Indian Space Program

Home
Brief History
Space Programme
Satellite Program
Launcher Program
Indian Cosmonaut
ISRO
 
Web Search
Google
A story of Indian Space Program
Satellites: : Aryabhata | APPLE | INSAT-1 | INSAT-2 | INSAT-3 | Bhaskara | IRS | Rohini

Launcher : : SLV | PSLV | ASLV | GSLV

Rohini Series (Click here to see the image)

(Launched by Indian launch vehicle SLV-3 )

Rohini 1A :

Launching tried by SLV-3 rocket, on 10 August, 1979, made by India, from Shriharikota. Rocket failed.

Rohini 1B

Launch Date : July 18, 1980

Weight : 35 kg

Orbit : 300 km x 900 km elliptical orbit (97 minutes period)

Lauched by : India, SLV-3 rocket

Objectives : The satelite provided data on the fourth stage performance and ranging.

Rohini-2

Launch Date : May 30, 1981

Weight : 35 kg

Lauched by : India, SLV-3 (D-1) rocket

Orbit : 300 km x 900 km elliptical orbit (97 minutes period)

Objectives : Carried a Land Mark sensor payload whose solid state camera performed to specifications. The satellite re-entered the earth's atmosphere nine days after lauch on account of the launch vehicle's injecting the satellite into a lower than expected altitude. However the orbit achieved was 186x418km instead of the planned 296x834km, leading to re-entry after eight days.

Rohini-3

Launch Date : April 17, 1983

Weight : 35 kg

Lauched by : India, SLV-3 (D-2)rocket

Orbit : 300 km x 900 km elliptical orbit (97 minutes period)

Objectives : The Smart Sensor Camera was the primary payload on board the satellite. It was operated for over five months and sent more than 2500 pictures frames in both visible and infrared bands for identification of landmarks and altitude and orbit refinement. The camera had on-board processing capability to use the data for classifying ground features like water, vegetation, bare land, clouds and snow. After completing all its mission goals, RS-D2 was closed down on Sept. 24, 1984. It re-entered orbit on 19 April 1990.

SROSS - Stretched Rohini Satellite Series

ISRO developed the Stretched Rohini Satellite Series (SROSS) for conducting various scientific experiments as well as for new and novel application-oriented missions. The first two satellites in the series did not make it into orbit due to launch vehicle failure. The third, SROSS-3, successfully attained an orbit on 20 May 1992.

Although they decayed rapidly, the orbital parameters were initially; apogee was 430km, perigee was 255km, and the orbital inclination was 46º. The satellite spin period was 10.6 sec. The satellite carried a gamma-ray burst (GRB) experiment and a retarded potential analyzer (RPA) payload. It re-entered orbit on 14 July 1992.

Instrumentation: The gamma-ray burst experiment was operated from 25 May 1992 until re-entry on 14 July 1992. The instrument consisted of a main and a redundant CsI(Na) scintillator operating in the energy range 20-3000 keV. The crystals were 76mm (main) and 37mm (redundant) in diameter. Each had a thickness of 12.5mm.

A 'burst mode' was triggered by the 100-1024 keV count rate exceeding a preset limit during a 256 or 1024 milliseconds time integration. In this mode, 65 seconds of temporal and 2 seconds of spectral data prior to the trigger are stored, as well as the subsequent 16 seconds of spectral data and 204 seconds of temporal data.

The low resolution data consists of two energy channels (20-100 keV and 100-1024 keV) from 65 seconds before the trigger to 204 seconds after the trigger in 256 milliseconds integrations. The 20-1024 keV rates are also recorded with a two milliseconds resolution for one second, prior to a one second after trigger and a 16 milliseconds resolution for one second prior to 8 second after the trigger. Energy spectra are conducted with a 124 channel PHA. Four pre-trigger spectra and 32 post-trigger spectra are recorded for every burst with a 512 millseconds integration time.

Science: During the mission lifetime, 53 triggers occurred. Most of these, as expected, were false. There were eight candidates for real bursts. One event, on 22 of June was also seen by CGRO and is believed real. Two other events could be real, as CGRO was not recording data at the time and so could not corroborate their occurrence.

Sources and Resources

  • Other source : www.bharatrakshak.com
   

Copyright Indian_Space_Program @2000