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Summary:
The Chang Special Sensor Microwave/Imager (SSM/I) Monthly Rainfall
Indices were generated using the SSM/I brightness temperatures (TB) from
the Defense Meteorological Satellite Program (DMSP) F8 and F11 satellites.
The data set contains gridded ocean monthly total rainfall indices. The
period of record for the data set is July, 1987 through December, 1995.
Table of Contents:
- Chang SSM/I Derived Monthly Rain Indices
- The Chang SSM/I Monthly Rainfall Indices were generated using the
SSM/I brightness temperatures from the DMSP satellites F8 and F11. The
data set contains gridded ocean monthly total rainfall indices. The data
are on a 5 x 5 degree grid covering the area from 50N to 50S and 180E to
180W. Each grid cell value is the average of the satellite's ascending
and descending estimates, corrected for beam fillings errors. Grid values
are computed only over the oceans.
The data is binned into months using the Global Precipitation Climate
Project (GPCP) convention. Using this convention, each month consists of
six pentads (30 days total) except for August which contains seven
pentads (35 days total).
- This information is not available at this time.
- Global ocean monthly rainfall indices
- This information is not available at this time.
- SM/I Level 1b Sensor Counts from DMSP F8, F10, F11
SSM/I Pathfinder Data Sets
Wentz Antenna Temperatures
Wentz Geophysical Products
SSM/I Prabhkara Brightness Temperatures
MSU Daily Ocean Precipitation
- Dr. Alfred Chang
Hydrological Sciences Branch, Code 974
NASA Goddard Space Flight Center
Greenbelt, Maryland 20771
U.S.A.
301-286-8997 (Voice)
301-286-1758 (Fax)
email address: ACHANG@RAINFALL.GSFC.NASA.GOV
- Retrieval of Monthly Rainfall Indices from Microwave
Observations
- 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 information in section 3: Theory of Measurements is quoted
from:
-
Wentz, F.J., User's Manual SSM/I Antenna Temperature Tapes.
Santa Rosa, CA: Remote Sensing Systems, 1988, pp 9-13. The absolute
brightness temperature of the scene (TB) incident upon the antenna is
received and spatially filtered by the antenna to produce an effective
input signal or antenna temperature (TA) at the input of the feedhorn
antenna. The procedure for deriving Earth antenna temperatures is
discussed below.
-
In computing the SSM/I antenna temperatures, the basic assumption is
that the radiometer output voltage is linearly related to the input
power at the mixer/preamplifier. Nonlinear effects such as
imperfections in the square-law detector and Intermediate Frequency
(IF) amplifier compression are assumed negligible. Expressing the input
power in terms of radiation temperature gives
V(i) = ckBg(TA(i) + TN) (1)
where V(i) is the radiometer output voltage,
TA(i) (Kelvin) is the radiation temperature entering the
feedhorn, and TN (Kelvin) is the radiometer noise
temperature. The constants are c = detector constant, k = Boltzmann
constant, B = receiver predetection bandwidth, and g = receiver
gain. The subscript i denotes either a cold-space observation (i =
C), a hot-load observation (i = H), or an Earth
observation (i = E). The gain and noise temperature are assumed
stable over the period of one scan, which is 1.9 seconds. That is to say, g
and TN are assumed to be the same for the cold-space,
hot-load, and Earth observations. The output voltage (V)
is converted to counts (C) by applying a scaling factor
(w) and a constant offset (P):
C(i) = wV(i) - P (2)
Combining (1) and (2) for i = C, H, and E gives
TA(E) = A *
C(E) + B
(3)
A = (TA(H) -
TA(C)) / (C(H) -
C(C)) (4)
B = ((TA(C) *
C(H)) - (TA(H) *
C(C))) / (C(H) -
C(C)) (5)
For each SSM/I scan, five cold counts and five hot counts are recorded
for each channel. (Only 85 GHz observations are taken on the B-scans). The
quantities C(C) and
C(H) are found by averaging the five individual
counts. The cold space antenna temperature TA(C)
is set to 2.7 K for all channels. The hot reference antenna temperature is
found from
TA(H) = T0(H) + 0.01(TO(P) - TO(H)) (6)
where TO(H) and
TO(P) are the physical temperatures of the hot
load and the radiator plate facing the hot load. The small correction for
the radiator plate is to account for radiative coupling between the hot
load and the top plate of the rotating drum assembly which faces the hot
load. There are three thermistors on the hot load and one on the radiator
plate. The temperature T0(H) is found by
averaging the three thermistor readings. Thus the A and
B coefficients can be computed, and equation (3) can be
inverted to recover the original values for the Earth-viewing counts
C(E).
