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IRS (Indian Remote Sensing Satellites) - Overview and early LEO Program of
ISRO
Following the successful demonstration flights of Bhaskara-1 and Bhaskara-2 - experimental Earth
observation satellites developed and built by ISRO (Indian Space Research Organization) - and
launched in 1979 and 1981, respectively, India began the development of an indigenous IRS (Indian
Remote Sensing Satellite) program. India realized quite early that
sustaining its space program in the
long run would depend on indigenous technological capabilities (in
particular, US export restrictions
made this clear). Keeping this in mind, besides building satellites,
India embarked as well on satellite
launch vehicle development in the early 1970s. As a consequence, India
has two very capable launch
systems at the start of the 21st century, namely PSLV (Polar Satellite
Launch Vehicle) and GSLV (Geosynchronous Satellite Launch Vehicle). 1)
IRS is the integrated LEO (Low Earth Orbit) element
of India's NNRMS (National Natural Resources
Management System) with the objective to provide a long-term spaceborne
operational capability to
India for the observation and management of the country's natural
resources (applications in agriculture, hydrology, geology, drought and
flood monitoring, marine studies, snow studies, and land use).
The intend of the program is to create an environment of new
perspectives for the Indian research community as a whole, to stimulate
the development of new technologies and applications, and to utilize
the
Earth resources in more meaningful ways.
Note: The INSAT system is India's GEO (Geosynchronous Earth Orbit) element, providing for simultaneous domestic communications and earth observation functions.
The IRS program started in the mid
1980s. Eventually, a continuous supply of synoptic, repetitive,
multispectral data of the Earth's land surfaces was obtained (similar
to the US Landsat program). In 1995,
IRS imagery was made available to a larger international community on a
commercial basis. The initial
program of Earth-surface imaging was extended by the addition of
sensors for complementary environmental applications. This started with
the IRS-P3 satellite which is flying MOS (Multispectral
Optoelectronic Scanner) for the measurement of ocean color. The IRS-P4
mission is dedicated to
ocean monitoring. 2) 3) 4)
Note: The availability of Landsat
imagery created a lot of interest in the science community. The
Hyderabad ground station started receiving Landsat data on a regular
basis in 1978. The Landsat program
with its design and potentials was certainly a great model and
yardstick for the IRS program.
• The first generation
satellites IRS-1A and 1B were designed, developed and launched
successfully during 1988 and 1991 with multispectral cameras with
spatial resolutions of 72.5 m and 36 m, respectively. These early
satellites were launched by Russian Vostok boosters from the Baikonur
Cosmodrome.
• Subsequently, the second generation remote sensing satellites IRS-1C and -1D with improved
spatial resolutions have been developed and successfully launched in 1995 and 1997, respectively.
IRS-1C/1D data has been used for cartographic and town planning applications.
|
Satellite
|
Launch
date
|
Sensor
complement
|
Spectral Bands
(µm)
|
Spatial
resolution (m)
|
Swath width
(km)
|
Repeat cycle
(days)
|
|
IRS-1A
|
17.03.1988
|
LISS-I, and
LISS-II A/B
(3 sensors)
|
0.45-0.52
0.52-0.59
0.62-0.68
0.77-0.86
|
72.5 m LISS-I
36 m LISS-II
|
148
74 x 2 (swath
of 148 km)
|
22
|
|
IRS-1B
|
29.08.1991
|
LISS-I and
LISS-II A/B
|
same as for
IRS-1A
|
|
148
74 x 2
|
22
|
|
IRS-P2
|
15.10.1994
|
LISS-II M
|
0.45-0.52
0.52-0.59
0.62-0.68
0.77-0.86
|
32 m x 37 m
|
66 x 2
(131 km for
combined
swaths)
|
24
|
|
IRS-1C
|
28.12.1995
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LISS-III
|
0.52-0.59
0.62-0.68
0.77-0.86
1.55-1.70
|
23.5
23.5
23.5
70
|
142
142
142
148
|
24
|
|
PAN
|
0.50-0.75
|
5.8
|
70
|
24 (5)
|
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WiFS
|
0.62-0.68
0.77-0.86
|
188
|
804
|
5
|
|
IRS-P3
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21.03.1996
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WiFS
|
0.62-0.68
0.77-0.86
1.55-1.70
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188
|
804
|
5
|
|
MOS-A
MOS-B
MOS-C
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0.75-0.77
0.41-1.01
1.595-1.605
|
1500
520
550
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195
200
192
|
Ocean surface
|
|
IXAE
|
Indian X-ray Astronomy Experiment
|
|
IRS-1D
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29.09.1997
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Satellite and instruments are identical to those of IRS-1C
|
|
IRS-P4
(OceanSat-1)
|
26.05.1999
