[ Identification | Description | Input parameters | Links ]

The ATHENA_1ring Instrument

Single pore version of the ATHENA SPO-optic in use as telescope.

Identification

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.
NameUnitDescriptionDefault
FLmThe focal length of the optical system12
optics_distmThe distance between souce and optic. In space this would be quite large :-).10
SRC_POS_XmDisplacement of source along X0
SRC_POS_YmDisplacement of source along Y0
offaxis_anglearcminAngle of collimated light from source0
reflectivity Data file containing reflectivities (such as from IMD)"mirror_coating_unity.txt"
E0keVCentral energy of X-rays5
dEkeVHalf spread of energy spectrum to be emitted from source0.001
shellnumber Actually the ring number.1
ringfile File which contains details for the meta shells."ref_design_breaks.txt"
geomfile"ATHENA_rings_1_20.dat"

Links


[ Identification | Description | Input parameters | Links ]

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