PHYS01200804001 Sohrab Abbas - Homi Bhabha National Institute
PHYS01200804001 Sohrab Abbas - Homi Bhabha National Institute
PHYS01200804001 Sohrab Abbas - Homi Bhabha National Institute
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Fig.37 Bragg reflection from the θ S =53.5 o monochromator observed with prism diffraction (cf.<br />
inset) of the optimal analyser.<br />
alignment of the analyser whose Bragg reflection as well as prism diffraction were monitored<br />
(Fig.38). The analyser rocking curve yielded the expected ~ 3.1 arcsec wide peak (circles) with a<br />
peak intensity of about 468 neutrons/s. The monochromator was then translated to illuminate the<br />
analyser with its prism diffraction alone. The corresponding analyser rocking curve of ~ 2.5 arcsec<br />
FWHM (cf. Fig.39) agrees well with theory (smooth blue curve), displaying a peak intensity of<br />
68.5 neutrons/s, After optimising the analyser alignment, the Cd sheet before the detector was<br />
translated to stop Bragg reflected neutrons from the analyser. With these Bragg prism diffractions,<br />
the analyser tilt adjustment became even more critical and had to be made in 0.9 arcsec steps, since<br />
prism diffraction peaks are narrower and sharper than the Bragg reflections. The rocking curve<br />
(Fig.40) consisting of a pair of 0.62 arcsec wide peaks separated by 2.2 arcsec (squares), is in fair<br />
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