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OCM
MSMR
|
0.4-0.9
6.6, 10.65, 18, 21
GHz (frequencies)
|
360 x 236
105x68, 66x43,
40x26, 34x22
(km for
frequency
sequence)
|
1420
1360
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2
2
|
|
IRS-P6
ResourceSat-1
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17.10.2003
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LISS-IV
|
0.52-0.59
0.62-0.68
0.77-0.86
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5.8
5.8
5.8
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70
|
24 (5)
|
|
LISS-III*
|
0.52-0.59
0.62-0.68
0.77-0.86
1.55-1.70
|
23.5
23.5
23.5
23.5
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140
|
24
|
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AWiFS
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0.62-0.68
0.77-0.86
1.55-1.70
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70
70
70
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740
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5
|
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IRS-P5
CartoSat-1
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05.05.2005
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PAN-F
PAN-A
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0.50-0.75
0.50-0.75
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2.5
2.5
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30
30
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2-line stereo
camera
|
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CartoSat-2
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10.01.2007
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PAN camera
|
0.50-0.85
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< 1
|
9.6
|
|
|
OceanSat-2
|
2008
|
OCM
SCAT
ROSA
|
0.40-0.90 8 bands
13.515 GHz
GPS occultation
|
360 x 236
25 km x 25 km
|
1420
1400
|
2
|
|
RISAT
|
2008
|
SAR
instrument
|
5.350 GHz
(C-band)
|
< 2 m to 50 m
|
100 - 600
|
|
|
Megha
Tropiques
(ISRO/CNES)
|
2009
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MADRAS
SAPHIR
ScaRaB
GPS-ROS
|
5 chan. radiometer
Atmos sounder
Radiation budget
Occultations
|
40 km x 60 km
|
1700
|
2
|
|
SARAL
(ISRO/CNES)
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2009/10
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AltiKa
DORIS
Argos-3
LRA
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35.75 GHz Ka-band altimeter
S/C tracking for POD services
Data collection system
Satellite laser ranging
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Table 1: Chronology of ISRO polar-orbiting imaging missions and instruments (starting with IRS series)
IRS-1A (Indian Remote Sensing Satellite-1A)
The spacecraft bus is box-shaped (1.6 m x 1.6 m x 1.5 m) with two solar panels (8.6 m2) as shown in
Figures 1 and 4.
The S/C structure is made of aluminum/aluminum honeycomb. The satellite
is three-axis stabilized utilizing a zero momentum system. Hydrazine
thrusters (80 kg fuel) are also used for
control and momentum dumping. The IRS series satellites are built
around a zero-momentum reaction wheel based system. Gyro-based attitude
reference using quaternion propagation with attitude
updates from Earth sensors and sun sensors (CCD-based is used for yaw
angle measurements) provide the high-pointing accuracy and stability
required for the imaging payload. Attitude is sensed by
Earth sensor, sun sensor, star sensor and dynamically tuned gyros. The
actuators are reaction wheels
(4), magnetic torquers, and hydrazine thrusters (sixteen 1-newton
thrusters). A pointing accuracy of
0.3º is achieved in pitch/roll and 0.5º in yaw. Attitude
determination accuracy of ±0.1º. Total S/C mass
= 975 kg (at launch), power = 700 W, two NiCd batteries (40 Ah) provide
power for the eclipse phase of
the orbit. The design life is three years. 5) 6) 7) 8) 9)
Figure 1: Illustration of the IRS-1A spacecraft (image credit: ISRO)
Launch: March 17, 1988 on a Russian launch vehicle Vostok-2M from the Baikonur Cosmodrome,
Kazhakstan.
Orbit: sun-synchronous orbit, nominal altitude = 904 km, inclination = 99.049º, period = 103.2 minutes; the repeat cycle = 22 days; equator crossing at 10:26 hours on descending node.
Application: Land use, agriculture, forestry, hydrology, soil classification, coastal wetland mapping,
natural resources (in particular pinpointing likely groundwater locations), disaster monitoring, cartography, etc.
RF communications: Payload
downlink in S-band and X-band. The satellite carried a real time
LISS-2A/B data downlink in X-band with a transfer rate of 10.4 Mbit/s
(2 links). The data was downlinked to a 10 m dish antenna at Shadnagar
on 20 W. The LISS-I data downlink was on 5 W S-band at
a rate of 5.4 Mbit/s. There was no onboard recorder. The payload data
were PCM/BPSK modulated.