-
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 Defense Meteorological Satellite Program (DMSP) Block 5D-2
spacecrafts fly in a near polar sun-synchronous orbit. The satellites
complete 14.1 revolutions per day and the subsatellite ground track
repeats approximately every 16 days.
- The mission of the DMSP is to provide global visual and infrared
meteorological and oceanographic data required to support worldwide
Department of Defense operations and high-priority programs. Timely
data are supplied to Air Force Global Weather Central, the Navy Fleet
Numerical Meteorology and Oceanography Center (FNMOC) and to deployed
tactical receiving terminals worldwide.
- Operational parameters include the following orbital
elements:
DMSP F8 DMSP F11
Maximum Altitude 882 Km 878 Km
Minimum Altitude 838 Km 841 Km
Inclination 98.8 Degrees 98.8 Degrees
Nodal Period 101.8 Min 101.9 Min
Equator Crossing 19:42 17:04
(Ascending)
- The SSM/I is a seven-channel, four-frequency linearly polarized
passive microwave radiometric system. The instrument measures
brightness temperatures at 19.3, 22.2, 37.0 and 85.5 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 of 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 approximately 1400 km.
-
For a discussion of channel sampling methods, please refer to Sensor
Measurement Geometry.
- Hughes Aircraft Company
-
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 tolerance is +/- 0.5 Kelvin for the lower frequencies and +/-
1 Kelvin for 85 Ghz.
- The antenna temperature of the SSM/I is calibrated each scan from
the input to the feedhorn through the output of the A/D converter.
For a complete discussion of the SSM/I calibration, please refer to
SSM/I
Instrument Evaluation (Hollinger et al. 1990).
- Not applicable for this data set.
- The Goddard DAAC obtains the monthly rainfall indices data set
via an ftp transfer from Dr. Al Chang, NASA Goddard Space Flight
Center.
- No additional data notes are available.
- No field notes are available.
- The SSM/I produces a swath width of approximately 1400 km and
approximately 14 orbits, comprised of ascending and descending
passes, per day for global coverage.

- The swath width for the SSM/I is approximately 1400 kilometers.
The Effective Field of View (EFOV) on the Earth Surface varies from
69 km along-track, 43 km cross-track for the 19 GHz channels to 15 km
along-track, 13 km cross-track for the 85 GHz channels.
- For a desecription of the scan projection, see Sensor
Measurement Geometry.
- The data are on a 5 x 5 degree grid for the area from 50N to 50S
and 180W to 180E.
- The period of record for the data set is from July, 1987 through
December, 1995. The DMSP F8 brightness temperatures were used to
compute the rainfall indices from July, 1987 through December, 1991.
The DMSP F11 brightness temperatures were used to compute the
rainfall indices from January, 1992 through December, 1995.
- A temporal coverage map is not available at this time.
- The rainfall indices data files are in monthly files which
contain 30 days of data, except for August which contains 35 days of
data. During the leap years, the data for February will contain 31
days. The following is a list of which Julian days are included in
each month.
Month Inclusive Dates Inclusive Julian Days
January 01/01 - 01/30 001 - 030
February 01/31 - 03/01 031 - 060 **
March 03/02 - 03/31 061 - 090
April 04/01 - 04/30 091 - 120
May 05/01 - 05/30 121 - 150
June 05/31 - 06/29 151 - 180
July 06/30 - 07/29 181 - 210
August 07/30 - 09/02 211 - 245
September 09/03 - 10/02 246 - 275
October 10/03 - 11/01 276 - 305
November 11/02 - 12/01 306 - 335
December 12/02 - 12/31 336 - 365
** Note that leap year will have an extra day.
- The parameter for this data set is precipitation.
- Precipitation - Any or all forms of liquid or solid water
particles that fall from the atmosphere and reach the surface of the
Earth. It includes drizzle, rain, snow, snow pellets, snow grains,
ice crystals, ice pellets, and hail. Precipitation is also defined as
a measurement of the quantity, expressed in centimeters or
milliliters of liquid water depth, of the water substance that has
fallen at a given location in a specified amount of time.
- The rainfall indices are in units of millimeters per month.
- The monthly rainfall indices were derived from Special Sensor
Microwave/Imager instrument measurements.
- The data ranges from -10.0 to 2378. The -10.0 value is a flag to
denote land cells or cells that have island contamination or cells in
which any rain retrieval that did not converge .
