This document summarizes a preliminary study of a new gamma imager for online monitoring of prompt gamma emission during proton radiotherapy. Monte Carlo simulations were performed to model the imager's response to proton beams interacting with a phantom. The imager was then tested experimentally at a proton therapy facility in Uppsala, Sweden. Tests were conducted using various detector crystals and proton beam energies impinging on water and PMMA phantoms. The results provide a proof-of-concept that the imager design may be capable of visualizing prompt gamma profiles and identifying the Bragg peak position within millimeters. Further optimization of detector components is still needed to achieve the desired performance levels for clinical use.
1. Quantitative NMR (qNMR) allows for both relative and absolute concentration determination of compounds in a mixture. It requires optimizing acquisition parameters and using an internal concentration standard for absolute quantification.
2. For relative quantification, integral ratios are used to determine molar ratios without needing a standard. For absolute quantification, integrals are compared to a known standard concentration to determine unknown concentrations.
3. Many factors must be controlled for accurate qNMR including sample preparation, acquisition parameters like relaxation delay and digital resolution, processing techniques, and analysis methods for relative or absolute quantification.
You will find here all the elements presented by the CENAPT team ( Drs. Guido Pauli and Charlotte Simmler) and pertaining to the NMR workshop at the American Society of Pharmacognosy (ASP 2017, Portland Oregon).
These slides summarize the different steps related to the implementation of quantitative NMR for purity analysis.
The document discusses simulation results of Geiger mode avalanche photodiode (G-APD) cells with and without a floating P-well structure. Transient current waveforms showed advantages of the P-well structure over the conventional structure, including a reduction in current pulse width by a factor of two and current tailing reduced by a factor of eight. The simulation also demonstrated avalanche self-quenching behavior in the P-well structure for the first time. This behavior combined with a bipolar transistor could benefit a new generation of devices currently under evaluation.
1. The document describes testing procedures for an ion chamber to characterize its performance and ensure reproducibility of results when used for reference dosimetry.
2. Tests include measuring the stem effect, cylindrical symmetry, and collection efficiency using different bias voltages.
3. Quantification of noise levels via the signal to noise ratio helps assess the chamber's suitability for low dose measurements.
Nuclear imaging PET CT Imaging Medical Physics Nuclear MedicineShahid Younas
The document discusses various types of collimators used in nuclear imaging, including parallel-hole collimators (such as low-energy high-sensitivity, low-energy all-purpose, and low-energy high-resolution collimators), pinhole collimators, converging collimators, and diverging collimators. It explains how each collimator works, its advantages and disadvantages, and factors that affect its imaging characteristics such as sensitivity, resolution, and field of view. The document also discusses image formation in gamma cameras and factors that affect spatial resolution and contrast.
Monte carlo Technique - An algorithm for Radiotherapy CalculationsSambasivaselli R
Monte Carlo techniques are used to simulate particle transport through complex geometries to calculate dose distributions. The key steps are: (1) sampling the distance to the next interaction, interaction type, and energy/direction of secondary particles, (2) tracking particle histories through condensed histories or splitting/Russian roulette, and (3) calculating dose deposition in voxels. While fully accurate, Monte Carlo is statistically limited by the number of histories. Variance reduction techniques increase efficiency but introduce weighting factors. Overall uncertainty is typically within 3% given proper commissioning and cross-section libraries.
1) Raman spectroscopy was used to study the thermal maturity of solid bitumen from a sample with low maturity (0.61% reflectance). However, initial measurements showed intense fluorescence that obscured the typical Raman bands.
2) Repeated measurements at the same location caused the fluorescence background to decrease over time, revealing the Raman bands more clearly without artificially altering the sample.
3) Multiple measurements allowed the fluorescent component to be isolated from the Raman spectrum, producing a clean spectrum free of background interference. This method provides a way to apply Raman spectroscopy to samples that normally exhibit strong fluorescence.
1. Quantitative NMR (qNMR) allows for both relative and absolute concentration determination of compounds in a mixture. It requires optimizing acquisition parameters and using an internal concentration standard for absolute quantification.
2. For relative quantification, integral ratios are used to determine molar ratios without needing a standard. For absolute quantification, integrals are compared to a known standard concentration to determine unknown concentrations.
3. Many factors must be controlled for accurate qNMR including sample preparation, acquisition parameters like relaxation delay and digital resolution, processing techniques, and analysis methods for relative or absolute quantification.
You will find here all the elements presented by the CENAPT team ( Drs. Guido Pauli and Charlotte Simmler) and pertaining to the NMR workshop at the American Society of Pharmacognosy (ASP 2017, Portland Oregon).
These slides summarize the different steps related to the implementation of quantitative NMR for purity analysis.
The document discusses simulation results of Geiger mode avalanche photodiode (G-APD) cells with and without a floating P-well structure. Transient current waveforms showed advantages of the P-well structure over the conventional structure, including a reduction in current pulse width by a factor of two and current tailing reduced by a factor of eight. The simulation also demonstrated avalanche self-quenching behavior in the P-well structure for the first time. This behavior combined with a bipolar transistor could benefit a new generation of devices currently under evaluation.
1. The document describes testing procedures for an ion chamber to characterize its performance and ensure reproducibility of results when used for reference dosimetry.
2. Tests include measuring the stem effect, cylindrical symmetry, and collection efficiency using different bias voltages.
3. Quantification of noise levels via the signal to noise ratio helps assess the chamber's suitability for low dose measurements.
Nuclear imaging PET CT Imaging Medical Physics Nuclear MedicineShahid Younas
The document discusses various types of collimators used in nuclear imaging, including parallel-hole collimators (such as low-energy high-sensitivity, low-energy all-purpose, and low-energy high-resolution collimators), pinhole collimators, converging collimators, and diverging collimators. It explains how each collimator works, its advantages and disadvantages, and factors that affect its imaging characteristics such as sensitivity, resolution, and field of view. The document also discusses image formation in gamma cameras and factors that affect spatial resolution and contrast.