The IRSO S/C control center is in Bangalore. TT&C function is provided by ISTRAC (ISRO Tracking
Network), supported by DLR (GSOC, Weilheim), NOAA (Fairbanks), ESA (Malindi) and the USSR
(Bearslake) ground stations.
Mission status: Spacecraft operations were ended in 1992.
Sensor complement:
LISS-I, -II (Linear Imaging
Self-Scanning Sensor), with a total of three cameras. LISS-I and
LISS-II are two multispectral camera assemblies, each with a different
resolution providing a swath of
about 150 km. Each LISS camera consists of the collecting optics,
imaging detectors, inflight calibration system, the processing
electronics, and data formatting electronics.
LISS-I employs four 2048-element
linear CCD detector arrays with spectral filters (Fairchild CCD
143A). All cameras use refractive type collecting optics with spectral
selection by appropriate filters.
The refractive optics were chosen to obtain a large FOV (Field of
View). A lens assembly for each spectral band is used for better
performance and effective utilization of the full dynamic range of the
CCDs.
Two LEDs (Light Emitting Diodes) per band are provided for inflight
calibration.
A LISS-I scene is 148 km x 174 km. The LISS-II A/B assembly features eight 2048-element linear
CCD detector arrays with spectral filters (2 parallel swaths of 74 km each for the LISS-II A/B assembly
with 3 km overlap, the total swath is 145 km). Four LISS-II scenes cover the area of one LISS-I scene.
10) 11) 12) 13)
|
Parameter
|
LISS-I
|
LISS-II A/B
|
|
Focal length
|
162.2 mm
|
324.4 mm
|
|
FOV, IFOV
|
9.4º, 80 µrad
|
4.7º+ 4.7º, 40 µrad
|
|
Spectral bands (µm)
|
0.46 - 0.52 (blue)
0.52 - 0.59 (green)
0.62 - 0.68 (red)
0.77 - 0.86 (NIR)
|
0.46 - 0.52 (blue)
0.52 - 0.59 (green)
0.62 - 0.68 (red)
0.77 - 0.86 (NIR)
|
|
Integration time
|
11.2 ms
|
5.6 ms
|
|
Ground resolution
|
72.5 m (each band)
|
36.25 m (each band)
|
|
Swath width
|
148 km
|
2 x 74 km
|
|
Radiometric resolution
|
7 bit
|
7 bit
|
|
Detector, elements
|
CCD, 2048
|
CCD, 2048
|
|
Data rate
|
5.2 Mbit/s
|
2 x 10.4 Mbit/s
|
|
Instrument mass, power
|
38.5 kg, 34 W
|
2 x 80.8 kg, 2 x 34 W
|
Table 2: Specifications of the LISS-I and -II instruments
Figure 2: Illustration of the LISS-I camera (image credit: ISRO)
Figure 3: Illustration of the LISS-II camera (image credit: ISRO)
IRS-1A data products are being acquired, processed and disseminated by NRSA (National Remote
Sensing Agency) Data Center, Hyderabad. These data products compete directly with Landsat TM and
MSS data as well as with SPOT Image data on the market.
IRS-1B (Indian Remote Sensing Satellite-1B)
IRS-1B is a follow-up satellite of IRS-1A. The IRS-1B spacecraft and instruments are practically
identical with those of IRS-1A (satellite mass = 975 kg).
Launch of the S/C was by a Russian
Vostok-2M vehicle from Baikonur on August 29, 1991 (same tracking
support configuration as for IRS-1A).
Orbit: Polar sun-synchronous orbit; altitude = 904 km, inclination = 99.49º, period = 103.2 minutes.
Repeat cycle: 22 days.
ISRO's policy allows ground stations from other countries to have direct access to the Indian satellite
imagery. Any existing ground station equipped to receive data from SPOT or from Landsat will be able
to receive IRS-1B satellite data with very minor changes (ISRO can supply the upgrade). 14) 15)
Figure 4: Line drawing of the IRS-1B spacecraft
Mission status: The IRS-1B satellite far outlived its design live of 3 years - being operational on its
10th anniversary after launch (Aug. 29, 2001). 16)
Afterwards, the S/C was being used for conducting various experiments including studying the design
margins of the various subsystems and to test different modes of operation using the available fuel.
