intro radiation atom-2013!01!31a

45
© UW and Brent K. Stewart PhD, DABMP 1 Introduction to Medical Imaging – Chapter 1 * Radiation and the Atom – Chapter 2 * Brent K. Stewart, PhD, DABMP Professor, Radiology Director, Diagnostic Physics a copy of this lecture may be found at: http://courses.washington.edu/radxphys/r2.html * refers to The Essential Physics of Medical Imaging, 3 rd ed., Bushberg, et al. 2012

Upload: keri-gobin

Post on 17-Nov-2015

25 views

Category:

Documents


0 download

DESCRIPTION

khfh

TRANSCRIPT

  • UW and Brent K. Stewart PhD, DABMP 1

    Introduction to Medical Imaging Chapter 1*Radiation and the Atom Chapter 2*

    Brent K. Stewart, PhD, DABMPProfessor, Radiology

    Director, Diagnostic Physics

    a copy of this lecture may be found at:http://courses.washington.edu/radxphys/r2.html

    * refers to The Essential Physics of Medical Imaging, 3rd ed., Bushberg, et al. 2012

  • UW and Brent K. Stewart PhD, DABMP 2

    Chapters 1 & 2 Lecture Objectives

    Intro to Medical Imaging what are we after technically? Contrast Spatial Resolution

    Generally describe what processes are involved in the diagnostic radiology imaging chain

    Describe the basic characteristics of electromagnetic (EM) radiation and how they are mathematically related

    Describe how atomic electronic structure determines the characteristics of emitted EM radiation

    Particulate radiation and the atomic nucleus whats the matter?

  • UW and Brent K. Stewart PhD, DABMP 3

    What a Nobel Path you Tread

    Roentgen (1901, physics): discovery of x-radiation Rabi (1944, physics): nuclear magnetic resonance

    (NMR) methodology Bloch and Purcell (1952, physics): NMR precision

    measurements Cormack and Hounsfield (1979, medicine): computed

    assisted tomography (CT) Ernst (1991, chemistry): high-resolution NMR

    spectroscopy Laterbur and Mansfield (2003, medicine): discoveries

    concerning magnetic resonance imaging (MRI)

  • UW and Brent K. Stewart PhD, DABMP 4

    Introduction to Medical Imaging

    Medical imaging requires some form of radiation capable of penetrating tissues

    This radiation must interact with the bodys various tissues in some differential manner to provide contrast

    The diagnostic utility of a medical image relates to both technical image quality and acquisition conditions

    Image quality results from many trade-offs Patient safety levels of radiation utilized (ALARA) Spatial resolution Temporal resolution Noise properties

  • UW and Brent K. Stewart PhD, DABMP 5

    MRI

    Transparency of Human Body to EM Radiation

    c.f. Macovski, A. Medical Imaging Systems, p. 3.

  • UW and Brent K. Stewart PhD, DABMP 6

    X-rays the Basic Radiological Tool

    Roentgens experimental apparatus (Crookes tube) that led to the discovery of the new radiation on 8 Nov. 1895 he demonstrated that the radiation was not due to charged particles, but due to an as yet unknown source, hence x radiation or x-rays

    Known as the radiograph of Bera Roentgens hand taken 22 Dec. 1895

  • UW and Brent K. Stewart PhD, DABMP 7

    NMR T1 for Tumor and Normal Tissue

    c.f. Damadian, R, et al. PNAS 1974; 71: 1471-3.

  • UW and Brent K. Stewart PhD, DABMP 8

    A Systematic Approach to Medical Imaging

  • X-ray Computed Tomography

    XX--ray Tuberay Tube

    DetectorsDetectors

    CT TableCT Table

    XX--ray Beamray Beam

    XX--ray Tuberay Tube

    DetectorsDetectors

    CT TableCT Table

    XX--ray Beamray Beam

    9Figure from M. Mahesh, Johns Hopkins

  • Other X-ray Modalities

    Plane-projection radiography Fluoroscopy Mammography

    UW & Brent K Stewart, Ph.D., DABMP 10c.f. http://emedicine.medscape.com/article/353833-media

    c.f. http://jlgh.org/assetMgmt/getImage.aspx?AssetID=46

  • Magnetic Resonance Imaging

    c.f. Bushberg, et al. The Essential Physics of Medical Imaging, 2nd ed., pp. 426, 429 & 461. UW & Brent K Stewart, Ph.D., DABMP 11

