level 2 Precipitation Rate data
set, the range of unscaled values is 0
- 100 mm/hr
- For the Level 3 Precipitation Rate
data set, the range of unscaled values is
0 - 2400 mm/day
-
- For a description of the type of objects
included in the Level 2 Precipitation Rate
files, refer to the
NOAA/NASA Special Sensor Microwave/ Imager (SSM/I) Pathfinder Daily Precipitation Rate Data (Level 2) and for the Level 3
Precipitation Rate files, refer to
NOAA/NASA SSM/I Pathfinder Pentad and Monthly Precipitation Rate Data Sets .
-
-
-
-
A general description of data granularity
as it applies to the IMS appears in the
EOSDIS Glossary.
-
For the Level 2 products, data is stored in
daily files by orbit. The DMSP satellite
completes just over 14 orbits each day. An
orbit is defined as starting when the
satellite crosses the equator going from
south to north. Since (swath) data is
stored by time, it's possible to have a
fraction of an orbit before the first and
last full orbits in a particular day's
file. Missing data is flagged, such that
any data falling on the previous or
following days (before 00:00:00 or after
23:59:59 UTC of the current day) will not
be present and the scan position will be
filled with a missing data flag.
For the Level 3 products, data are
stored as grids to which all orbits for a
given period (i.e., either a pentad or a
month) have been interpolated.
-
- All of the data in the Pathfinder Level 2
and Level 3 data sets are stored in
Heirarchical Data Format (HDF).
-
-
-
-
The TB rain rate equation used over land
surfaces is
- TB = 251.0 - (4.19 * R)
-
where TB is the brightness temperature and
R is the precipitation rate in mm/hr.
-
For temperatures over an ocean surface, the
equation is
- TBocean = 251.0 - (2.09 * R)
-
where R is as defined above and TBocean is
the brightness temperature over an ocean.
Over the coastal regions, the slope
(multiplier for the precipitation rate R)
is an average of the land and ocean values.
-
-
- The above formulae are derived
statisitically from microwave modelling
observations. For more information, refer
to the list of references in the
NOAA/NASA Special Sensor Microwave/ Imager (SSM/I) Pathfinder Daily Precipitation Rate Data (Level 2)
.
-
-
-
-
The antenna temperature data are read
into the processing software, and, scan
by scan, are checked for data quality.
The 19, 22, and 37 GHz channels are
interpolated to match the resolution of
the 85 GHz channels. The data from the
channels is then used to screen each of
the 85 GHz horizontal polarization
pixels for a precipitation signature. A
linear regression equation is then
applied to the 85 GHz pixels which have
been selected as having precipitation.
This data is output as the Level 2
Precipitation Rate data.
These data are then used to create
the Level 3 Precipitation Rate data.
The precipitation rates are
interpolated to a 1 degree
latitude-longitude grid, after a
pixel-weighting scheme has been
applied. Any grid bin populated by
ambiguous (low confidence) data or cold
surface (ice surface) data above a
certain threshold is flagged as bad.
These data are output as the Level 3
Precipitation Rate data
A discussion of the Level 2
processing sequence can be found in the
NOAA/NASA Special Sensor Microwave/ Imager (SSM/I) Pathfinder Daily Precipitation Rate Data (Level 2) and for
the Level 3 processing sequence, refer
to
NOAA/NASA SSM/I Pathfinder Pentad and
Monthly Precipitation Rate Data
Sets .
-
- No changes have been made to the
processing sequence.
-
-
-
- No enhancements were made to the
GSCAT2 algorithm, except to enable the
algorithm to accept the NOAA-NASA
Pathfinder Antenna Temperature data set
as input.
-
- The only calculated variable is the
precipitation rate.
-
- No graphs or plots are available.
-
-
-
- No information on error sources is
available at this time.
-
-
-
- Studies have been conducted by the
GSCAT2 algorithm developers. Refer to the
list of references available in NOAA/NASA Special Sensor Microwave/ Imager (SSM/I) Pathfinder Daily Precipitation Rate Data (Level 2) for information on the
data validation.