IRS-1E (Indian Remote Sensing Satellite-1E), (P1)
A technological mission with the primary objective to test an ISRO-developed launch vehicle by the
name of PSLV-D1 (Polar Satellite Launch Vehicle-Developmental flight 1). The IRS-1E spacecraft
is a modified IRS-1A engineering model. 17)
Launch: The launch occurred on Sept. 20 1993 from SHAR (Sriharikota Launching Range, Andhra
Pradesh, ISRO's main launch site, India, located on India's east coast at 13.57º N, 80.293º E, about 100
km north of Chennai). Unfortunately, the satellite failed to achieve orbit (PSLV failure of 2nd stage, a
newly developed launch vehicle of ISRO - the PSLV control software prevented attaining orbit). The
mission ended in the ocean.
Nominal orbit: Sun-synchronous polar orbit with equatorial crossing at 10:30 AM on descending
node, altitude = 904 km, period = 103 min, repeat cycle = 22 days.
Sensor complement: (LISS-I, MEOSS)
LISS-I (Linear Imaging Self-Scanning System). Same definition as under IRS-1A.
MEOSS (Monocular
Electro-Optical Stereo Scanner), a DLR (Germany) experimental sensor
with
pushbroom CCD technology. MEOSS is a stereo camera system capable of
recording three images simultaneously with a single lens by means of
linear scanning (3-line stereo system). MEOSS has a
single lens with a focal length of 61.6 mm and 3 CCD line sensor arrays. Each CCD array comprises
3236 sensor elements with 10.7 µm in size. The scanner operates in the spectral range of 0.57-0.7 µm.
Resolution = 50 m along track, 158 m in cross-track, 45 m in vertical direction; swath width = 510 km,
8 bit quantization. Application: stereo view capability to study topography, geology, terrain analysis
and modeling, snow/ice mapping, meteorology (cloud height and movement), etc. 18) 19) 20) 21)
The
MEOSS concept had already been demonstrated on an airborne platform of
DLR in 1986 and in
1989. Prior to the IRS-1E flight, MEOSS was also launched on the
SROSS-2 (Stretched Rohini Satellite Series) mission of ISRO (July 13,
1988 on ISRO's ASLV launcher). However, SROSS-2 experienced also a
launcher failure.
|
Number of linear CCD arrays
|
3
|
|
Nominal focal length nadir/stereo
|
61.6 mm
|
|
CCD element size
|
10.7 µm
|
|
Number of active pixels per array nadir/stereo
|
3236
|
|
Stereo angle
|
±23.5º
|
Table 3: Some basic characteristics of the MEOSS instrument
Figure 5: Observation geometry of the MEOSS 3-line stereo camera (image credit: DLR)
IRS-P2 (Indian Remote Sensing Satellite-P2)
An ISRO mission with the objective
to acquire remote sensing data for oceanographic, land, and atmospheric
applications (demonstration of the IRS-1C/1D bus). The spacecraft is
three-axis stabilized
using conically scanning Earth sensors and dynamically tuned gyros for
attitude sensing, and reaction
wheels, magnetic torquers and monopropellent hydrazine thrusters as
actuators. Inertial attitude referencing with the star sensor updates
is one of the major ISRO developments for astronomical X-ray
observations. The attitude control system of IRS-P2 provides
multipurpose functions by pointing for
remote sensing, and inertial pointing for the X-ray observations. S/C
mass = 870 kg, solar power = 510
W, two 21 Ah NiCd batteries. 22)
Launch: October 15, 1994 from SHAR (Sriharikota Launching Range) with a PSLV-D2 launcher. A
major objective of this launch was to demonstrate/qualify the newly developed launch vehicle PSLV
(Polar Satellite Launch Vehicle) of ISRO. This time around, the PSLV functioned correctly, allowing
IRS-P2 to assume its orbit.
Orbit: Sun-synchronous circular
orbit with an equatorial crossing at 10:30 AM descending node, altitude
= 817 km, inclination = 98.7º, repeat cycle = 24 days, period = 101.35 min.
RF communications: No onboard data storage capability. Downlink broadcast of R/T science data in
X-band (8.316 GHz, PCM/QPSK/PM modulation, data rate = 2 x 10.4 Mbit/s) to a dedicated ground
station network and to a general user community. TT&C operations in S-band.
Mission status: The IRS-P2 spacecraft continued in operations until September 1997. 23)
Sensor complement:
LISS-IIM (Linear Imaging Self-Scanning System-II Modified). Same definition as under IRS-1A.