Monte carlo Technique - An algorithm for Radiotherapy CalculationsSambasivaselli R
Monte Carlo techniques are used to simulate particle transport through complex geometries to calculate dose distributions. The key steps are: (1) sampling the distance to the next interaction, interaction type, and energy/direction of secondary particles, (2) tracking particle histories through condensed histories or splitting/Russian roulette, and (3) calculating dose deposition in voxels. While fully accurate, Monte Carlo is statistically limited by the number of histories. Variance reduction techniques increase efficiency but introduce weighting factors. Overall uncertainty is typically within 3% given proper commissioning and cross-section libraries.
1) Raman spectroscopy was used to study the thermal maturity of solid bitumen from a sample with low maturity (0.61% reflectance). However, initial measurements showed intense fluorescence that obscured the typical Raman bands.
2) Repeated measurements at the same location caused the fluorescence background to decrease over time, revealing the Raman bands more clearly without artificially altering the sample.
3) Multiple measurements allowed the fluorescent component to be isolated from the Raman spectrum, producing a clean spectrum free of background interference. This method provides a way to apply Raman spectroscopy to samples that normally exhibit strong fluorescence.
Nuclear imaging, PET CT MEDICAL PHYSICSShahid Younas
SPECT provides tomographic images of radiotracer distribution by acquiring 2D projection images from multiple angles around the patient and reconstructing transverse slices. Projection images are blurred due to attenuation, scatter, and resolution loss with distance from the collimator. Reconstruction methods like filtered back projection aim to reduce blurring by deconvolving the projection data with an appropriate filter. The choice of filter depends on the noise and resolution properties of the acquired projection images for a given study.
This document contains the results of an experiment measuring signal frequencies and amplitudes across two channels. For part A, various frequency and amplitude measurements are displayed for signals on channel 1 and channel 2. Calculations are shown for the sampling time, frequency, and maximum bandwidth based on the measurements. For part B, more frequency and amplitude measurements are displayed for signals on each channel after applying a reconstruction filter.
This document presents a new method for locating ungrounded faults in underground distribution systems using wavelet analysis and artificial neural networks (ANNs). Voltage and current signals are simulated for different fault types, locations, and conditions using EMTP software. Wavelet analysis is used to extract features from the signals related to fault classification and location. ANNs are then applied to classify fault types based on the extracted features and to determine the fault location for each fault type based on additional extracted features. The results indicate the technique can accurately locate faults under a variety of system conditions.
This document summarizes an experimental study that measured the saturation thickness of granite and glass materials using gamma backscattering. Gamma backscattering is a non-destructive testing technique that can determine material thickness and density by detecting gamma photons backscattered from within a material. The experiment used a 137Cs radioactive source and gamma spectroscopy system to measure the backscattered gamma photon count rates from granite and glass slabs of increasing thickness. The results were analyzed to estimate the saturation thickness for each material, above which increasing thickness does not significantly increase the backscattered count rate.
This document summarizes the goals and process of modeling treatment beams in a treatment planning system (TPS) during a radiation oncology rotation. The goals were to model one photon beam, one electron beam, and wedges, and then validate the modeled beams. Modeling involved collecting beam data, defining the machine and beams in the TPS, and fine-tuning parameters to match measured and computed dose distributions. Validation compared modeled and measured profiles, percent depth doses, and other dosimetric tests. The rotation provided an understanding of the nuances of TPS modeling.
This document summarizes characterization tests performed on an FPGA-based spectrometer prototype for heterodyne receivers at the Large Millimeter Telescope (LMT). The spectrometer uses two ADC ports, each with four cores capable of sampling at 1.25 Gs/s. Tests included offset/gain/phase calibration to reduce spurs and improve signal-to-noise ratio, linearity tests showing a linear response up to amplifier saturation, and Allan variance measurements showing noise follows the radiometer equation out to 1000 seconds of integration time. Future work includes adding two more modes, integrating with other instruments, and performing science observations at the LMT.
This document discusses single photon emission computed tomography (SPECT). SPECT generates transverse images depicting the distribution of gamma ray emitting nuclides in patients. Projection images are acquired from an arc of 180 or 360 degrees around the patient and transverse images are reconstructed using filtered back-projection or iterative methods. The goals of SPECT reconstruction are to estimate the true radioactivity distribution from the measured projection data while accounting for effects like attenuation, scatter, and detector response. Filtering is applied to projection images before back-projection to "deblur" the reconstructed images and improve spatial resolution.
Hacking cddvd blu ray for fun and scientific researchEn-Te Hwu
https://www.youtube.com/watch?v=5bqujaldaCQ
There are other hackers works described in the open access review paper:
https://pubs.acs.org/doi/abs/10.1021/acssensors.8b00340
This document summarizes the results from field testing a prototype Fast Array of Single-Pixel Telescopes (FAST) for ultra-high energy cosmic ray detection. Key findings include:
1) The FAST prototype operated very stably and detected laser shots and air shower candidates consistent with expectations.
2) Reconstructed air shower maximum depths from FAST data alone could achieve 30 g/cm^2 resolution for energies above 10^19.5 eV.
3) Future improvements to the FAST design were identified, and a full 30°×30° prototype is the next step.
This lecture discusses the development of nuclear imaging techniques. It begins with an overview of nuclear imaging and its use of gamma rays and x-rays to form images. The earliest device was the rectilinear scanner, which used a single moving detector. The Anger gamma camera was a significant improvement as it allowed simultaneous detection over a large area. Modern gamma cameras use NaI(Tl) scintillator crystals coupled to PMTs to convert gamma ray interactions to light and then electrical signals. Digital processing is used to determine interaction locations and form images. Collimators are used to selectively detect gamma rays from a desired direction.
