. The objective of this paper is to configure our cosmic ray detector so that we can see muons. By establishing our ability to count muons we can conduct different experiments to extend our understanding of the effect of cosmic rays.
The document summarizes a gamma ray spectroscopy lab experiment. Key findings include:
- Gamma rays from various radioactive samples were measured using a sodium iodide detector and spectrometer interface.
- A linear relationship was found between the gamma ray energies and their channel numbers on the spectrometer.
- All major gamma ray interactions (photoelectric effect, Compton scattering) were observed except pair production which requires higher energies.
- The unknown isotope was identified as Cesium-137 based on its measured energy of 655.5 keV, though the author initially disagreed with this assessment.
Microwave radiation anomaly of Wenchuan earthquake and its mechanism.pptgrssieee
The document presents a study on microwave radiation anomalies before the 2008 Wenchuan earthquake in China. A new method is proposed to extract microwave radiation anomalies from satellite data by eliminating effects of terrain and weather. Analysis found positive microwave anomalies from 40 days to 2 days before the earthquake near the epicenter. Experimental work on rock samples under loading showed that microwave radiation increases in the fracturing stage, providing a potential explanation for the observed pre-earthquake microwave anomalies.
1) The experiment used gamma-ray spectroscopy to analyze spectra from various radioactive sources. Spectra were recorded at different photomultiplier tube voltages to study resolution and efficiency.
2) Analysis found the number of dynodes in the photomultiplier tube to be 6.5, and resolution R was determined to be inversely proportional to gamma ray energy as expected.
3) Activity of a potassium chloride sample was estimated using detector efficiency calculations, finding 1.7×10^17 40K nuclei, consistent with the expected amount.
Problemas (43 Pág. - 107 Probl.) de Carga Eléctrica y Campo Eléctrico - SearsLUIS POWELL
This document discusses electric charge and electric fields through examples applying Coulomb's law. It provides calculations of forces between charged objects, determining net forces and accelerations. Key points include:
- Calculating the number of electrons needed to produce a given net charge on an object.
- Using mass and atomic mass to determine numbers of atoms and electrons in objects.
- Applying Coulomb's law to calculate forces and accelerations between two or more point charges.
- Finding vector sums of forces to determine net force and direction on a charge from multiple other charges.
1) Light displays both wave-like and particle-like properties, known as wave-particle duality. It will behave as a wave in experiments measuring wave properties such as interference and diffraction, and as a particle in experiments measuring particle properties such as in Compton scattering.
2) In 1924, Louis de Broglie postulated that all matter has an intrinsic wavelength that is related to its momentum, not just light. He derived that the wavelength λ of a particle with momentum p is given by λ = h/p, where h is Planck's constant.
3) De Broglie's hypothesis established the wave-like nature of matter and was pivotal in the development of quantum mechanics,
Measurement of the Lifetime of the 59.5keV excited State of 237Np from the Al...theijes
This document summarizes an experiment that measured the lifetime of the 59.5keV excited state of 237Np using delayed coincidence techniques. 241Am decays via alpha emission to both the 103keV and 59.5keV excited states of 237Np. The lifetime of the 59.5keV state was measured by detecting coincidences between alpha particles from 241Am decay and gamma rays from the decay of the 59.5keV state. A plastic scintillator detector was used to detect alpha particles and another thicker plastic scintillator was used to detect gamma rays. The measured lifetime of the 59.5keV state was 66 nanoseconds, close to the accepted value of 67 nanoseconds. Delayed coincidence methods provide an efficient way to study short-lived
The document summarizes a gamma ray spectroscopy lab experiment. Key findings include:
- Gamma rays from various radioactive samples were measured using a sodium iodide detector and spectrometer interface.
- A linear relationship was found between the gamma ray energies and their channel numbers on the spectrometer.
- All major gamma ray interactions (photoelectric effect, Compton scattering) were observed except pair production which requires higher energies.
- The unknown isotope was identified as Cesium-137 based on its measured energy of 655.5 keV, though the author initially disagreed with this assessment.
Microwave radiation anomaly of Wenchuan earthquake and its mechanism.pptgrssieee
The document presents a study on microwave radiation anomalies before the 2008 Wenchuan earthquake in China. A new method is proposed to extract microwave radiation anomalies from satellite data by eliminating effects of terrain and weather. Analysis found positive microwave anomalies from 40 days to 2 days before the earthquake near the epicenter. Experimental work on rock samples under loading showed that microwave radiation increases in the fracturing stage, providing a potential explanation for the observed pre-earthquake microwave anomalies.
1) The experiment used gamma-ray spectroscopy to analyze spectra from various radioactive sources. Spectra were recorded at different photomultiplier tube voltages to study resolution and efficiency.
2) Analysis found the number of dynodes in the photomultiplier tube to be 6.5, and resolution R was determined to be inversely proportional to gamma ray energy as expected.
3) Activity of a potassium chloride sample was estimated using detector efficiency calculations, finding 1.7×10^17 40K nuclei, consistent with the expected amount.
Problemas (43 Pág. - 107 Probl.) de Carga Eléctrica y Campo Eléctrico - SearsLUIS POWELL
This document discusses electric charge and electric fields through examples applying Coulomb's law. It provides calculations of forces between charged objects, determining net forces and accelerations. Key points include:
- Calculating the number of electrons needed to produce a given net charge on an object.