The LISS-IIM instruments (there are two just as LISS-II A/B) are realized with a single optical feed
utilizing the full ±5º FOV (there are 4 lenses in one optical head). The instrument employs pushbroom
scanning and a linear CCD line detector array with 4 spectral bands in VNIR (0.45-0.52 µm,
0.52-0.59 µm, 0.62-0.68 µm, 0.77-0.86 µm. Focal length = 324.4 mm. The ground resolution is 32 m
(cross-track) x 37 m (along-track). The combined swath is 131 km. The instrument mass is 80.8 kg (x
2), the instrument power is 34 W (x 2).
1) P. Kumar Sangatramani, K. Sangatramani, "India in Space - 2020," 2003,
http://www.bharat-rakshak.com/MONITOR/Space%20Essay/entry5.htm
2) G. Joseph, B. L. Deekshatulu, "Evolution of Remote Sensing in India," Space in Pursuit of New Horizon, National Academy of
Sciences publication, (editor: R. K. Verma and others), Allahabad, 1992, pp. 331-354
3) K. Kasturirangan, G. Joseph, et al., "IRS Mission," Current Science, Vol. 61, No. 3 and 4, Aug. 25, 1991, pp. 136-151
4) P. S. Goel, "Spacecraft Technology Development in India," Space Forum, Vol. 5, No 1-3, 2000, pp. 5-38
5) "Indian Remote Sensing Satellite and Associated Data Products," A.K.S. Gopalan, Proceedings of the Twenty-Third International
Symposium of Remote Sensing of the Environment, Vol. I, p. 71, ERIM, Ann Arbor, MI, 1990
6) IRS NewsLetter, ISRO, Vol. 2 No. 1, March 1991
7) http://ceos.cnes.fr:8100/cdrom-98/ceos1/isro/eospro/irs1b.htm
8) http://www.nrsa.gov.in/satellites/irs-1a.html
9) http://www.geocities.com/indian_space_story/irs1b.html
10) G. Joseph, IRS-1A Camera - Its Evolution and Realization," brochure of NNRMS (National Natural Resources Management
System), Bangalore, India
11)
Note: At the time of project initiation, CCD arrays with maturity of
production were limited to 2048 elements. Hence the swath of
LISS-I was limited to about 150 km. Since LISS-II has a better
resolution by a factor of two compared to the LISS-I camera, two
LISS-II cameras were needed to produce a swath similar to that of
LISS-I.
12) J. Kirshnamurthy, A. S Padmavathy, V. Jayaraman, Uday Raj, "Inter Sensor Comparison of Indian Remote Sensing Satellite - 1A
Linear Imaging Self Scanning Sensors for Radiometric behavior," ACRS (Asian Conference on Remote Sensing) 1991, Oct.
30-Nov. 5, 1991, Singapore, http://www.gisdevelopment.net/aars/acrs/1991/mapfs/mapfs04pf.htm
13) http://www.csre.iitb.ac.in/isro/irs-1b.html
14) "India Expands Access to Imagery," Space News Aug. 26 - Sept. 8, 1991, p. 22
15) "India Calls IRS-1B Launch a Success," Space News, September 9-15, 1991, p. 12
16) "IRS-1B Completes 10 years of Remote Sensing Mission," Aug. 29, 2001, URL: http://asia.spaceref.com/news/viewpr.html?pid=5875
17)
Note: The satellite designations P1, P2, P3, etc. stand for the
launches carried out by the PSLV (Polar Satellite Launch Vehicle),
the launch vehicle developed by ISRO
18) IRS-1E MEOSS Utilization Plan, ISRO, July 1991
19)
F. Lanzl, "The Monocular Electro-Optical Stereo Scanner (MEOSS)
satellite experiment," ISPRS Vol. 26-I, pp. 617-620, Stuttgart, 1986
20) M. Lehner, "Triple stereoscopic imagery simulation and digital image correlation for Monocular Electro-optical Stereo Scanner
(MEOSS) project," ESA Proceedings of the International Symposium on Progress in Imaging Sensors, Nov. 1986, pp. 477-484
(SEE N87-24738 18-43)
21) F. Lanzl, "The Monocular Electro-optical Stereo Scanner (MEOSS) satellite experiment," 38th IAF (International Astronautical
Congress), England, Oct. 10-17, 1987
22) Document on Configuration of IRS-P2 and MOS and their Interfaces, ISAC, Bangalore, Nov. 1992
23) http://www.geocities.com/indian_space_story/irs.html
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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