First results from the full-scale prototype for the Fluorescence detector Arr...Toshihiro FUJII
The Fluorescence detector Array of Single-pixel Telescopes (FAST) is a design concept for the next generation of ultrahigh-energy cosmic ray (UHECR) observatories, addressing the requirements for a large-area, low-cost detector suitable for measuring the properties of the highest energy cosmic rays. In the FAST design, a large field of view is covered by a few pixels at the focal plane of a mirror or Fresnel lens. Motivated by the successful detection of UHECRs using a prototype comprised of a single 200 mm photomultiplier-tube and a 1 m2 Fresnel lens system [Astropart.Phys. 74 (2016) 64-72], we have developed a new full-scale prototype consisting of four 200 mm photomultiplier-tubes at the focus of a segmented mirror of 1.6 m in diameter. In October 2016 we installed the full-scale prototype at the Telescope Array site in central Utah, USA, and began steady data taking. We report on first results of the full-scale FAST prototype, including measurements of artificial light sources, distant ultraviolet lasers, and UHECRs.
35th International Cosmic Ray Conference — ICRC2017 18th July, 2017
Bexco, Busan, Korea
The document describes the Fluorescence detector Array of Single-pixel Telescopes (FAST) project. FAST aims to build an array of low-cost single-pixel fluorescence detectors spaced over large areas to study ultra-high energy cosmic rays (UHECR). Each FAST station would have 12 telescopes with 4 PMTs each, covering a 30°x360° field of view. An array of 500 stations over 150,000 km2 could achieve an exposure over 12 times that of the Pierre Auger Observatory. Simulations show FAST may achieve 10% energy resolution and 35 g/cm2 Xmax resolution for cosmic rays above 1019.5 eV. The full-scale FAST prototype has been constructed and work is ongoing to develop
This dissertation presents the development of a novel multi-slit collimated imaging system to image prompt gamma rays (PGs) emitted during proton beam cancer therapy, in order to verify proton beam range. The system uses a multi-slit collimator paired with a position-sensitive LSO scintillation detector to provide two-dimensional PG imaging. Initial measurements using a 50 MeV proton beam demonstrated the ability to reconstruct 2D PG distributions at clinical beam currents and localize the Bragg peak position to within 1-2 mm, suggesting the potential for the system to detect small shifts in proton range while delivering a fraction of a typical treatment dose. Further investigation and system optimization is warranted to validate system performance at clinical beam energies and implement
This document discusses a study that fabricated paraffin wax phantoms to measure absorbed radiation doses and compare them to other phantom materials like water, solid water, and PMMA. Two paraffin wax phantoms were made, one with bubbles and one without, and both were scanned using a CT scanner. Absorbed doses were measured in the phantoms using ionization chambers and a linear accelerator. Scaling factors were calculated to determine the absorbed dose in different phantoms relative to a water phantom. The results found paraffin wax phantoms had the lowest deviation from water, around 1%, while PMMA had the highest at over 5%. Paraffin wax phantoms were determined to be a suitable
EDS softwares INCA and EDAX_EM forum_Yina Guo_May 2016YinaGuo
The document discusses energy dispersive spectroscopy (EDS) using scanning electron microscopy (SEM) and transmission electron microscopy (TEM). It provides an overview of how EDS works, factors that influence resolution and detection limits, and tips for acquisition and analysis using EDS software. Examples are given of multipoint analysis, elemental mapping, and line scans to identify phases in a steel sample.
Development of a prototype for Fluorescence detector Array of Single-pixel Te...Toshihiro FUJII
This document summarizes the results from the first field test of the Fluorescence detector Array of Single-pixel Telescopes (FAST) concept. The test involved a single FAST telescope prototype installed at the Telescope Array site in Utah. Key results included stable operation under night sky backgrounds, detection of laser shots and air shower signals consistent with expectations, and a successful collaboration between the Pierre Auger, Telescope Array and JEM-EUSO experiments. Future plans involve developing a full 30x30 degree prototype to further validate the FAST concept.
AFM talk ASAS 10dec2015 Jenny to publish.pptxPonrajVijayan1
AFM was invented in 1986 by Binning and colleagues and belongs to the scanning probe microscopy family. It uses a sharp tip on a flexible cantilever to scan a sample surface at an atomic scale resolution and detect short-range forces between the tip and sample. AFM can operate in various modes including contact, tapping, and dynamic contact modes and is capable of imaging in air, liquid, and other environments.
Single Electron Spin Detection Slides For Uno Interviewchenhm
1. The document discusses different algorithms for detecting weak electron spin signals in single electron spin microscopy, including energy detector, matched filter, power-law detector, M-quadratic detector, and generalized likelihood ratio detector.
2. Simulation results show that detection performance improves with more prior knowledge of the signal characteristics, and the M-quadratic detector achieves better performance than the energy detector with lower computation time.
3. Future work involves developing optimal quadratic detection schemes and implementing the algorithms on a computer cluster for real-time signal detection.
This document summarizes an experimental study that measured the saturation thickness of granite and glass materials using gamma ray backscattering. Gamma rays from a 137Cs source were directed at samples of increasing thickness. The count rate of backscattered gamma rays was measured with a NaI detector and analyzed with spectroscopy software. The count rate increased linearly with thickness up to a saturation point, beyond which additional thickness did not increase the count rate. Determining this saturation thickness is important because thickness can be measured below it and density gauges operate above it. The experiment found saturation thicknesses for granite and glass, providing useful data for non-destructive testing using gamma ray backscattering.