-
- The NOAA/NASA Pathfinder Team
believes this data set to be an accurate
representation of the algorithm as
developed by the GSCAT2 algorithm
developers.
-
- There is no data about the
measurement error at this time.
-
- The algorithm was implemented to use
SSM/I Pathfinder Antenna Temperature data
sets as input, and the Level 2 and Level
3 output were reviewed by the algorithm
developers to ensure that the algorithm
had been properly implemented.
-
- The Pathfinder Level 2 and Level 3
Precipitation Rate data have been through
a rigorous quality control procedure, and
both data sets are judged to be accurate
representations of the algorithm. For
details, contact the GSFC DAAC Help Desk
Office.
-
-
-
- This algorithm is a scattering algorithm
and will primarily identify convective
precipitation. Stratiform precipitation will
be underestimated.
-
-
The algorithm will sometimes define pixels
of precipitation rate as "ambiguous" which
indicates a lower confidence in the
existence of precipitation at that pixel.
Sometimes these ambiguous pixels are the
result of surface ice or snow melting. The
user should be cautious when using these
pixels in large scale precipitation
studies. A significant number of ambiguous
pixels should be viewed as suspect data.
The algorithm will also label pixels as
"cold surface", which are associated with
snow/ice fields. No precipitaion is
associated with cold surface pixels.
Precipitation rates which are co-located
with a large number of "cold surface"
pixels should also be treated as suspect
data.
All reference materials refer to
brightness temperatures; however, at the
direction of the algorithm developers,
antenna temperatures were used in the
computation of the precipitation rates.
In some of the Level 3 pentad grids,
there are bins which are obviously
ambiguous precipitation rates, although
they are not flagged. This is due to the
higher ambiguous/cold surface threshold
used in the pentad processing (40%) as
opposed to the lower threshold of the
monthly processing (20%). This allows a
precipitation rate average to be calculated
even at the occurrence of higher
ambiguous/cold surface counts. Most of
these bins occur in the far Norhtern
Hemisphere polar region during the summer
months
-
- See Section 11.2 Known
Problems with the Data above for usage
guidance.
-
- No other information at this time.
-
- Monitoring of global precipitation.
-
- Please Note: These files were generated and
archived at MSFC. Recently the SSM/I pathfinder
dataset is moved to Goddard DAAC. The file
description written in each file has not been
updated for the new point of contact and user
service mail address since in few months this
data will be replaced with the new version of
SSM/I path finder data produced by Drs. Adler and
George Huffman group at Goddard NASA. However for
more information on the existing data and
informations on the old and new algorithms please
contact the Goddard Space Flight
Center DAAC Help Desk.
-
-
-
-
Three pieces of software are sent with the
Level 2 Precipitation Rate data as
utilities to aid in handling the data
within the files. The routines are
"extractpr.c", "getorbpr.c", and
"getfiledesc_pr.c". A makefile is also sent
along to compile this software. The user
will also need to access NCSA's HDF library
software, which is free from NCSA via ftp.
A README is also sent along with the data
to help the user understand the files and
the data.
-
Three pieces of software are sent with the
Level 3 Precipitation Rate data as
utilities to aid in handling the data
within the files. The routines are
"extractrg.c", "getfiledesc.c" and
"read_bin.c". A makefile is also sent along
to compile this software. The user will
also need to access NCSA's HDF library
software, which is free from NCSA via ftp.
Documentation is also sent along with the
data to help the user understand the files
and the data.
-
For more information about the Level 2
software and how to use it, refer to
NOAA/NASA Special Sensor Microwave/ Imager (SSM/I) Pathfinder Daily Precipitation Rate Data (Level 2) and for the Level 3
software, see
NOAA/NASA SSM/I Pathfinder Pentad and
Monthly Precipitation Rate Data Sets.
-
- To access information about how to
retrieve the HDF libraries, please refer to
the Goddard DAAC HDF
Information Page
-
-
-
Goddard Space Flight Center
DAAC Help Desk.
-
-
- GSFC Distributed Active Archive
Center
-
-
This data set is available via several
ways: by contacting the GSFC DAAC Help
Desk, by accessing the Goddard DAAC
Prepackaged Tape Ordering System via the
WWW interface, or Anonymous FTP.