  • Ultrasound

    c.f. Bushberg, et al. The Essential Physics of Medical Imaging, 2nd ed., p. 501.

    c.f. http://www.cs.adelaide.edu.au/~evan/project/prog1.htm 12

  • Nuclear Medicine/Positron Emission Tomography

    c.f. http://www.griffwason.com/gw_images/MRI_scanner/glw-pet_scanner1.jpg

    c.f. http://www.medscape.com/content/2003/00/45/79/457982/art-ar457982.fig10.jpg 13

  • UW and Brent K. Stewart PhD, DABMP 14

    Spatial Resolution What are the limits?

    c.f. Bushberg, et al. The Essential Physics of Medical Imaging, 2nd ed., p. 15.

  • UW and Brent K. Stewart PhD, DABMP 15

    Contrast What does it depend on?

    Radiation must interact with the bodys various tissues in some differential manner to provide contrast

    X-ray/CT: differences in e- density (e-/cm3 = e-/gr) Ultrasound: differences in acoustic impedance (Z = c) MRI: endogenous and exogenous differences

    endogenous: T1, T2, H, flow, perfusion, diffusion exogenous: TR, TE, and TI

    NM: concentration () of radionuclide or + emitter Contrast agents exaggerate natural contrast levels

    Iodinated (x-ray/CT) Paramagnetic (MRI) Microspheres (US)

  • UW and Brent K. Stewart PhD, DABMP 16

    Radiation and the Physics of Medical Imaging

    Without radiation, life itself would be impossible Prof. Stewart

    Radiation is all around us. From natural sources like the Sun to man made sources that provide life saving medical benefits, smoke detectors, etc... - nuclearactive.com

    Youre soaking in it Madge, Palmolive spokeswoman

    10 Gy/day keeps the Dr. away "Its not the volts thatll get ya, its

    the amps. Billy Crystal, Running Scared

  • UW and Brent K. Stewart PhD, DABMP 17

    Radiation

    The propagation of energy through: Space Matter

    Can be thought of as either: Corpuscular (particles, e.g., electron) Electromagnetic (EM) Acoustic

    Acoustic radiation awaits the ultrasound sessions later on in the course

  • UW and Brent K. Stewart PhD, DABMP 18

    Characterization of Waves

    Amplitude: intensity of the wave Wavelength (): distance between identical points on adjacent

    cycles [m, nm] (1 nm = 10-9 m) Period (): time required to complete one cycle () of a wave [sec] Frequency (): number of periods per second = (1/) [Hz or sec-1] Speed of radiation: c = [m/sec]

    c.f. Bushberg, et al. The Essential Physics of Medical Imaging, 2nd ed., p.18.

  • UW and Brent K. Stewart PhD, DABMP 19

    Electromagnetic (EM) Radiation

    EM radiation consists of the transport of energy through space as a combination of an electric (E) and magnetic (M) field, both of which vary sinusoidally as a function of space and time, e.g., E(t) = E0 sin(2ct/), where is the wavelength of oscillation and c is the speed of light

    c.f. Bushberg, et al. The Essential Physics of Medical Imaging, 2nd ed., p.19.

  • UW and Brent K. Stewart PhD, DABMP 20

    The Electromagnetic (EM) Spectrum

    Physical manifestations are classified in the EM spectrum based on energy (E) and wavelength () and comprise the following general categories: Radiant heat, radio waves, microwaves Light infrared, visible and ultraviolet X-rays and gamma-rays (high energy EM emitted from the nucleus)

    c.f. http://www.uic.com.au/ral.htm

  • UW and Brent K. Stewart PhD, DABMP 21

    EM Radiation Share the Following

    Velocity in vacuum (c) = 3 x 108 m/sec Highly directional travel, esp. for shorter Interaction with matter via either absorption or scattering Unaffected by external E or M fields Characterized by , frequency (), and energy (E) So-called wave-particle duality, the manifestation

    depending on E and relative dimensions of the detector to . All EM radiation has zero mass.

    *X-rays are ionizing radiation, removing bound electrons - can cause either immediate or latent biological damage

  • UW and Brent K. Stewart PhD, DABMP 22

    EM Wave and Particle Characteristics

    Wave characteristics used to explain interference and diffraction phenomena: c [m/sec] = [m] [1/sec] As c is essentially constant, then 1/ (inversely proportional) Wavelength often measured in nanometers (nm = 10-9 m) Frequency measured in Hertz (Hz): Hz = 1/sec or sec-1

    c.f. Bushberg, et al. The Essential Physics of Medical Imaging, 2nd ed., p.18.