International Journal of Engineering and Science Invention (IJESI)inventionjournals
This paper presents an experimental study of saturation thickness for granite and glass materials using gamma backscattering. Gamma backscattering is a non-destructive technique to determine thickness and density of materials. The study used a 137Cs radioactive source and gamma spectroscopy system to measure the count rate of backscattered gamma photons from granite and glass slabs of increasing thickness. It was found that for granite, the count rate increased linearly up to 1.2cm thickness and saturated at 2.2cm thickness. For glass, the count rate increased linearly up to 1.6cm and saturated at 2.4cm thickness. The saturation thickness depends on the material density and represents the limit where thickness measurement is possible using gamma backscattering.
Gamma cameras use NaI(Tl) scintillation crystals and photomultiplier tubes to detect gamma rays emitted by radiotracers injected into patients. They produce 2D images used for nuclear medicine diagnoses. Key components include parallel hole collimators to filter gamma rays, crystals that convert gamma rays to light, PMTs that convert light to electrical signals, and computers for image processing. Quality assurance tests image uniformity, resolution, background levels, and the center of rotation. Gamma cameras have improved diagnosis since their development in the 1950s and remain an important tool in nuclear medicine.
Nuclear imaging, PET CT MEDICAL PHYSICSShahid Younas
SPECT provides tomographic images of radiotracer distribution by acquiring 2D projection images from multiple angles around the patient and reconstructing transverse slices. Projection images are blurred due to attenuation, scatter, and resolution loss with distance from the collimator. Reconstruction methods like filtered back projection aim to reduce blurring by deconvolving the projection data with an appropriate filter. The choice of filter depends on the noise and resolution properties of the acquired projection images for a given study.
This document contains the results of an experiment measuring signal frequencies and amplitudes across two channels. For part A, various frequency and amplitude measurements are displayed for signals on channel 1 and channel 2. Calculations are shown for the sampling time, frequency, and maximum bandwidth based on the measurements. For part B, more frequency and amplitude measurements are displayed for signals on each channel after applying a reconstruction filter.
This document presents a new method for locating ungrounded faults in underground distribution systems using wavelet analysis and artificial neural networks (ANNs). Voltage and current signals are simulated for different fault types, locations, and conditions using EMTP software. Wavelet analysis is used to extract features from the signals related to fault classification and location. ANNs are then applied to classify fault types based on the extracted features and to determine the fault location for each fault type based on additional extracted features. The results indicate the technique can accurately locate faults under a variety of system conditions.
This document summarizes an experimental study that measured the saturation thickness of granite and glass materials using gamma backscattering. Gamma backscattering is a non-destructive testing technique that can determine material thickness and density by detecting gamma photons backscattered from within a material. The experiment used a 137Cs radioactive source and gamma spectroscopy system to measure the backscattered gamma photon count rates from granite and glass slabs of increasing thickness. The results were analyzed to estimate the saturation thickness for each material, above which increasing thickness does not significantly increase the backscattered count rate.
This document summarizes the goals and process of modeling treatment beams in a treatment planning system (TPS) during a radiation oncology rotation. The goals were to model one photon beam, one electron beam, and wedges, and then validate the modeled beams. Modeling involved collecting beam data, defining the machine and beams in the TPS, and fine-tuning parameters to match measured and computed dose distributions. Validation compared modeled and measured profiles, percent depth doses, and other dosimetric tests. The rotation provided an understanding of the nuances of TPS modeling.
This document summarizes characterization tests performed on an FPGA-based spectrometer prototype for heterodyne receivers at the Large Millimeter Telescope (LMT). The spectrometer uses two ADC ports, each with four cores capable of sampling at 1.25 Gs/s. Tests included offset/gain/phase calibration to reduce spurs and improve signal-to-noise ratio, linearity tests showing a linear response up to amplifier saturation, and Allan variance measurements showing noise follows the radiometer equation out to 1000 seconds of integration time. Future work includes adding two more modes, integrating with other instruments, and performing science observations at the LMT.
This document discusses single photon emission computed tomography (SPECT). SPECT generates transverse images depicting the distribution of gamma ray emitting nuclides in patients. Projection images are acquired from an arc of 180 or 360 degrees around the patient and transverse images are reconstructed using filtered back-projection or iterative methods. The goals of SPECT reconstruction are to estimate the true radioactivity distribution from the measured projection data while accounting for effects like attenuation, scatter, and detector response. Filtering is applied to projection images before back-projection to "deblur" the reconstructed images and improve spatial resolution.
Hacking cddvd blu ray for fun and scientific researchEn-Te Hwu
https://www.youtube.com/watch?v=5bqujaldaCQ
There are other hackers works described in the open access review paper:
https://pubs.acs.org/doi/abs/10.1021/acssensors.8b00340
This document summarizes the results from field testing a prototype Fast Array of Single-Pixel Telescopes (FAST) for ultra-high energy cosmic ray detection. Key findings include:
1) The FAST prototype operated very stably and detected laser shots and air shower candidates consistent with expectations.
2) Reconstructed air shower maximum depths from FAST data alone could achieve 30 g/cm^2 resolution for energies above 10^19.5 eV.
3) Future improvements to the FAST design were identified, and a full 30°×30° prototype is the next step.
This lecture discusses the development of nuclear imaging techniques. It begins with an overview of nuclear imaging and its use of gamma rays and x-rays to form images. The earliest device was the rectilinear scanner, which used a single moving detector. The Anger gamma camera was a significant improvement as it allowed simultaneous detection over a large area. Modern gamma cameras use NaI(Tl) scintillator crystals coupled to PMTs to convert gamma ray interactions to light and then electrical signals. Digital processing is used to determine interaction locations and form images. Collimators are used to selectively detect gamma rays from a desired direction.