The DAAC Help Desk also provides additional
information on the Goddard DAAC system
capabilities, and other supported datasets.
The Help Desk can be reached at:
EOS Distributed Active Archive Center (DAAC)
Code 610.2
NASA Goddard Space Flight Center
Greenbelt, Maryland 20771
Internet:daacuso@daac.gsfc.nasa.gov
301-614-5224 (voice)
301-614-5268 (fax)
ANONYMOUS FTP:
The Precipitation Global Data Set also
resides on-line at the Goddard DAAC
anonymous FTP and may be accessed either
directly from this document,
SSM/I Pathfinder Daily
Precipitation
SSM/I Pathfinder Pentad
Precipitation
SSM/I Pathfinder Monthly
Precipitation
- or can be acessed via FTP at
- ftp daac.gsfc.nasa.gov
- login: anonymous
- password: < your internet address
>
- cd
http://disc.sci.gsfc.nasa.gov/data/precipitation/precip/ssmi_pathf_monthly(pentad
or daily)
-
- The GSFC DAAC plans to periodically check
with the data producer regarding updates to
the data set.
-
- Data sets are provided on 8 mm tapes, or
via FTP.
-
-
Satellite/Instrument/Data
Processing Documentation:
-
- Hollinger, J. P., R. Lo, G. Poe,
R. Savage, and J. Peirce,1987:
Special Sensor Microwave/Imager User's
Guide.
- Hollinger, J. P., ed,
1989: DMSP Special Sensor
Microwave/Imager Calibration/Validation Final
Report Volume 1.
- MSFC DAAC Users Guide to Special Sensor
Microwave Imager (SSM/I) Data (NESDIS Level
1b Format), 1993: George C. Marshall Space
Flight Center Distributed Active Archive
Center, pub.
- Wentz, F.J., 1991:
User's Manual SSM/I Antenna Temperature Tapes
(Revision 1).
-
Journal Articles and
Study Reports:
-
- Adler, Robert F., A. J. Negri, P.
R. Keehn, and I. M. Hakkarinen,
1993: Estimation of Monthly Rainfall
over Japan and Surrounding Waters from a
Combination of Low-Orbit Microwave and
Geosynchronous IR Data. Journal of
Applied Meteorology,
32, 335-356.
- Adler, Robert F., H.-Y. M. Yeh,
N. Prasad, W.-K. Tao and J. Simpson,
1991: Microwave Simulations of a
Tropical Rainfall System with a
Three-Dimensional Cloud Model. Journal of
Applied Meteorology,
30, 924-953.
- Adler, Robert F., G. J. Huffman,
and P. R. Keehn, 1994: Global
Tropical Rain Estimates From
Microwave-adjusted and Geosynchronous IR
Data. Remote Sensing Reviews, in
press.
- Hollinger, J. P., J. L. Peirce,
and G. A. Poe, 1990: SSM/I
Instrument Evaluation. IEEE Transactions
on Geoscience and Remote Sensing,
28(5), 781-790.
-
EOSDIS glossary
-
EOSDIS acronyms
Other Terms:
- NOAA: National Oceanic and
Atmospheric Administration
- NASA: National Aeronautics
and Space Administration
- DMSP: Defense Meteorological
Satellite Program
- SSM/I: Special Sensor
Microwave/Imager
- GSCAT2: Goddard Scattering
Algorithm Version 2
- HDF: Hierarchical Data
Format
- Ta: Antenna Temperature
- Tb: Brightness
Temperature
- PR: Precipitation Rate
- mm: millimeter
- GHz: Gigahertz
- March 11, 1997
- March 11, 1997
- Intentionally left blank
- Intentionally left blank
- Hydrology Data Support Team
(hydrology@daac.gsfc.nasa.gov)
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http://disc.gsfc.nasa.gov/guides/GSFC/guide/ssmi_pathf_preciprate_data.gd.shtml
Change History
- Version 2.0
- Version baselined on addition to the GES
Controlled Documents List, March 11, 1997.
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