The Salyut 4 Space Station
Mission OverviewThe Salyut-4 space station was launched on 26 December 1974. It was in an orbit with an apogee of 355 km and a perigee of 343 km. The orbital period was 91.3 minutes. It was at an inclination of 51.6 degrees. The X-ray telescope was switched on on 15 January 1975. Salyut-4 reentered the Earth's atmosphere on 2 February 1977.
InstrumentationThe Salyut-4 X-ray instrument, often called the Filin telescope, consisted of four gas flow proportional counters, three of which have a total detection surface of 450 sq cm in the energy range 2-10 keV, and one of which has an effective surface of 37 sq cm for the range 0.2-2 keV. The field of view was limited by a slit collimator to 3 deg x 10 deg FWHM. The instrumentation also included optical sensors which were mounted on the outside of the station together with the X-ray detectors, and power supply and measurement units which were inside the station. Ground based calibration of the detectors is considered along with in-flight operation in three modes: inertial orientation, orbital orientation, and survey. Data could be collected in 4 energy channels: 2-3.1 keV, 3.1-5.9 keV, 5.9-9.6 keV, and 2-9.6 keV in the larger detectors. The smaller detector had discriminator levels set at 0.2 keV, 0.55 keV, and 0.95 keV.
ScienceAmong others, observations of Sco X-1, Cir X-1, Cyg X-1, and A0620-00 were published from the Filin data. A highly variable low energy (0.6-0.9 keV) flux was detected in Sco X-1. Cir X-1 was not detected at all during a 5 July 1975 observation, providing an upper limit on the emission of 3.5e-11 erg/sq-cm/s in the 0.2-2.0 keV range. Cyg X-1 was observed on several occasions. Highly variable flux, in both the time and energy domains, was observed.
Page authors: Lorella Angelini Jesse Allen HEASARC Home | Observatories | Archive | Calibration | Software | Tools | Students/Teachers/Public Last modified: Thursday, 26-Jun-2003 13:48:17 EDT HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details. |