First results from the full-scale prototype for the Fluorescence detector Arr...Toshihiro FUJII
The Fluorescence detector Array of Single-pixel Telescopes (FAST) is a design concept for the next generation of ultrahigh-energy cosmic ray (UHECR) observatories, addressing the requirements for a large-area, low-cost detector suitable for measuring the properties of the highest energy cosmic rays. In the FAST design, a large field of view is covered by a few pixels at the focal plane of a mirror or Fresnel lens. Motivated by the successful detection of UHECRs using a prototype comprised of a single 200 mm photomultiplier-tube and a 1 m2 Fresnel lens system [Astropart.Phys. 74 (2016) 64-72], we have developed a new full-scale prototype consisting of four 200 mm photomultiplier-tubes at the focus of a segmented mirror of 1.6 m in diameter. In October 2016 we installed the full-scale prototype at the Telescope Array site in central Utah, USA, and began steady data taking. We report on first results of the full-scale FAST prototype, including measurements of artificial light sources, distant ultraviolet lasers, and UHECRs.
35th International Cosmic Ray Conference — ICRC2017 18th July, 2017
Bexco, Busan, Korea
The document describes the Fluorescence detector Array of Single-pixel Telescopes (FAST) project. FAST aims to build an array of low-cost single-pixel fluorescence detectors spaced over large areas to study ultra-high energy cosmic rays (UHECR). Each FAST station would have 12 telescopes with 4 PMTs each, covering a 30°x360° field of view. An array of 500 stations over 150,000 km2 could achieve an exposure over 12 times that of the Pierre Auger Observatory. Simulations show FAST may achieve 10% energy resolution and 35 g/cm2 Xmax resolution for cosmic rays above 1019.5 eV. The full-scale FAST prototype has been constructed and work is ongoing to develop
This dissertation presents the development of a novel multi-slit collimated imaging system to image prompt gamma rays (PGs) emitted during proton beam cancer therapy, in order to verify proton beam range. The system uses a multi-slit collimator paired with a position-sensitive LSO scintillation detector to provide two-dimensional PG imaging. Initial measurements using a 50 MeV proton beam demonstrated the ability to reconstruct 2D PG distributions at clinical beam currents and localize the Bragg peak position to within 1-2 mm, suggesting the potential for the system to detect small shifts in proton range while delivering a fraction of a typical treatment dose. Further investigation and system optimization is warranted to validate system performance at clinical beam energies and implement
This document discusses a study that fabricated paraffin wax phantoms to measure absorbed radiation doses and compare them to other phantom materials like water, solid water, and PMMA. Two paraffin wax phantoms were made, one with bubbles and one without, and both were scanned using a CT scanner. Absorbed doses were measured in the phantoms using ionization chambers and a linear accelerator. Scaling factors were calculated to determine the absorbed dose in different phantoms relative to a water phantom. The results found paraffin wax phantoms had the lowest deviation from water, around 1%, while PMMA had the highest at over 5%. Paraffin wax phantoms were determined to be a suitable
EDS softwares INCA and EDAX_EM forum_Yina Guo_May 2016YinaGuo
The document discusses energy dispersive spectroscopy (EDS) using scanning electron microscopy (SEM) and transmission electron microscopy (TEM). It provides an overview of how EDS works, factors that influence resolution and detection limits, and tips for acquisition and analysis using EDS software. Examples are given of multipoint analysis, elemental mapping, and line scans to identify phases in a steel sample.
Development of a prototype for Fluorescence detector Array of Single-pixel Te...Toshihiro FUJII
This document summarizes the results from the first field test of the Fluorescence detector Array of Single-pixel Telescopes (FAST) concept. The test involved a single FAST telescope prototype installed at the Telescope Array site in Utah. Key results included stable operation under night sky backgrounds, detection of laser shots and air shower signals consistent with expectations, and a successful collaboration between the Pierre Auger, Telescope Array and JEM-EUSO experiments. Future plans involve developing a full 30x30 degree prototype to further validate the FAST concept.
AFM talk ASAS 10dec2015 Jenny to publish.pptxPonrajVijayan1
AFM was invented in 1986 by Binning and colleagues and belongs to the scanning probe microscopy family. It uses a sharp tip on a flexible cantilever to scan a sample surface at an atomic scale resolution and detect short-range forces between the tip and sample. AFM can operate in various modes including contact, tapping, and dynamic contact modes and is capable of imaging in air, liquid, and other environments.
Single Electron Spin Detection Slides For Uno Interviewchenhm
1. The document discusses different algorithms for detecting weak electron spin signals in single electron spin microscopy, including energy detector, matched filter, power-law detector, M-quadratic detector, and generalized likelihood ratio detector.
2. Simulation results show that detection performance improves with more prior knowledge of the signal characteristics, and the M-quadratic detector achieves better performance than the energy detector with lower computation time.
3. Future work involves developing optimal quadratic detection schemes and implementing the algorithms on a computer cluster for real-time signal detection.
This document summarizes an experimental study that measured the saturation thickness of granite and glass materials using gamma ray backscattering. Gamma rays from a 137Cs source were directed at samples of increasing thickness. The count rate of backscattered gamma rays was measured with a NaI detector and analyzed with spectroscopy software. The count rate increased linearly with thickness up to a saturation point, beyond which additional thickness did not increase the count rate. Determining this saturation thickness is important because thickness can be measured below it and density gauges operate above it. The experiment found saturation thicknesses for granite and glass, providing useful data for non-destructive testing using gamma ray backscattering.
International Journal of Engineering and Science Invention (IJESI)inventionjournals
This paper presents an experimental study of saturation thickness for granite and glass materials using gamma backscattering. Gamma backscattering is a non-destructive technique to determine thickness and density of materials. The study used a 137Cs radioactive source and gamma spectroscopy system to measure the count rate of backscattered gamma photons from granite and glass slabs of increasing thickness. It was found that for granite, the count rate increased linearly up to 1.2cm thickness and saturated at 2.2cm thickness. For glass, the count rate increased linearly up to 1.6cm and saturated at 2.4cm thickness. The saturation thickness depends on the material density and represents the limit where thickness measurement is possible using gamma backscattering.