- The following is sample of a partial month of the rainfall
indices data set.
Y87M07
-10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0
-10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0
-10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 179.2
111.7 143.1 62.6 55.5 154.9 206.5 219.4 157.9 61.5 178.8
116.1 50.1 46.2 20.2 10.2 15.1 23.1 -10.0 -10.0 -10.0
-10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0
-10.0 85.4 191.6 98.3 52.0 32.9 85.3 20.4 19.0 64.1
80.1 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0
-10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0
-10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 -10.0 222.0
-10.0 139.8 267.1 184.7 107.8 138.6 169.5 218.1 358.2 311.5
-
A general description of data granularity as it applies to the
IMS appears in the
EOSDIS Glossary.
-
The complete data set is contained in a single file that has a
volume of approximately 1.18 Megabyte.
- The Chang monthly rainfall indices data set is in ASCII
format.
- The file name is:
- gpcp_ssmi_1295_5.0_v23
- Each grid cell value is the average of the satellite ascending
and descending estimates, corrected for beam filling errors. The
equation used to calculate the estimates is
(ascending + descending) * 0.5 * 1.5.
The grid values are computed only over the oceans and the grid cells
which correspond to land are set to a flag of -10.0.
- This information is not available at this time.
- This information is not available at this time.
- This information is not available at this time.
- Average Monthly Precipitation
- No graphs or plots are available.
- No known sources of error exist at this time.
- This information is not available at this time.
- This information is not available at this time.
- This information is not available at this time.
- This information is not available at this time.
- The GSFC DAAC assures that the data file can be read and contains
all data within the specified period of record.
- The rainfall indices were computed only over the oceans for this
data set. Therefore, this data set should not be used to examine land
surface rainfall.
- There are 33 cells set to -10.0 due to island contamination. Any
rain retrieval that did not converge for a given cell results in that
cell being set to -10.0.
- This information is not available at this time.
- This information is not available at this time.
- This information is not available at this time.
- The data producer provides periodic updates to the data set with
increased temporal coverage. The GSFC DAAC will work with the data
producer to include the additional data in the archive.
- There is no software associated with this data set.
- This information is not applicable to this data set.
- Goddard Space Flight Center DAAC User
Services.
- GSFC Distributed Active Archive Center
- This data set resides on DAAC Anonymous FTP.
-
The DAAC User Services or 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)
DAAC SEARCH AND ORDER SERVICES:
The Goddard DAAC maintains archives of these datasets. The data stored
in our archives can be ordered using the following search and order
utilities
ANONYMOUS FTP:
The Chang precipitation data set resides on DAAC anonymous FTP. The
data files may be accessed from this document,
Chang SSM/I Derived Monthly Rain
Data
- or directly via FTP at
- ftp disc1.gsfc.nasa.gov
- login: anonymous
- password: < your internet address >
- cd data/hydrology/precip/chang
- The GSFC DAAC will continue to archive and distribute updates
received from the data producer. The Goddard DAAC plans to
periodically check with the data producer regarding the data set
revisions.
- Data sets are available on 8mm tape, 4mm DAT, or anonymous ftp.
- Wilheit, T., A. Chang, L. Chiu, 1991: Retriecal of monthly
rainfall indices from microwave radiometric measurements using
probability distribution functions. Journal of Atmospheric and
Oceanic Technology, 8, 118-136.
- Chang, A., L. Chiu, T. Wilheit, 1993: Random errors of oceanic
monthly rainfall derived from SSM/I using PDF. MWR, 121,
2351-2354.
- Wentz, F. J., User's Manual SSM/I Antenna Temperature Tapes
(Revision 1), RSS Technical Report 120191, 70 pp, Remote Sensing
Systems, Santa Rosa, CA, 1 December 1991.
- 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.
Distributed Active Archive Center
Defense Meteorological Satellite Program
Fleet Numerical Meteorology and Oceanography Center
Global Precipitation Climate Project
Goddard Space Flight Center
Microwave Sounding Unit
Special Sensor Microwave/Imager
Brightness Temperatures
Uniform Resource Locator
EOSDIS acronyms
-
- August 1, 1996
-
- August 1, 1996
-
- Not available at this time.
-
- Not available at this time.
-
- Suraiya Ahmad (ahmad@daac.gsfc.nasa.gov)
-
-
http://disc.sci.gsfc.nasa.gov/DATASET_DOCS/chang_gpcp_ssmi_precip_data.html
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