ͼ1£1 XRFÒÇÆ÷µÄÍâ¹ÛÌØÕ÷
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XÉäÏß¹âÔ´£º°×É«XÉäÏß¡£¼´¾ßÓи÷ÖÖ²¨³¤µÄXÉäÏߣ¬¿É·ÖÎöÇ°ÃæËùÁз¶Î§µÄËùÓÐÔªËØ¡£·ÅÉäÐÔÍ¬Î»ËØ¹âÔ´£º·ÅÉä³öµÄÉäÏßÒàÔÚXÉäÏß·¶Î§£¬µ«ÄÜÁ¿Êǹ̶¨µÄ¡£Òò´ËÖ»ÄÜ·ÖÎö²¿·ÖÔªËØ£¬ÒÇÆ÷µÄÌå»ý¿ÉÒÔºÜС£¬×îÐÂÐ͵ÄÏ൱ÓÚÒ»¸ö¼ÆËãÆ÷µÄ´óС¡£
ͬ²½·øÉä¹âÔ´£º¹âÔ´µÄÄÜÁ¿¸ü´ó£¬¶ÔºóÐøµÄ¶þ´ÎÉäÏß¼ì²âºÜÓÐÀû£¬ËùÒÔ·ÖÎö¾«¶È¸ü¸ß£¬µ« ÒÇÆ÷Ôì¼ÛºÜ°º¹ó¡£ 2 ·ÖÎöÔÀí When the atoms in a sample material are irradiated with high-energy primary x-ray photons, electrons are ejected in the form of photoelectrons. This creates electron 'holes' in one or more of the orbits, converting the atoms into ions - which are unstable£¨Figure 1£2(1)£©.
Figure 1£2 XRF·ÖÎöÔÀí(1)
To restore the atoms to a more stable state, the holes in inner orbits are filled by electrons from outer orbits. Such transitions may be accompanied by an energy emission in the form of a secondary x-ray photon - a phenomenon known as \£1(2)).
Figure 1£2 XRF·ÖÎöÔÀí(2)
The various electron orbits are called K, L, M, etc., where K is closest to the nucleus. Each corresponds to a different energy level - and the energy (E) of emitted fluorescent photons is determined by the difference in energies between the initial and final orbit for the individual transitions(Figure 1£3).
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Figure 1£3 Electron orbits K, L, M,
Characteristic x-ray emissions result in an energy spectrum that is a \£4). So we can determine the element kinds in the sample. And also the intensities of the peaks in the spectrum are roughly proportional to the concentrations of the constituent elements.
Figure 1£4 Characteristic x-ray emissions result
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²¨³¤É«É¢ÐÍXRF£ºWAVELENGTH DISPERSIVE XRF (WDS-XRF)
ͨ¹ý·ÖÎöÑùÆ·ÔÚÈëÉäXÉäÏß×÷ÓÃϲúÉúµÄ¶þ´ÎXÉäÏß(Ó«¹âÉäÏß)µÄ²¨³¤£¬À´¶¨ÐÔ»ò¶¨Á¿·ÖÎöÑùÆ·µÄÔªËØ×é³É¼°º¬Á¿¡£
ÄÜÁ¿É«É¢ÐÍXRF: ENERGY-DISPERSIVE XRF £¨EDS£XRF£© ͨ¹ý·ÖÎöÑùÆ·ÔÚÈëÉäXÉäÏß×÷ÓÃϲúÉúµÄ¶þ´ÎXÉäÏß(Ó«¹âÉäÏß)µÄÄÜÁ¿£¬À´¶¨ÐÔ»ò¶¨Á¿·ÖÎöÑùÆ·µÄÔªËØ×é³É¼°º¬Á¿¡£ WDS-XRF and EDS-XRF(ͼ1£5)
ͼ1£5 XRF¹¤×÷Á÷³Ì¿òͼ
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4 WDS-XRF Wavelength dispersive XRF uses a crystal to separate the various wavelengths: for every angle of incident radiation(ÈëÉä·øÉä), the only wavelength reflected to the detector is the one that conforms to Bragg¡¯s formula: n? = 2d sin ?
where ? is the wavelength of the x-ray radiation produced by the sample; d is a constant characteristic of every crystalline substance (i.e. the x-ray crystal); and ? is the angle on incidence of the x-radiation on the sample. The crystals and their planes often used are as follow£¨±í1£2£©.
±í1£2 ³£Óõķֹ⾧Ìå
How to determine the wavelength£¨Í¼1£6£©: Detector is rotating when doing the wavelength determination, also the crystal is rotating by half speed. So, by changing the angle of the crystal, you can select any wavelength for specific elements of interest.
Different crystal can be used determine different elements. When doing measurement, we often need to change crystals for the various elements, finally we can yield results in any form desired: qualitative, ratio, quantitative, graphic, etc.
The relationship between the range of analyzing element and the crystals, and the 2 theta scanning range£¨±í1£3£©.
ͼ1£6 ²¨³¤²â¶¨Ê¾Òâͼ
±í1£3 The relationship between the range of analyzing element and the crystals
Element range Ti22£U92 Al19£ Ti22 Mg12 Na11 ¡¢F9 ¡¢Mg12
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crystals LiF EDDT ADP TAP 2?scanning ranges 5¡ã£90¡ã 35¡ã£145¡ã 0¡ã£+3¡ã 5¡ã£+3¡ã Analyzing Procedure: Every element has a strongest X ray wavelength. In order to determine it, first we should measure the intensity of that wavelength.
For example, strongest Line and their 2? position for Ni, Fe, & Ru, when detected by different crystal£¨±í1£4£©.
±í1£4 Strongest Line and their 2? position for Ni, Fe, & Ru
In order to make the determination more accurate, we should also measure their accompanying peaks£¨±í1-5£©.
±í1£5 Ni, FeµÄKÏµÌØÕ÷
Analyzing Procedure£¨Í¼1£7£©:
ͼ1£7 ·ÖÎö³ÌÐò¿òͼ
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? WDS was introduced in the early 1950s.
? WDS spectrometer systems employ diffraction by a single crystal to separate characteristic wavelengths emitted
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