Gamma cameras use NaI(Tl) scintillation crystals and photomultiplier tubes to detect gamma rays emitted by radiotracers injected into patients. They produce 2D images used for nuclear medicine diagnoses. Key components include parallel hole collimators to filter gamma rays, crystals that convert gamma rays to light, PMTs that convert light to electrical signals, and computers for image processing. Quality assurance tests image uniformity, resolution, background levels, and the center of rotation. Gamma cameras have improved diagnosis since their development in the 1950s and remain an important tool in nuclear medicine.
Luigi Giubbolini | Time/Space-Probing Interferometer for Plasma DiagnosticsLuigi Giubbolini
By Luigi Giubbolini Published article about Rapid progress in plasma applications requires new instrumentation. Luigi Giubbolini has engineering experience in industrial, government laboratory & academic environments.
The document summarizes a PhD thesis defense on vectorial statistical characterization of optical signals for high-speed communication and quantum communication. It discusses the motivations and objectives of developing an optical pulsed source with picosecond pulses, tunable repetition rate from MHz to GHz, high extinction ratio, and low noise for applications in optical undersampling and quantum key distribution. The proposed architecture generates pulses using a semiconductor optical amplifier, compresses them using soliton effects in fiber, and suppresses pedestals using an optical filter. Characterization shows pulses down to 1 ps can be generated with repetition rates from 100 MHz to 790 MHz and carrier wavelengths from 1540 nm to 1565 nm, with timing jitter below 3 ps.
The document describes the development of a dual microchannel plate (MCP) framing camera for imaging high-energy x-rays above 50 keV. A dual MCP configuration is proposed to increase the sensitivity at high energies by using the first MCP as a low-gain photocathode and the second MCP as a high-gain electron multiplier. Testing of a dual MCP module showed a detective quantum efficiency of 4.5% for 59 keV x-rays, which is 3 times higher than a single thick MCP typically used in such cameras. The dual MCP configuration separates the photon absorption from electron multiplication to reduce statistical noise compared to a single thick MCP operated at high gain.
The document summarizes the PAMELA experiment's silicon tracker, including its design, components, performance, and preliminary analysis of flight data. The tracker uses silicon microstrip sensors and VA1 readout chips to precisely measure particle trajectories in the magnetic spectrometer. Initial flight data shows the tracker is working as expected, with nominal noise levels, signal-to-noise ratios, and spatial resolution allowing for momentum and charge identification of cosmic rays.
Nanonics produces atomic force microscopy (AFM) systems that provide singular excellence in structural and functional imaging for biology. Their systems feature unique glass probes that do not obscure the optical axis and allow transparent integration with microscopes. Nanonics' tuning fork feedback provides unprecedented force sensitivity down to the mechanical force of a single photon. This allows true non-contact imaging and switching between AFM and STM feedback with the same probe. Nanonics systems are capable of imaging previously impossible structures like microvilli in live cells.
CMOS logic scaling is reaching a point with gradually diminishing returns. So that is why so-called Beyond CMOS compute paradigms have gained a lot of attention in the last decade. It is however far from trivial to beat advanced ultimately-scaled CMOS logic realisations. Plasmonics wave computing is one potential emerging option which could have better area-performance metrics for high performance computing and especially exascale computing servers. In this talk a review will be provided of the current status of this technology and why and where it could be beneficial.
Nanoscale cascaded plasmonic logic gates for non-boolean wave computation
Siena16_Bennati
1. PRELIMINARY
STUDY
OF
A
NEW
GAMMA
IMAGER
FOR
ON-‐LINE
MONITORING
PROMPT-‐GAMMA
EMISSION
DURING
PROTON
RADIOTHERAPY
PAOLO
BENNATI
KTH
-‐ SCHOOL
OF
TECHNOLOGY
AND
HEALTH
STOCKHOLM,
SWEDEN
14th
Topical
Seminar
on
Innovative
Particle
and
Radiation
Detectors
(IPRD16)
3
-‐ 6
October
2016
Siena,
Italy
2. COLLABORATION
• Royal
Institute
of
Technology
– KTH,
Stockhom Sweden
• Skandion Clinik,
Uppsala
Sweden
• La
Sapienza
University,
Roma
Italy
IPRD16
-‐ Siena,
3-‐6/October
3. PROTON
THERAPY
• Better
dose
delivery
than
X-‐ray
could
spares
healthy
tissue
• An
online
imaging
system
is
strongly
requested
to
improve
verification
of
range
in
tissue:
Ø Prompt-‐gamma
imager
Ø IN-‐BEAM
PET
scanner
(Beta+
emission)
Ø Compton
camera
Images
from
“Proton-‐beam
therapy”
S.Yjanik,
Springer
(2013)
• Requirements:
• on-‐line
with
the
treatment
• 2
mm
spatial
resolution
IPRD16
-‐ Siena,
3-‐6/October
4. SYSTEM
CHARACTERISTICS
• Compact
gamma
camera
equipped
with
THIN
scintillation
crystal
• Knife-‐edge
collimator
*
I. 2
mm
and
30° aperture.
II. Magnification
2:1
*
Perali I,
et
al.
Phys
Med
Biol (2014) 59(19)
Gamma
camera
developed
at
La
Sapienza
University,
Rome
Italy
IPRD16
-‐ Siena,
3-‐6/October
5. DETECTOR
SPECIFICATIONS
Specifications pro cons
Crystal Two new
crystal:
• Cry019
– 6
mm
• LFS*
– 2mm
thickness
• Fast
and
high-‐Z crystal
• Free image
digitization
• Negligible
Compton
reabsorption
Negligible efficiency
at
2-‐6
MeV
photons
Phototodetector Hamamatsu
H8500-‐100
multianodes-‐PMT
• super
bialkaly catode
(QE
-‐35%)
• 50x50
mm2 area
Metal
channel
dynodes
and
the
new
super-‐bialkaly
photocatode offer high
performances
and
reduced
anode
signal
-‐
Electronics
($) • FPGA
based
• 64-‐independent
channels
read-‐out
• 100KHz clock
• About
20’000-‐30’000
max
count
rate
• low
noise
• Single
photon
detection
• Limited
count-‐rate
capability (for
proton
therapy!)
