Single pore version of the ATHENA SPO-optic in use as telescope.
Identification
Site: AstroX_ESA
Author: Erik B Knudsen & Desiree D. M. Ferreira (email)
Origin: DTU Physics/DTU Space
Date: 12/12/2016
Description
A model of the ATHENA-telescope using a single ring as optical element. That means to make use of this instrument
it is necessary to run a series of simulation while varying the input parameter porenumber.
At present, the porenumber really means ring number.
The model needs as input a file geomfile, which contains (in ascii) tabled details about the geometry of the shells.
The data in the geomfile is assumed to be in the format:
#row L/m rad_h/m rad_m/m rad_p/m width/m
...
row: running index for the rows/rings
L: The length of the plates for this ring
rad_h: The radius at the "hyperbolic" end of the optic. At the detector end.
rad_m: The radius at the midpoint of the optic. This is the reference.
rad_p: The radius at the "parabolic" and of the optic. At the source end.
width: pore width ?
Example: ATHENA_1ring.instr shellnumber=3
Input parameters
Parameters in boldface are required;
the others are optional.
Name
Unit
Description
Default
FL
m
The focal length of the optical system
12
optics_dist
m
The distance between souce and optic. In space this would be quite large :-).
10
SRC_POS_X
m
Displacement of source along X
0
SRC_POS_Y
m
Displacement of source along Y
0
offaxis_angle
arcmin
Angle of collimated light from source
0
reflectivity
Data file containing reflectivities (such as from IMD)
"mirror_coating_unity.txt"
E0
keV
Central energy of X-rays
5
dE
keV
Half spread of energy spectrum to be emitted from source