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Kalpana-1/MetSat-1 (Meteorological Satellite-1)
MetSat-1 is ISRO's first dedicated GEO weather satellite project built by ISRO. So far, meteorological services had been combined with telecommunication and television services in
the INSAT series. MetSat-1 is a precursor to the future INSAT system that will have separate satellites for meteorology and telecommunication & broadcasting services.
Note: In a commemorative ceremony on Feb. 6, 2003, the MetSat-1 satellite of ISRO was
renamed to Kalpana-1 by Indian Prime Minister Atal Bihari Vajpayee. This is to honor Kalpana Chawla, born in Karnal (1961), India, who died as a NASA astronaut on Feb. 1, 2003
over the southern USA when Space Shuttle Columbia (flight STS-107, Jan. 16 - Feb. 1,
2003) and her crew perished during reentry.
The exclusive meteorological payload has its advantages in such arguments as: 1) 2) 3)
· The scarce resource of orbital slot and frequency spectrum are best exploited, if the
missions (communication vs meteorological) are made exclusive
· The performance of the meteorological payload gets somewhat constrained in the environment of high power transponders
· There is an urgent need to realize an in-orbit replacement for this all-too-important
national service of meteorology. MetSat-1 has to fill the void caused by two important
meteorological payloads, namely VHRR/2 on INSAT-2E which failed already in 1999.
On Nov. 4, 2000, ISRO was forced to retire INSAT-2B, after it ran out of station-keeping fuel (in July 2000, INSAT-2B completed its design life of seven years of operation).
This action stopped of course also the VHRR instrument on INSAT-2B, used for operational meteorology. MetSat-1 is considered a cost-effective solution to serve exclusively
in GEO for meteorological payloads and services.
The policy on future ISRO GEO satellites continues to separate the meteorological and
communication payloads on a case-by-case basis. The next exclusive meteorological satellite of ISRO is INSAT-3D which will carry a meteorological imager, a meteorological
sounder as well as SAS&R and DRT payloads. Since the configuration of INSAT-3 series of
satellites is already decided, the multipurpose INSAT-3A carries a VHRR and a CCD camera besides SAS & R and DRT payloads. The configuration of INSAT-4 series is yet to be
decided.
Figure 1: Schematic illustration of the MetSat-1 spacecraft I-1000 bus
The MetSat-1 spacecraft was developed by ISAC (ISRO Satellite Center), Bangalore. MetSat has been designed using a new spacecraft bus (I-1000 bus) employing lightweight structural elements like CFRP (Carbon Fibre Reinforced Plastic). A central structural thrust cylinder provides mounting interfaces propellant tanks, pressurant tank, equipment panels,
payload, solar array assembly, and with the launch vehicle. Structural brackets are provided
to mount momentum wheels, reaction wheel, RCS (Reaction Control System) thrusters,
earth sensors, sun sensors, LAM (Liquid Apogee Motor), and propulsion components.
MetSat-1 is three-axis stabilized (momentum biased control subsystem). However, unlike
its INSAT predecessors, the MetSat-1 spacecraft does not feature a sail/boom design. The
attitude is sensed by suite of sensors (gyros, Earth sensors, digital sun sensor, coarse analog
sun sensors, and solar panel sun sensor). Magnetic torquers serve as actuators to unload the
momentum of the wheels. In addition, active thrusters are used (one 440N LAM for orbit
raising maneuvers and eight 22 N thrusters for orbit and attitude control). The propulsion
system employed is a unified bi-propellant with mono-methyl hydrazine (MMH) as fuel and
mixed oxides of nitrogen (MON3) as oxidizer. The S/C employs passive thermal control system by utilizing multi-layer insulation blankets, optical solar reflectors, heat sinks, paints,
thermal grease, thermal shields etc. A bank of 112 heaters spread over the satellite maintain
the temperature of individual subsystems. 4) 5) 6)
Figure 2: Illustration of the deployed Kalpana-1/MetSat-1 spacecraft
The S/C has a launch mass of 1055 kg including 560 kg of propellant (495 kg S/C dry mass).
Electrical power of 550 W is generated by a single panel solar array of 2.15 m x 1.85 m using
GaAS solar cells. The solar panel features a drive mechanism to point it into the sun. A
single battery (18 Ah Ni-Cd) provides power for eclipse phases. MetSat-1 has a design life of
7 years with an operational goal of 10 years.
The launch of MetSat-1 into GTO took place on Sept. 12, 2002 with ISRO's PSLV (Polar
Satellite Launch Vehicle) from the "Satish Dhawan Space Center, SHAR," India (initial
GTO of 220 km x 34500 km with 17.67º inclination). All post-launch spacecraft operations
and support activities are conducted by MCF (Master Control Facility) at Hassan located in
south-west India. The instrument data are acquired by the Meteorological Utilization Center in New Delhi.
Orbit: Geostationary orbit with a spacecraft position at 74º E longitude (first imagery was
received from VHRR/2 was received on Sept. 23, 2002; also GEO position was reached).
In-orbit performance evaluation of MetSat and its payload started on Sept. 24, 2002.
RF communication: The downlink frequency for the payload data is in C-band (4503.05
MHz) at data rates of up to 526.5 kbit/s. The EIRP is 18 dBW. A new element called planar
array antenna is used to transmit VHRR/2 and Data Relay Transponder (DRT) data.
Status of mission: Kalpana-1/MetSat-1 is operating nominally as of 2004.