• No
trigger
*Luthetium fine
silicate
($)
A.Fabbri et.al Nuclear
Physics
B-‐Proceedings
Supplements
215
(1),
328-‐332,
2011
IPRD16
-‐ Siena,
3-‐6/October
6. GATE*
MC
SIMULATION
-‐ 100,
150,
200
MeV
Proton
Energy
-‐ PMMA
Phantom
– 16cm
diam.
x
24cm
length
-‐ Knife-‐edge
collimator
and
a
gamma
camera
with
an
ideal
LYSO
crystal
-‐ Detector
at
90° respect
the
proton
beam
-‐ NO
magnification
The
simulation
was
divided
in
two
phases:
first,
the
interaction
of
protons
in
the
phantom.
Second,
the
imaging
system
was
modeled
and
the
first
simulation
was
used
as
imput.
*Gate
7.1
with
QGSP-‐BIC-‐HP-‐EMZ
reference
physics
list
IPRD16
-‐ Siena,
3-‐6/October
7. GATE
MC
RESULTS
• We
verify
a
correlation
between
the
inflection
point
and
the
position
of
the
Bragg-‐
peak
as
for
Janssen
et
al.,
which
resulted
about
9mm
at
100,
150
and
200
MeV
• MC
shows
that
our
detector
could
be
able
to
identify
the
gamma
profile.
The
gap
with
BP
rise
to
12mm.
Inflection
point
Prompt
gamma
imaged
by
knife-‐edge
gamma
system
Prompt
gamma
from
150MeV
protons
detected
with
no
energy
selection
Gustaf Lönn,
KTH
Master Degree Thesis,
ref:diva2:937846
IPRD16
-‐ Siena,
3-‐6/October
8. THE
PROTON
FACILITY
@
UPPSALA
• The
Skandion Clinic
is
the
first
clinical
centre for
proton
therapy
in
Scandinavia
joint
investment
of
several
university
hospitals.
• The
clinic
is
planned
to
treat
between
1000
and
2500
patients
annually,
each
with
an
average
of
15
fractions
(individual
treatments).
• Two
treatment
room
(a
third
one
is
planned)
and
a
research
room
will
use
protons
accelerated
up
to
260
MeV
energy
(at
60%
of
speed
of
light).
Treatment
room
Aerial
view
of
the
clinic
IPRD16
-‐ Siena,
3-‐6/October
(from
http://www.skandionkliniken.se)
9. EXPERIMENTAL
SETUP:
THE
PROTON
ROOM
Proton
noddle
Patient
bed
gantry
10
cm
FoV and
centered
at
12.5
cm
2.0 liters Water
Phantomdetector
Lead
brick
Proton
beam
Detector
was
installed
on
the
patient
bed.
Lasers
were
used
to
align
the
phantom
with
the
beam
and
the
collimator
IPRD16
-‐ Siena,
3-‐6/October
10. SUMMARY
OF
THE
MEASUREMENTS
Crystal
used
for
the
test
Thickness Efficiency at
4
MeV*
Phantom tested Proton
energy
range
1ST test CRY019
50mm diameter
6
mm 15% Water
Phantom:
2liter
bottle
-‐ 12cm
diameter)
110
>
145
MEV
2ND test LFS crystal
50
× 50
mm2
2
mm >5% PMMA
Phantom
16
cm
diameter
X
24
cm
length
100
>
160
MeV
3rd test LFS
crystal +5mm
step
shifting of the
phantom
(fixed
energy)
150
MeV
*Value
for
LSO
crystal
>>
photofraction =
2%
IPRD16
-‐ Siena,
3-‐6/October
11. Calibration:
Luthetium natural
radioactivity
Pulse
height
spectrum
from
Lu177
self-‐activityc
Lu176
natural
abundance
(2.6%
of
Lu)
is
responsible
of
about
2800
cps
detector
count-‐rate.
NB:
In
case
of
self-‐activity,
the
spectrum
is
the
results
of
convolution
of
beta-‐ continuous
spectrum
(always)
with
1,
or
plus,
gamma-‐rays
(modulated
by
the
sensitivity
of
that
energies)
Correction
for
image
non-‐uniformity
Images
shows
less
non-‐uniformity
at
the
edges
Light
field
image
and
image
profile
12. CRY019
IMAGE
CALIBRATION
@511KEV
Methods:
1
mm
diameter
Na22
free
source
was
used
to
measure
spatial
resolution
(SR)
and
position
linearity
-‐ Linearity
=
1cm
step
scanning
results
in
about
(2.5-‐3)
pixels
-‐ Field
of
view:
about
60
mm
(far
less
that
what
expected!)
1
cm
step
scanning
Results:
Na22
source
imaged
as
a
line
source
ER%
=
1/5.4
=
18%
@
511keV
Na22
measured
pulse
height
spectrum
511keV
-‐
(15-‐20)%
ERFWHM
NB.Since the
very
low
activity,
PH
spectrum
and
images
were
obtained
by
subtraction
of
an
equivalent
background.
