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X-ray Production. kVp KINETIC ENERGY OF ELECTRONS.

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Presentation on theme: "X-ray Production. kVp KINETIC ENERGY OF ELECTRONS."— Presentation transcript:

1 X-ray Production

2

3 kVp KINETIC ENERGY OF ELECTRONS

4 CATHODE MADE OF TUNGSTEN + 1%-3% THORIUM

5 TUNGSTEN Z # 74 MELTING POINT- 3,410 DEG. CELSIUS

6 THORIUM Z # 90

7 THERMIONIC EMISSION CATHODE HEATED UP TO AT LEAST 2,200 DEG. CELSIUS

8 ANODE TUNGSTEN TARGET

9 TUNGTEN AS TARGET HIGH Z# EFFICIENCY OF X-RAY PRODUCTION HIGH MELTING POINT –3,410 ° C– TARGET HEATED TO 2,000 ° C

10 X-RAY PRODUCTION BREMSSTRAHLUNG RADIATION CHARACTERISTIC RADIATION

11 BREMSSTRAHLUNG RADIATION If an incoming free electron gets close to the nucleus of a target atom, the strong electric field of the nucleus will attract the electron, thus changing direction and speed of the electron. The Electron looses energy which will be emitted as an X-ray photon. The energy of this photon will depend on the degree of interaction between nucleus and electron, i.e. the passing distance. Several subsequent interactions between one and the same electron and different nuclei are possible. X-rays originating from this process are called bremsstrahlung. Bemsstrahlung is a German word directly describing the process: "Strahlung" means "radiation", and "Bremse" means "brake

12 Bremsstrahlung Radiation

13 BREMS

14 DIFFERENT DEGREES OF DECCELERATION X-RAYS HEAT

15 BREMS RADIATION IS: POLYENERGETIC ! 90% OF X-RAYS ARE PRODUCED THROUGH BREMS INTERACTIONS WHEN KVP APPLIED

16 BREMS EMISSION- CONTINUOUS

17 The high energy electron can also cause an electron close to the nucleus in a metal atom to be knocked out from its place. This vacancy is filled by an electron further out from the nucleus. The well defined difference in binding energy, characteristic of the material, is emitted as a monoenergetic photon. When detected this X-ray photon gives rise to a characteristic X-ray line in the energy spectrum. Characteristic X-rays

18 Characteristic Radiation KE OF PROJECTILE ELECTRON > BINDING ENERGYORBITAL ELECTRON

19 CHARACTERISTIC CASCADE

20 TUNGSTEN-74 K-70 KEV L-12 KEV M-2.8 KEV BINDING ENERGIES OF DIFFERENT SHELL ELECTRONS

21 CHARACTERISTIC X-RAYS L K = 58 keV MK 70-3 = 67 keV M L 12-3 = 9 keV

22 TRANSFER OF ELECTRONS BETWEEN OUTER SHELLS RESULTS IN: HEAT PRODUCTION !

23 EACH CHARACTERISTIC RADIATION ( ex. K TO L TRANSFER) IS: MONOENERGETIC ! THERE ARE MANY CHARACTERISTIC RADIATION PRODUCED IN ONE ATOM THEREFORE CHARACTERISTIC RADIATION IS ALSO POLYENERGETIC !

24 CHARACTERISTIC EMISSION- LESS POLYENERGETIC!

25 X-RAYS PRODUCTION AN INEFFICIENT PROCESS 80 KVP 99.4% HEAT 0.6% X-RAYS

26 % EFFICIENCY OF X-RAY PRODUCTION % EFFICIENCY= K * Z * kVp K = 1 * 10 -4

27 X-RAY EMISSION ISOTROPICAL- IN EVERY DIRECTION

28 USEFUL RADIATION – PROJECTED TOWARD THE PATIENT

29 LEAKAGE RADIATION HOUSING

30 OFF-FOCUS RADIATION USEFUL OFF-FOCUS


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