The SPEKTROSAT mission
Abstract
SPEKTROSAT, the follow-up mission to ROSAT will be equipped with a transmission grating spectrometer with a spectral resolution of 0.2 A over the wavelength range between 6 and 300 A. Third-order aberrations are minimized by a mounting of the grating elements according to the Rowland-torus geometry. The ROSAT mirror system will be slightly changed by a redesign of the optical stops in order to reduce the field of view. The Focal Instrumentation has to be modified for a better match with the spectroscopic requirements. Since SPEKTROSAT is almost identical to ROSAT, this concept offers a large amount of science at relatively low costs. Its limiting line sensitivity will be about 20 times better than that of the EINSTEIN-OGS.
- Publication:
-
IAU Colloq. 115: High Resolution X-ray Spectroscopy of Cosmic Plasmas
- Pub Date:
- 1990
- Bibcode:
- 1990hrxr.conf..295P
- Keywords:
-
- Astronomical Spectroscopy;
- Rosat Mission;
- Satellite Instruments;
- Spaceborne Astronomy;
- X Ray Astronomy;
- Field Of View;
- Mirrors;
- Sky Surveys (Astronomy);
- X Ray Sources;
- Astronomy