Gamma Cameras and SPECT Flashcards
The resolution of a collimator is expressed as the
FWHM of a line source
Collimators generally involve a tradeoff between
spatial resolution
sensitivity
parallel-hole collimators may be classified as
high sensitivity (low resolution)
general-purpose
high resolution (low-sensitivity)
Typical collimator for Tc-99m and Tl-201
low energy
Typical collimator for Ga-67, In-111
Medium energy
Typical collimator for I-131 and F-18 (non-PET)
High-energy
Typical count range for planar image
500,000 to 1 M
SPECT images are typically reconstructed using this matrix
128 x 128
For brain SPECT, typical collimators may include
hybrid convergin and parallel hole
Typical bit depth in terms of gray levels
8 bit, 256 gray levels
Gamma cameras typically have this number of PMTs
37, 61, 91 PMTs
A typical window for Tc-99m imaging
20%
Efficiency of the detector crystal increases with
thickness
Inclusion of scattered photons in a gamma camera acquisition causes
decrease in spatial resolution
Primary cause of limited intrinsic resolution in a gamma camera
statistical fluctuation in the distribution of light photons among photmultiplier tubes from one scintillation to the next
As gamma or x-ray energy decreases, intrinsic resolution
decreases do to larger relative statistical fluctuations in the light photons per scintillation event.
As a rule of thumb, intrinsic resolution in a gamma camera and energy are related as
1 / √E
(similar to relative uncertainty in count statistics)
Thicker detectors result in
increased sensitivity
decreased intrinsic resolution
The system resolution is largely determined by the
collimator resolution
Efficiency for 140 keV with NaI(Tl)
70% to 90% for 6.4mm and 12.7 mm thick crystals
Efficiency of NaI(Tl) for 500 keV photons
less than 20%
The energy resolution improves according to photon energy as
1 / √E
due to relatively decreased statistical fluctuations at higher energy
For Tc-99m, a lower energy threshold of 130 keV should remove photons that have been scattered through angles greater than
45 degrees, but only at about 50% due to the blurring of the spectrum (for scattered and unscattered photons)