#1
#2
#3
#4
#5
13. CRY019
CRYSTAL:
WATER
PHANTOM
EXPERIMENT
Proton
energy
(MeV)
WATER:
BP
depth
(cm)
PMMA:
BP
depth
130 12.6 10.7
135 13.5 11.4
145 15.3 12.9
Collimator
aligned
to
“see”
at
“12.5
cm
depth”
Proton&
beam
expected&BP
Detector&
“plane”
phantom
IPRD16
-‐ Siena,
3-‐6/October
14. Results:
Proton
beam
monitoring
As
function
of
proton
Energy
12
Proton&
beam
expected&BP
Detector&
“plane”
phantom
Note:
inverse
projection
15. uFoV of
the
gamma
camera
Centered
at
12.5
cm
deep
IMAGE
PROFILE
AT
135MEV
Proton
beam
60x60
image
digit.,
Peak
of
gamma
at
pixel=29±1,
that
correspond
to
the
center
of
the
FoV
that
was
set
at
12.5
cm
Polynomial
fit
to
identify
the
maximum
IPRD16
-‐ Siena,
3-‐6/October
16. NEW
EXPERIMENT:
50X50
LFS
CRYSTAL
– PMMA
PHANTOM
Proton
energy
(MeV)
WATER:
BP
depth
PMMA:
BP
depth
(cm)
130 12.6 10.7
135 13.5 11.4
140 14.4 12.2
145 15.3 12.9
150 16.2 13.7
155 17.2 14.5
160 18.1 15.4
Collimator
centered
To
“see”
at
“13
cm
depth”
Proton&
beam
expected&BP
Detector&
“plane”
phantom
IPRD16
-‐ Siena,
3-‐6/October
17. LFS
IMAGE
CALIBRATION
Methods:
1mm
diameter
Co57
collimated
source
3mm
scanning
step
scanning
to
measure
spatial
resolution
(SR)
and
linearity
LFS
natural
background
(from
Lu178
decay)
3
mm
New
image
digit
60x60,
1.2mm
=1px.
When
using
the
knife-‐edge
collimator,
this
number
become
1px=2.4mm
(M=2:1)
50
>
200
FoV with
#13
spot
which
corresponds
to
about
40mm
linearity:
Digit
250x250
>>
250um
=
1px
18. GAMMA
PROMPT
IN
PMMA
PHANTOM
Polynomial
fit
to
identify
the
peak
of
the
emission
Centered
at
12.5
cm
deep
Image
profile
of
the
central
FoV
IPRD16
-‐ Siena,
3-‐6/October
19. E
(MeV)
Expected
BP “deep”
(cm)
“Estimated gamma
peak” (cm)*
Estimated BP
position in cm
(+12 mm of
column #3)
140 12.2 cm 13-‐2.1
=
10.9± 0.3 12.1 ± 0.3
150 13.7 cm 13-0.7 = 12.3± 0.3 13.5 ± 0.3
160 15.4 cm 13+0.7 = 13.7± 0.3 14.9 ± 0.3
*From
the
polynomial
fit
Comparison
at
150MeV:
profile
of
gamma
and
Profile
obtained
by
closing
the
collimator
IPRD16
-‐ Siena,
3-‐6/October
20. 3RD EXPERIMENT:
TRANSLATE
THE
PHANTOM
AT
FIXED
PROTON
ENERGY
Metod:
Ø 5
mm
step
translation
of
the
phantom
Ø Collimator
aligned
at
13
cm
Ø Proton
energy
150MeV
–>
exp.
BP
at
13.7
cm
Result:
The
profile
of
gamma
“moves”
As
function
of
the
translation
of
the
Phantom.
Polinomial fit
IPRD16
-‐ Siena,
3-‐6/October
21. #
Energies
(MeV)
Collimator
configuration
Expected
BP
position
(cm)
Measured
BP
Count-‐
rate
(cps)
notes
2 110 Knife edge 9.1 Out
of
FoV ⋍21’000 0.3
nA
3 120 ‘’ 10.7 na ⋍25’000
4 135* ‘’ 13.1 13.0
cm ⋍33’000 Critical
count-‐rate
5 145 ‘’ 14.9 na ⋍39’000 Critical
count-‐rate
6 230 ‘’ >20 na ⋍47’000
(!)
Excess
of
count/rate
#
Energies
(MeV)
Collimator
config.
Expected
BP
position
(cm)
Extimated BP
(cm)
Count-‐
rate
(cps)
notes
2 130 Knife edge 10.7 Out
of
FoV ⋍18’000 0.5
nA
3 135 ‘’ 11.4 na ⋍19’700
4 140* ‘’ 12.2 12.1 ⋍20’000
5 145 ‘’ 12.9 ⋍22’000
6 150* ‘’ 13.7 13.5 ⋍23’000
7 155 ‘’ 14.5 ⋍24’000
8 160* “ 15.4 14.9 ⋍25’000
LFS
crystal
&
PMMA
phantom
Cry019
crystal
&
Water
phantom
*
Measurement
was
also
performed
by
closing
the
collimator
IPRD16
-‐ Siena,
3-‐6/October
22. CONCLUSION
• Results
seems
promising
to
realize
an
imaging
device
for
online
monitoring
proton
therapy,
even
though
count-‐rate
remain
a
critical
point
(max
current
is
far
from
the
clinical
dose
rate).
• Cry019
shows
higher
image
contrast
than
LFS,
but
is
limited
in
FoV
and
sensitivity
Future
works
(among
others):
• More
and
more
simulation
>>
to
assess
the
accuracy
of
the
results
• Design
an
improved
imaging
system
(collimator,
detector
and
geometry)
• Image
and
spectral
analysis
>>
remove
double
hit
and
improve
positioning
IPRD16
-‐ Siena,
3-‐6/October
23. ACKNOWLEDGEMENTS
• Skandion Cliniken,
Uppsala
Sweden
• Alexandru Dasu
• KTH
STH
group,
Stockholm
• Massimiliano
Colarieti Tosti
• Gustaf Lönn
• David
Larsson
• La
Sapienza
University,
Rome
Italy
• Roberto
Pani
• Roma
Tre
University,
Rome
Italy
• Andrea
Fabbri
• Francesco
De
Notaristefani
Work
supported
by
Stockholm
Country
Council
(SLL)
IPRD16
-‐ Siena,
3-‐6/October