ABSNM NMPI study materials
ABSNM NMPI study resources

ABSNM NMPI cheat sheet

ABSNM NMPI · Keep the key ideas within reach.

Quick reference

Basic Instrumentation Principles and Electronics

  • Ohm's law: V = IR; power P = VI = I²R = V²/R.

  • Pulse height is proportional to the charge collected at the preamplifier input: V = Q/C.

  • Preamplifier converts charge to voltage; amplifier shapes and amplifies pulses; pulse height analyzer sorts by amplitude.

  • Resistor–capacitor (RC) circuit time constant τ = RC; a pulse decays to 37% after one τ, 50% after 0.693τ.

  • Paralyzable dead time: observed rate m = n/(1 + nτ); nonparalyzable: m = n·e^(−nτ) for random events.

  • Photomultiplier tube gain G = δ^n, where δ is dynode multiplication factor and n is number of dynodes.

  • Energy resolution (FWHM) improves as the square root of the number of photoelectrons collected.

  • Coincidence resolving time 2τ must be shorter than the time between unrelated events to reject randoms; randoms rate ≈ 2τ·R1·R2.

Quick reference

Radiation Detection and Counting Systems

  • NaI(Tl) has high light output and good efficiency for 140 keV gamma rays; resolution ~6–7% FWHM at 140 keV.

  • Gas-filled detectors operate in ionization, proportional, or Geiger–Müller regions depending on applied voltage.

  • Well counter: NaI(Tl) well crystal with high geometric efficiency for small samples; used for blood/urine counting.

  • Dose calibrator: reentrant ionization chamber; measures activity in becquerels or curies; daily constancy check required.

  • Geiger–Müller counter has a thick dead layer and low efficiency for gamma rays; used for contamination surveys.

  • Energy spectrum: photopeak, Compton continuum, and backscatter peak; photopeak centroid identifies the radionuclide.

  • Dead-time loss can be corrected using the paralyzable or nonparalyzable model; observed count rate must be corrected to true rate.

  • Survey meter choice depends on radiation type: GM for beta/gamma contamination, ion chamber for dose rate, scintillation for low-level gamma.

Quick reference

Gamma Camera Components and Operation

  • NaI(Tl) crystal thickness typically 3/8 inch (9.5 mm) for 140 keV; thicker crystals improve high-energy efficiency but degrade spatial resolution.

  • Photomultiplier tubes are optically coupled to the crystal; Anger logic computes event position from weighted PMT signals.

  • Collimator hole geometry determines sensitivity and resolution: sensitivity ∝ hole diameter² / length²; resolution improves with longer, smaller holes.

  • Parallel-hole collimator: image size equals object size; pinhole collimator magnifies and is used for small organs (thyroid).

  • Energy window typically 20% centered on the photopeak (e.g., 126–154 keV for Tc-99m 140 keV).

  • Uniformity correction maps are acquired with a flood source and applied to subsequent images.

  • Spatial resolution (FWHM) of a gamma camera is typically 7–10 mm at 10 cm from the collimator.

  • Septal penetration occurs when photons pass through collimator septa; septal thickness must be sufficient for the photon energy.

Quick reference

Image Acquisition, Processing, and Quality Control

  • Matrix size and pixel size: pixel size = field of view / matrix dimension; smaller pixels improve sampling but reduce counts per pixel.

  • Photopeak window width affects sensitivity and scatter inclusion; narrower windows reduce scatter but increase noise.

  • Uniformity QC: integral uniformity and differential uniformity; NEMA protocols specify acceptance limits.

  • Flood field uniformity correction: acquire 10–20 million counts; calculate integral and differential uniformity.

  • Spatial resolution and linearity QC: use a bar phantom or line sources; evaluate FWHM and distortion.

  • Energy resolution QC: measure photopeak FWHM; typical NaI(Tl) value 6–7% at 140 keV.

  • Count rate performance: test dead time and maximum count rate; paralyzable vs nonparalyzable behavior.

  • Image filtering: Butterworth and Hanning filters; cutoff frequency and order control smoothing and noise.

Quick reference

Emission Tomography (SPECT and PET) Instrumentation

  • SPECT: gamma camera rotates around patient; reconstruction by filtered backprojection or iterative methods (OSEM).

  • PET: annihilation photons 511 keV emitted at ~180°; coincidence detection with timing window ~4–12 ns.

  • PET detector: scintillation crystal (e.g., LSO, BGO) coupled to PMT or SiPM; time-of-flight improves SNR.

  • Randoms in PET: random coincidence rate ≈ 2τ·R1·R2; corrected by delayed-window or model-based methods.

  • Scatter correction in PET: tail-fitting or Monte Carlo; scatter fraction typically 30–50% in 3D mode.

  • Attenuation correction: CT-based or transmission-source-based; essential for quantitative PET.

  • SPECT collimator choice: low-energy high-resolution (LEHR) for Tc-99m; medium-energy for I-131.

  • PET spatial resolution: ~4–6 mm FWHM; dominated by crystal size and positron range.

Quick reference

Instrumentation Quality Assurance and Regulatory Compliance

  • Daily QA: dose calibrator constancy, gamma camera uniformity and energy peaking.

  • Weekly/monthly QA: spatial resolution, linearity, sensitivity, and count rate performance.

  • Annual QA: full calibration and performance testing per NEMA or AAPM protocols.

  • Dose calibrator accuracy: ±5% for radionuclides used clinically; constancy within ±10%.

  • Gamma camera uniformity: integral uniformity typically <5% and differential <3% for useful field of view.

  • Regulatory: NRC 10 CFR Part 35 and state regulations govern medical use of byproduct material.

  • Record keeping: QA results must be documented and retained per regulatory requirements.

  • Acceptance testing: performed before first clinical use; establishes baseline for subsequent QA.