  • UW and Brent K. Stewart PhD, DABMP 23

    EM Wave and Particle Characteristics

    Particle characteristics when interacting with matter, high energy EM radiation act as energy quanta: photons

    E [Joule] = h = hc/, where h = Plancks constant (6.62x10-34 Joule-sec = 4.13x10-18 keV-sec)

    If E expressed in keV and in nm: E [keV] = 1.24/ [nm]

    c.f. Bushberg, et al. The Essential Physics of Medical Imaging, 2nd ed., p.18.

  • UW and Brent K. Stewart PhD, DABMP 24

    Transparency of Human Body to EM Radiation

    c.f. Bushberg, et al. The Essential Physics of Medical Imaging, 2nd ed., p.18. c.f. Macovski, A. Medical Imaging Systems, p. 3.

  • UW and Brent K. Stewart PhD, DABMP 25

    Raphex 2000 Question: EM Radiation

    G46. Regarding electromagnetic radiation: A. Wavelength is directly proportional to frequency. B. Velocity is directly proportional to frequency. C. Energy is directly proportional to frequency. D. Energy is directly proportional to wavelength. E. Energy is inversely proportional to frequency.

  • UW and Brent K. Stewart PhD, DABMP 26

    Raphex 2001 Question: EM Radiation

    G51. Which of the following has the highest photon energy? A. Radio waves B. Visible light C. Ultrasound D. X-rays E. Ultraviolet

  • UW and Brent K. Stewart PhD, DABMP 27

    Raphex 2001 Question: EM Radiation

    G52. Which of the following has the longest wavelength? A. Radio waves B. Visible light C. Ultraviolet D. X-rays E. Gamma rays

  • UW and Brent K. Stewart PhD, DABMP 28

    Raphex 2002 Question: EM Radiation

    G51. Visible light has a wavelength of about 6 x 10-7 m. 60Co gammas have a wavelength of 10-12 m and an energy of 1.2 MeV. The approximate energy of visible light is: A. 720 MeV B. 72 keV C. 2 eV D. 7.2 x 10-4 eV E. 2 x 10-6 eV

    E1 = hc/1 and E2 = hc/2, so E11 = hc = E22 E2 = E11/2 = (12 x 105 eV)(10-12 m)/(6 x 10-7 m) = 2 eV

  • UW and Brent K. Stewart PhD, DABMP 29

    Cartoon of the Day

    c.f. www.physics.utah.edu/~mohit/Physics_Cartoons.html.

  • UW and Brent K. Stewart PhD, DABMP 30

    Particulate Radiation

    Corpuscular radiations are comprised of moving particles of matter the energy of which is based on the mass and velocity of the particles

    Kinetic energy (KE) = m0v2 (for non-relativistic velocities)

    Simplified Einstein mass-energy relationship: E = m0c2

    The most significant particulate radiations of interest are:

    Alpha particles 2+

    Electrons e-

    Positron +

    Negatrons -

    Protons p+

    Neutrons n0

    Interactions with matter are collisional in nature and are governed by the conservation of energy (E) and momentum(p = mv).

  • UW and Brent K. Stewart PhD, DABMP 31c.f. http://www.ktf-split.hr/periodni/en/index.html

  • UW and Brent K. Stewart PhD, DABMP 32

    Electronic Structure Electron Orbits

    Pauli exclusion principle No two electrons in an atom may

    have identical quantum numbers

    max. 2n2 electrons per shell Quantum Numbers

    n: principal q.n. which e- shell : azimuthal angular momentum

    q.n. ( = 0, 1, ... , n-1) m: magnetic q.n. orientation of

    the e- magnetic moment in a magnetic field (m = -, -+1, ..., 0, ... -1, )

    ms: spin q.n. direction of the e-

    spin (ms = + or -)

    c.f. Bushberg, et al. The Essential Physics of Medical Imaging, 2nd ed., p.21.

