electromagnetic waves and x-ray creation Flashcards

1
Q

gamma rays (10^-12m - 10^-16m)

A
  • highest energy photons and have extremely short wavelength
  • generated by changes in energy levels of the nucleus of atom
  • used in nuclear medicine and PET scans
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2
Q

x-rays

A
  • 10^-10m
  • high energy photons
  • generated by deceleration of fast moving e-s
  • generated by changed in energy of innermost orbital e-s of atoms
  • gamma n x are detected by photography, ionisation chamber and phosphorescence
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3
Q

properties of gamma and x

A
  • penetrate matter
  • ionise gas (remove e-s)
  • cause fluorescence
  • photoelectric emissions from metals
  • reflected and diffracted by crystals
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4
Q

uv radiation

A
  • 10^-8 m - 10^-9 m
  • detected with light sensitive circuits (CCDs, photography and fluorescence
  • absorbed by glass
  • causes chem reactions e.g sun damage- skin damage
  • the ionosphere, ayer high in atmosphere, was created by UV radiation from sun ionising atoms in this layer
  • generated by orbital e-s of atoms
  • also by sun and generated mercury vapour lamps
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5
Q

infrared radiation

A
  • 10^-6m
  • generated by outer e-s in atoms and molecules and changes in vibrational and rotational energies of molecules (all bonds between atoms vibrate and the freq of vibrations is characteristic of atomic bones involved
  • makes colourful images depicting elevated skin temp
  • night sights use IR radiation, thermal cameras
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6
Q

microwaves

A
  • 10^-4 m - 10^-1m
  • emerging biomedical imaging modality
  • noninvasive assessments of functional and pathological conditions of soft tissue
  • ultrawide band microwave imaging is promising method for detection of breast cancer
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7
Q

radio waves

A
  • 10^3m
  • astronomy
  • MRI
  • communication
  • generated by oscillating e-s in special circuits to radioactive aerials (the transmitter)
  • tuned oscillatory circuit (radio receiver)
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8
Q

electromagnetic waves

A
  • single frequency EM wave exhibit a sinusoidal variation of electric and magnetic fields in space
  • magnetic variation is perpendicular to electric field
  • EM waves travel in straight lines
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9
Q

electromagnetic wave description

A
  • sinusoidal wave
  • amplitude- height of wave
  • wavelength- length of one cycle
  • frequency- cycles per second
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10
Q

electromagnetic wave equation

A

c=f x lambda

c= speed of wave (ms-1)
f= frequency (Hz)
lambda= wavelength

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11
Q

energy of electromagnetic radiation equation

A

E= h x f
h= plancks constant (6.626x10^-34)
f= frequency

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12
Q

photon

A
  • think of light as a series of particles or photons
  • elementary particle
  • em radiation therefore consists of discrete quantises packets of energy which we call photons
  • no mass, no electric charge and does not decay spontaneously
  • consists of oscillating electric field component E and oscillating magnetic field component B
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13
Q

inverse square law

A
  • expresses the way radiation energy propagates though space
  • E= I / r^2
  • E= energy
  • I= radiation intensity
  • r= distance from source
  • rule states that the “power intensity per unit area from a power source, if the rays strike the surface at a right angle, varies inversely according to the square of the distance of the source”
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14
Q

x-ray creation

A

there are 2 types of interactions of electrons with the anode target produce radiation
1. interaction with the atomic nucleus produce bremsstrahung x-ray photons
2. interaction with e- shells which produces characteristic x-ray photons

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15
Q

bremsstrahlung spectrum

A
  • energy distribution for a 90 kVp acceleration potential
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16
Q

bremsstrahlung radiation

A
  • characterised by continuous distribution of radiation
  • referred to as the continuous x-ray spectrum
  • an e- with kin energy of 70 keV can lose all, none and any intermediate level of its kin energy in a bremsstrahung interaction
  • for e-s with kin energy of 70 keV, the brem. emissions can have an energy in the range of 0-70 keV
  • 70keV in joules corresponds to the cut off wavelength
17
Q

bremsstrahlung equation

A
  • E= h x c / lambda
  • min lambda=. h x c / E max
  • h= plancks
  • c=. velocity of em radiation in a vacuum 3 x 10^8ms-1
18
Q

characteristic radiation

A
  • atomic electron from innermost shell is ejected by incoming high energy e-, creating a vacancy in the shell
  • e- from next shell drops down to fill vacancy so charactertic x-ray unique to thus element is emitted
  • produced a vacancy in that shell- transitions depend on differences in energy between shells
19
Q

x-ray spectrum

A

2 production processes occur: bremsstrahlung rad. and characteristic x-rays