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Published byJulian Gorbet Modified over 10 years ago
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X-rays 10 12 10 6 10 3 10 1 10 -1 10 -3 Long Wave IR Visible UV X-rays Gamma rays wavelength (nm) Frau Röntgen's hand
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10 12 10 6 10 3 10 1 10 -1 10 -3 Long Wave IR Visible UV X-rays Gamma rays wavelength (nm) X-rays
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X-ray tube
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X-rays
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White radiation Produced upon "collisions" with electrons in target Any amount of energy can be lost up to a max. amount Continuous variation of wavelength Characteristic radiation Specific energies absorbed Specific x-ray wavelengths emitted Wavelengths characteristic of target atom type White radiation Produced upon "collisions" with electrons in target Any amount of energy can be lost up to a max. amount Continuous variation of wavelength Characteristic radiation Specific energies absorbed Specific x-ray wavelengths emitted Wavelengths characteristic of target atom type
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X-rays Mechanism Decelerating charges give off radiation Mechanism Decelerating charges give off radiation
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X-rays Mechanism Decelerating charges give off radiation Mechanism Decelerating charges give off radiation
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X-rays Mechanism Decelerating charges give off radiation Mechanism Decelerating charges give off radiation
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X-rays Mechanism Decelerating charges give off radiation Mechanism Decelerating charges give off radiation
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X-rays Mechanism Decelerating charges give off radiation Mechanism Decelerating charges give off radiation
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X-rays Typical tube spectrum
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X-rays - vary tube voltage Intensity Wavelength E ≈ hc/ Kedge E >> hc/ Kedge E > hc/ Kedge I conts = AiZV ~2 I char = Ai(V-V crit ) ~1.5
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X-rays More electron transitions
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X-rays Cu spectrum
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X-rays Al spectrum
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X-rays Au L spectrum
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X-rays Moseley's law - energy vs. atomic number
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X-ray sources Sealed tubes - Coolidge type common - Cu, Mo, Fe, Cr, W, Ag Sealed tubes - Coolidge type common - Cu, Mo, Fe, Cr, W, Ag Ka = (2 Ka1 + Ka2 )/3
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X-ray sources Sealed tubes - Coolidge type common - Cu, Mo, Fe, Cr, W, Ag intensity limited by cooling requirements (2-2.5kW) (~99% of energy input converted to heat) Sealed tubes - Coolidge type common - Cu, Mo, Fe, Cr, W, Ag intensity limited by cooling requirements (2-2.5kW) (~99% of energy input converted to heat)
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X-ray sources Intensity changes with take-off angle But resolution decreases with take-off angle
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X-ray sources
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Other X-ray sources Rotating anode high power - 40 kW demountable various anode types Rotating anode high power - 40 kW demountable various anode types
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Other X-ray sources Synchrotron need electron or positron beam orbiting in a ring beam is bent by magnetic field x-ray emission at bend Synchrotron need electron or positron beam orbiting in a ring beam is bent by magnetic field x-ray emission at bend Advantages 10 -4 - 10 -5 radians divergence (3-5 mm @ 4 m) Advantages 10 -4 - 10 -5 radians divergence (3-5 mm @ 4 m) high brilliance wavelength tunable high brilliance wavelength tunable
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Other X-ray sources Synchrotron Advantages 10 -4 - 10 -5 rad divergence (3-5 mm @ 4 m) high brilliance wavelength tunable Synchrotron Advantages 10 -4 - 10 -5 rad divergence (3-5 mm @ 4 m) high brilliance wavelength tunable
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Other X-ray sources Synchrotron need electron or positron beam orbiting in a ring beam is bent by magnetic field x-ray emission at bend Advantages 10 -4 - 10 -5 rad divergence (3-5 mm @ 4 m) high brilliance wavelength tunable high signal/noise ratio Synchrotron need electron or positron beam orbiting in a ring beam is bent by magnetic field x-ray emission at bend Advantages 10 -4 - 10 -5 rad divergence (3-5 mm @ 4 m) high brilliance wavelength tunable high signal/noise ratio
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X-ray sources Synchrotron Advantages 10 -4 - 10 -5 rad divergence (3-5 mm @ 4 m) high brilliance wavelength tunable Synchrotron Advantages 10 -4 - 10 -5 rad divergence (3-5 mm @ 4 m) high brilliance wavelength tunable
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X-ray sources Synchrotron Advantages 10 -4 - 10 -5 rad divergence (3-5 mm @ 4 m) high brilliance wavelength tunable Synchrotron Advantages 10 -4 - 10 -5 rad divergence (3-5 mm @ 4 m) high brilliance wavelength tunable
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Beam conditioning Collimation
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Beam conditioning Monochromatization -filters – materials have atomic nos. 1 or 2 less than anode 50-60% beam attenuation placing after specimen/before detector filters most of specimen fluorescence allows passage of high intensity & long wavelength white radiation Monochromatization -filters – materials have atomic nos. 1 or 2 less than anode 50-60% beam attenuation placing after specimen/before detector filters most of specimen fluorescence allows passage of high intensity & long wavelength white radiation X-rays detector filter specimen
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Beam conditioning Monochromatization -filters – materials have atomic nos. 1 or 2 less than anode 50-60% beam attenuation placing after specimen/before detector filters most of specimen fluorescence allows passage of high intensity & long wavelength white radiation Monochromatization -filters – materials have atomic nos. 1 or 2 less than anode 50-60% beam attenuation placing after specimen/before detector filters most of specimen fluorescence allows passage of high intensity & long wavelength white radiation
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Beam conditioning Monochromatization Crystal monochromators – LiF, SiO 2, pyrolytic graphite critical – reflectivity ex: for MoK , LiF 9.4% graphite 54 % Monochromatization Crystal monochromators – LiF, SiO 2, pyrolytic graphite critical – reflectivity ex: for MoK , LiF 9.4% graphite 54 %
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Beam conditioning Monochromatization Crystal monochromators – LiF, SiO 2, pyrolytic graphite critical – reflectivity ex: for MoK , LiF 9.4% graphite 54 % resolution – determines peak/bkgrd ratio & spectral purity best - Si – 10" graphite – 0.52° Monochromatization Crystal monochromators – LiF, SiO 2, pyrolytic graphite critical – reflectivity ex: for MoK , LiF 9.4% graphite 54 % resolution – determines peak/bkgrd ratio & spectral purity best - Si – 10" graphite – 0.52°
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Beam conditioning Monochromatization Monochromator shape usually flat – problems with divergent beams concentrating type – increases I by factor of 1.5-2 Monochromatization Monochromator shape usually flat – problems with divergent beams concentrating type – increases I by factor of 1.5-2
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