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About McXtrace Documentation |
[ Identification | Description | Input parameters | Links ] The
Single shell model of the NuSTAR-optic in use as telescope.
|
Name | Unit | Description | Default |
FL | m | The focal length of the optical system | 10.12 |
FLd | m | The distance from the optics centre to the detector. If 0 the detector is placed at the focal plane. | 0 |
optics_dist | m | The distance between souce and optic. In space this would be quite large :-). | 10 |
offaxis_angle | arcmin | Angle of collimated light from source | 0 |
drx | arcsec | Rotation of shell along X | 0 |
dry | arcsec | Rotation of shell along Y | 0 |
drz | arcsec | Rotation of shell along Z | 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 | The row number for the miror module. This defines the shell. | 0 | |
parabolic_datafile | File which contains the geometry of the parabolic (primary) mirrors. (i.e. radii,lengths) | "om_con_1a_110901_t1.txt" | |
hyperbolic_datafile | File which contains the geometry of the hyperbolic (secondary) mirrors. (i.e. radii,lengths) | "om_con_3a_110901_t1.txt" |
NuSTAR_1shell.instr
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[ Identification | Description | Input parameters | Links ]
Generated for mcxtrace 3.5.24