Method for calibration of TOF-PET detectors using cosmic radiation

1. A method for calibration of Time-of-Flight Positron Emission Tomography (TOF-PET) detectors comprising polymeric scintillator strips and photoelectric converters, wherein cosmic radiation is used as a source of radiation, the method comprising the steps of:

recording times of reactions of particles of cosmic radiation with the scintillator strips;

determining spectra of distribution of differences in the times at which pulses are recorded at ends of the scintillator strips connected to photoelectric converters;

using the determined spectra to determine timing synchronization constants of the photoelectric converters, the constants being related to:

delays within the electronics;

speed of light propagation within the scintillator strip of the detection module; and

resolution of the difference in times of the signals recorded at the ends of the module.

2. The method according to claim 1 , comprising measuring a charge (Q A , Q B ) at the ends of the scintillator connected to the photoelectric converters, wherein the charge is a result of the reaction of the particle of cosmic radiation with the scintillator and determining an effective light pulse attenuation length and amplification coefficients of the photoelectric converters to be used to determine calibration constants of energy synchronization of the detectors.

3. The method according to claim 2 , comprising determining a reference function separately for each detector by measuring charges (Q A , Q B ) that correspond to losses in energy being deposited at distinct, precisely identified places of reactions of the particles of cosmic radiation (x).

4. The method according to claim 1 , comprising mutually calibrating at least two TOF-PET detectors by measuring the time of flight (TOF) of the particle of cosmic radiation across the scintillators of two detectors; determining the distance traveled by the particle between two scintillator strips; and determining relative time delays between the detection modules on the basis of a difference between the measured time of flight of the particle and the time of flight calculated from the distribution of particle speeds at Earth's surface.

5. The method according to claim 1 , comprising mutually calibrating at least two TOF-PET detectors by: acquiring reference spectra of times of flight of particles of cosmic radiation across two detectors; wherein the reference spectra are acquired by determining times of flight of the particles between two scintillators aligned in parallel one over the other, acquiring of the spectra of times of flight of the particles between the detectors, inverting the order of detectors and acquiring the reference spectra of times of flight of the particles between the same scintillators aligned in parallel one over the other in a reverse order, and subsequently acquiring reference spectra of the times of flight of the particles between the detectors; wherein the values of the delays of the detection modules are selected by fitting the spectra of the times of flight of the particles across the two detectors to the reference spectra of the times of flight of the particles with the detection module pair delays as free fitting parameters.

6. The method according to claim 5 , wherein the spectra of the particle speeds are fitted to the reference spectra of the particle speeds.

7. The method according to claim 5 , wherein the reference spectra are acquired for any configuration of detector pairs within the TOF-PET scanner.