    For a more detailed discussion, see - http://hyperphysics.phy-astr.gsu.edu/hbase/chemical/eleorb.html

  • UW and Brent K. Stewart PhD, DABMP 33

    Electronic Structure Electron Orbits (2)

    c.f. Hendee, et al. Medical Imaging Physics, 4th ed., p.13.

    c.f. Hendee, et al. Medical Imaging Physics, 2nd ed., p.4.

    s, p, d, f, g, h,

  • UW and Brent K. Stewart PhD, DABMP 34c.f. http://www.ktf-split.hr/periodni/en/index.html

  • Electron Configuration Table

    UW and Brent K. Stewart PhD, DABMP 35c.f. http://en.wikipedia.org/wiki/Periodic_table c.f. http://en.wikipedia.org/wiki/Electron_configuration

  • UW and Brent K. Stewart PhD, DABMP 36

    Electronic Structure Electron Binding Energy

    c.f. Bushberg, et al. The Essential Physics of Medical Imaging, 2nd ed., p.22.

    Eb Z2

    c.f. http://astro.u-strasbg.fr/~koppen/discharge/

    Highly suggested, very nice detailed description - http://hyperphysics.phy-astr.gsu.edu/hbase/hyde.html

  • Tungsten Bremsstrahlung Characteristic X-rays

    UW and Brent K. Stewart PhD, DABMP 37c.f.: Bushberg, et al., The Essential Physics of Medical Imaging, 2nd ed., p. 101.

  • UW and Brent K. Stewart PhD, DABMP 38

    Radiation from Electron Transitions

    Characteristic X-rays Auger Electrons and Fluorescent Yield (K):

    (characteristic x-rays/total) Preference for Auger e- at low Z

    c.f. Bushberg, et al. The Essential Physics of Medical Imaging, 2nd ed., p.23.

    c.f. Sorenson, et al. Physics in Nuclear Medicine, 1st ed., p.8.

  • UW and Brent K. Stewart PhD, DABMP 39

    The Atomic Nucleus

    Covered in later Nuclear Medicine sessions Composition of the Nucleus

    Protons and Neutron Number of protons = Z (same Z: isotopes) Number of neutrons = N (same N: isotones) Mass number = A = Z + N (same A: isobars) Chemical symbol = X Notation: AZXN, but AX uniquely defines an isotope (also written

    as X-A) as X implies Z and N = A - Z For example 131I or I-131, rather than 13153X78

    Isomers: nuclides with same N and Z) but different energies, e.g., 99Tc and its metastable state 99mTc

  • UW and Brent K. Stewart PhD, DABMP 40

    Raphex 2000 Question: Atomic Structure

    G10-G14. Give the charge carried by each of the following: A. +4 B. +2 C. +1 D. 0 E. -1

    G10. Alpha particle G11. Neutron G12. Electron G13. Positron G14. Photon

  • UW and Brent K. Stewart PhD, DABMP 41

    Raphex 2002 Question: Atomic Structure

    G17. Tungsten has a K-shell binding energy of 69.5 keV. Which of the following is true? A. The L-shell has a higher binding energy. B. Carbon has a higher K-shell binding energy. C. Two successive 35 keV photons could remove an electron

    from the K-shell. D. A 69 keV photon could not remove the K-shell electron, but

    could remove an L-shell electron.

  • UW and Brent K. Stewart PhD, DABMP 42

    Raphex 2001 Question: Atomic Structure

    G18. How many of the following elements have 8 electrons in their outer shell? Element: Sulfur Chlorine Argon Potassium Z: 16 17 18 19 A. None B. 1 C. 2 D. 3 E. 4

  • UW and Brent K. Stewart PhD, DABMP 43

    Raphex 2001 Question: Atomic Structure

    G18. B The nth shell can contain a maximumof 2n2 electrons, but no shell can contain more than 8 if it is the outer shell. The shell filling is as follows:

    Z K shell L shell M shell N shell Sulfur 16 2 8 6 0 Chlorine 17 2 8 7 0 Argon 18 2 8 8 0 Potassium 19 2 8 8 1

    For interactive answer, see - http://hyperphysics.phy-astr.gsu.edu/hbase/chemical/eleorb.html

  • UW and Brent K. Stewart PhD, DABMP 44c.f. http://www.ktf-split.hr/periodni/en/index.html

  • UW and Brent K. Stewart PhD, DABMP 45

    Raphex 2002 Question: Atomic Structure

    G15. 22688Ra contains 88 __________ . A. Electrons B. Neutrons C. Nucleons D. Protons and neutrons