[ Identification | Description | Input parameters | Links ]
ATHENA_1ring
InstrumentA 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
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 | 0.001 |
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" |
ATHENA_1ring.instr
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[ Identification | Description | Input parameters | Links ]
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