next up previous contents
Next: Effective Area and Telescope Up: The SODART Mirror Modules Previous: The SODART Mirror Modules

Introduction

The SODART Mirror Modules, designated FM1 & FM2, are two identical, multiply-nested, thin-foil telescopes. The mirror surfaces are conical approximations to a Wolter 1 geometry telescope, and are designed for moderate on-axis spatial resolution and high throughput above $\sim $6 keV. The mirrors are assembled in quadrants and then attached to a support structure to form a complete mirror.

Parameters for each unit are listed in Table 2, and the available instrumentation is listed in Table 3.


 
Table 2: Mirror Module Parameters
 
Field of View (diameter) 60 $^{\prime}$
Half Power Diameter 2.5-3 $^{\prime}$
Focal Length 8 m
Inner Shell Diameter 16.32 cm
Outer Shell Diameter 60 cm
Reflecting surface 350 Å gold
Shell material 0.4 mm aluminum
Shell separation (min) 0.52 mm
Shell length 20 cm
Number of shells 143
Mass per telescope 101 kg
Total mirrored surface 62 m2
 


 
Table 3: Mirror Module Instrumentation
 
FM1 FM2
LEPC-1 LEPC-2
HEPC-1 HEPC-2
KFRD-1 KFRD-2
SIXA SXRP
  OXS
 

Pre-flight calibration of the mirrors has been conducted at the Expanded Beam X-ray Optics Facility at the Daresbury Synchrotron, and is described in detail in Christensen et al. (1997). Their results are summarized here.


next up previous contents
Next: Effective Area and Telescope Up: The SODART Mirror Modules Previous: The SODART Mirror Modules
Tomas P. Girnius
1999-01-21