Sensor complement: (VHRR/2, DRT)
VHRR/2 (Very High Resolution Radiometer), a modified version of VHRR heritage instruments flown on INSAT-2A, -2B, and -2E. The VHRR/2 observes in VIS, water vapor and
TIR bands providing a spatial resolution of 2 km in VIS band and 8 km for the rest. VHRR/2
was developed by SAC (Satellite Application Center), Ahmedabad, India. The instrument
operates in three scanning modes:
· Full frame mode (20º North-South x 20º East-West), minimum in about 33 minutes covering the entire Earth disk
· Normal frame mode (14º N-S x 20º E-W), minimum in about 23 minutes
· Sector frame mode in which the sector can be positioned anywhere in steps of 0.5º in the
N-S direction to cover 4.5º N-S x 20º E-W. This mode is particularly suited for rapid,
repetitive coverage during severe weather conditions like a cyclone.
The nominal frame repetition rates are: 40, 30 and 20 minutes respectively. VHRR/2 is an
optomechanical system. The incoming solar radiation is reflected onto a Ritchey-Chretien
telescope of 20 cm aperture by a beryllium scan mirror mounted at 45º to the optical axis.
The optical system includes a gold-film dichoric beam-splitter that transmits visible light
energy and reflects WV/TIR energy, so that the radiation from the Earth is channelized to
the visible and IR focal planes simultaneously. The visible band detector configuration consists of two staggered arrays of four silicon photodiodes each; while two sets of mercury-cadmium telluride detector elements operating nominally at 100-110 K sense the WV/thermal
radiation. The scan mirror is mounted on a two-axis, gimballed scan mechanism system to
generate a 2-D image by sweeping the detector instantaneous field of view (FOV) across the
Earth's surface in east to west (fast scan) and north to south (slow scan).
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Spectral band: VIS
Spectral band: TIR
Spectral band: MWIR (Water vapor)
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0.55 - 0.75 µm; Integrated out-of-band response <3%
Inter detector mismatch <5%
10.5 - 12.5 µm; Integrated out-of-band response <3%
Out-of-band response peak <0.1%
5.7 - 7.1 µm
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Spatial resolution VIS
Spatial resolution TIR and MWIR
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56 µrad (or 2 km x 2 km)
224 µrad (or 8 km x 8 km)
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Radiometric performance: SNR
Radiometric performance: NEDT
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>6 for VIS at 2.5% albedo
<0.25 K at 300 K for IR channel
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Dynamic range of TIR/MWIR channels
Dynamic range of VIS channel
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4-340 K
0-100%
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Misregistration between VIS and IR
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<56 µrad
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Modulation Transfer Function (MTF)
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>21% for IR and TIR; >23% for VIS channel
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Table 1: Specification of the VHRR/2 instrument
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Imaging mode
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Coverage
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Repeatability
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Full scan
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20º N-S and 20º E-W
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33 min
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Normal scan
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14º N-S and 20º E-W
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23 min
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Sector scan
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4.5º N-S and 20º E-W
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23 (3 times)
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Table 2: Imaging modes of the VHRR/2 instrument
Figure 3: Schematic illustration of the VHRR/2 instrument
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Channel
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No of detectors
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MTF (Modulation
Transfer
Function)
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Dynamic range
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Noise performance
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VIS
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4 +4 redundant
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>0.23 approx.
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0-100% albedo
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6 : 1 min at 2.5% albedo
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Water Vapor (WV)
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1 + 1 redundant
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>0.21 approx.
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4-340 K
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0.25 K at 300 K
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TIR
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1 + 1 redundant
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>0.21 approx.
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4-320 K
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0.5 K at 300 K
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Table 3: Design parameters of VHRR/2
DRT (Data Relay Transponder). DRT is part of a DCS (Data Collection System) of ISRO.
The objective is to collect data from unattended meteorological platforms in the ground
segment. DRT receives receives signals from unattended weather data collection platforms
and retransmits them to the central station. The data from these payloads are being used for
comprehensive weather status and forecasting.
RF communication of DRT: Uplink frequency = 402.75 MHz; downlink frequency =
4506.05 MHz; bandwidth = ± 100 kHz; EIRP = 21 dBW (min).
Note: MetSat-1 does not carry SAS&R (Satellite Aided Search and Rescue) system. In the
INSAT-2 series, the INSAT-2A and -2B satellites carried SAS&R transponders as well as
DRTs (Data Relay Transponders). According to ISRO information, INSAT-3A (launch
April 9, 2003) and INSAT-3D (to be launched subsequently), will carry SAS&R and DRT
payloads.
1) Information provided by S. Krishnamurthy of ISRO/HQ and by Killugudi S. Jayaraman of Bhopal, India
2) V. K. Kaila, A. S. Kirankumar, T. K. Sundaramurthy, S. Ramakrishnan, M. Y. S. Prasad, P. S. Desai, V. Jayaraman,
B. Manikiam, "METSAT - a unique mission for weather and climate," Current Science, Vol. 83, No 9, Nov. 2002,
pp.1081-1088
3) http://www.isro.org/rep2003/Webpgs/pg8.htm
4) V. K. Kaila, V. R. Katti, "METSAT - A Dedicated Meteorological Mission of ISRO," 4th IAA Symposium on Small
Satellites for Earth Observation, April 7-11, 2003, Berlin, Germany
5) S. K. Srivastav, S. Prasad, R. C. .Bhatia, D. Singh, V. R. Rao, "Current and Future Satellite Programs and Systems
in India," The 2003 EUMETSAT Meteorological Satellite Conference, Weimar, Germany, Sept. 29 - Oct. 3, 2003
6) http://www.isro.org/rep2004/Geostationary.htm
This description was provided by Herbert J. Kramer from his documentation of: "Observation of the Earth and Its Environment: Survey of Missions and Sensors" - comments and corrections to this article are welcomed by the author.
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