LEG 1st order distance = 5366.55*(12.398/1.486)/9921 = 4.513 mm From first-light HSI image measured: 4.513 mm (!)
8/24/96: Herman makes progress on it: "Brad Wargelin reports in his 2nd floor shift report that the dispersion distance [for 5th order MEG - dd] was found to be 55.933 mm from 0th order [I assume this is along-dispersion-axis distance and not Y-axis-only distance - dd] and that the image was at an angle of 3.96 degrees from the horizontal. If this angle is added to the estimate of the stage to dispersion angle, one gets an angle of 4.81 degrees as the angle between the LETG and MEG dispersion directions, which is within the tolerances (5.0 deg +/- 0.5 deg). The period of the MEG is then estimated to be 4000.92 A [? see calculations below - dd], which is within the tolerances of the expected period, which is 4000.72 ."
Grating equation for normal incidence: lambda sin ( theta_diffraction ) = m x -------- p for flat focal surface: dispersion distance theta_diffraction = atan ( --------------------- ) Rowland diameter Rowland diameter for TMA/TOGA is 5366.55 mm based on measurements and TMA focal length. LEG Period (first-light data) ----------------------------- sin ( atan(4.513/5366.55) ) = 1 x (12.398/1.486)/p p = 9921.17 A (LEG sub-assembly period = 9921.36) MEG Period (fifth-order MEG data) ----------------------------- sin ( atan(55.933/5366.55) ) = 5 x (12.398/1.486)/p p = 4002.70 A (MEG-TOGA sub-assembly period = 4000.72 +/- 4A)
Note that we're getting into the regeme where knowing the 12.398 AkeV factor and the X-ray line energy (1.486 keV) to the 0.1% level is required!
8/28/96: Dan writes: Based on beam-centering measurements of the LEG, MEG, and HEG +-1 and 0 orders the following parameters should accurately predict the location of TOGA grating images:
Grating Roll angle Period LEG -0.9073 deg 9915.7 A MEG 3.9489 deg 4004.5 A HEG -5.9974 deg 2002.3 A
The periods are based on Al-K measurements and constants used are: 12.398 AkeV, 1.486 keV, 5366.55 mm. These values will be used to update the awk script (rehearsal.pl ?) that produces detector locations for measurements at rehearsal. The angles of roll are positive moving from facility Y axis towards the facility Z axis.