14.8 The Ring_c McXtrace Component
Date: Feb. 2017 Version: 1.1 Release: McXtrace 1.2 Origin: DTU Physics, DTU
Space
Stack of conical shells as part of a Wolter optic.
Identification
Description
A stack of conical shells is simulated. To intersect the Wolter I plates we take advatage of
the azimuthal symmetry and only consider the radial component of the photon’s
wavevector.
Input parameters
Parameters in boldface are required; the others are optional.
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Name |
Unit |
Description |
Default |
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ring_nr |
1 |
Ring number; selects the data block read
from size_file |
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radius_m |
m |
Ring radius of the upper (reflecting)
plate of the shell at the optic centre. |
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|
Z0 |
m |
Distance between optics centre plane and
focal spot (essentially focal length). |
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xwidth |
m |
Currently not used by the component |
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yheight |
m |
Height of the shell. |
|
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gap |
m |
Gap between the
plate and the intersection plane with the
hyperbolic section. (currently ignored) |
0 |
|
chamferwidth |
m |
Width of side walls. |
0 |
|
length |
m |
Length along the optical axis |
0 |
|
mirror_reflec |
|
Data file containing reflectivities of the
reflector surface (TOP). |
”” |
|
bottom_reflec |
|
Data file containing reflectivities of the
bottom surface (BOTTOM). |
”” |
|
R_d |
|
Default reflectivity value to use if no
reflectivity file is given. Useful f.i. is
one surface is reflecting and the others
absorbing. |
1 |
|
primary |
|
If non-zero, the shell is considered a
primary reflector, and extends towards
negative z. I.e. the entry plane is behind
the z=0-plane. If zero, the shell is
considered secondary and extends from
the z=0-plane and towards positive z. |
1 |
|
dalpha |
deg |
Offset to the alpha angle computed from
the focal length. Useful for targeting
the modified conical geometry (currently
ignored). |
0 |
|
waviness |
rad |
Waviness of the shell reflecting surface.
The slope error is assumed to be
uniformly distributed in the interval
[-waviness:waviness]. |
0 |
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longw |
|
If non-zero, waviness is 1D and along the
shell axis. |
0 |
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