- Using mass and atomic mass to determine numbers of atoms and electrons in objects.
- Applying Coulomb's law to calculate forces and accelerations between two or more point charges.
- Finding vector sums of forces to determine net force and direction on a charge from multiple other charges.
1) Light displays both wave-like and particle-like properties, known as wave-particle duality. It will behave as a wave in experiments measuring wave properties such as interference and diffraction, and as a particle in experiments measuring particle properties such as in Compton scattering.
2) In 1924, Louis de Broglie postulated that all matter has an intrinsic wavelength that is related to its momentum, not just light. He derived that the wavelength λ of a particle with momentum p is given by λ = h/p, where h is Planck's constant.
3) De Broglie's hypothesis established the wave-like nature of matter and was pivotal in the development of quantum mechanics,
Measurement of the Lifetime of the 59.5keV excited State of 237Np from the Al...theijes
This document summarizes an experiment that measured the lifetime of the 59.5keV excited state of 237Np using delayed coincidence techniques. 241Am decays via alpha emission to both the 103keV and 59.5keV excited states of 237Np. The lifetime of the 59.5keV state was measured by detecting coincidences between alpha particles from 241Am decay and gamma rays from the decay of the 59.5keV state. A plastic scintillator detector was used to detect alpha particles and another thicker plastic scintillator was used to detect gamma rays. The measured lifetime of the 59.5keV state was 66 nanoseconds, close to the accepted value of 67 nanoseconds. Delayed coincidence methods provide an efficient way to study short-lived
Cosmic rays originate from outside Earth's atmosphere and are detected using scintillators coupled to photomultiplier tubes (PMTs). The authors characterized each PMT by measuring detection rates while varying threshold levels and applied voltages to determine optimal operating parameters. Threshold scans revealed the minimum voltage required to detect particles above noise, while voltage scans showed detection peaks used to set the high voltage for each PMT. Statistical analysis accounted for measurement uncertainties. Data acquisition software converted pulse readings to binary for computer analysis, with words identifying run numbers and detection channels. Overall, adjusting PMT thresholds and voltages improved the quality of cosmic ray energy data collected.
1. The document describes an experiment to verify Faraday's law of electromagnetic induction by measuring the induced electromotive force in a coil as it passes through a changing magnetic field.
2. The experiment varies both the velocity of the coil by changing the angle it swings through the magnetic field, and the strength of the magnetic field by adjusting the distance between magnet poles.
3. Data on the induced voltage, magnetic field, and angular velocity of the coil is recorded and analyzed to understand the relationships between these variables as described by Faraday's law.
The document describes a lab experiment to measure the Hall effect using an Indium Arsenide sample. Students will apply a magnetic field perpendicular to the current flow and measure the resulting Hall voltage. This will allow them to determine properties like the Hall coefficient, carrier mobility, and doping density. Additionally, the Hall device can be used as a magnetic field sensor by measuring the Hall voltage produced by varying currents through an electromagnet.
Optical interferometery to detect sound waves as an analogue for gravitationa...Thomas Actn
This document describes an experiment using a Michelson interferometer to detect sound waves as an analogue for gravitational waves. A tuning fork resonating at 440Hz and a piezoelectric crystal were used to generate sound waves near one arm of the interferometer. An Arduino and oscilloscope measured the resulting interference patterns. The Arduino detected the tuning fork frequency accurately but the oscilloscope only detected around half the frequency due to its limited sampling. Multiple constituent frequencies were detected from hand claps, mimicking bursts from supernovae. While the setup could detect these 'fake' gravitational waves, its low sampling rate limited the detectable frequency window.
The engineering team measured acceleration data from an elevator in the MEEM building to validate an AMESim model of the elevator. They found the simulation results did not match the experimental data, so the AMESim model was not validated. To improve performance, they increased the proportional gain in the model to 45, which increased the deceleration rate. However, their recommendation was based on an invalid model that did not accurately represent the real elevator.
Ethan conducted a photoelectric effect experiment to calculate Planck's constant. The experiment involved measuring the stopping potential of electrons emitted from a metal surface under monochromatic light of varying wavelengths. Plotting average stopping potential versus the reciprocal of wavelength produced a straight line, from which Planck's constant could be calculated using the slope. Ethan's calculated value of Planck's constant had a 36% error compared to the accepted value, which was within an acceptable range for the experiment.
Performance analysis of bio-Signal processing in ocean Environment using soft...IJECEIAES
Wireless communication has become an essential technology in our day-to-day life both in air and water medium. To monitor the health parameter of human begins, advancement techniques like internet of things is evolved. But to analyze underwater living organisms health parameters, researchers finding difficulties to do so. The reason behind is underwater channels has drawbacks like signal degradation due to multipath propagation, severe ambient noise and Attenuation by bottom and surface loss. In this paper Artificial Neural Networks (ANN) is used to perform data transfer in water medium. A sample EEG signal is generated and trained with 2 and 20 hidden layers. Simulation result showed that error free communication is achieved with 20 hidden layers at 10th iteration. The proposed algorithm is validated using a real time watermark toolbox. Two different modulation scheme was applied along with ANN. In the first scenario, the EEG signal is modulated using convolution code and decoded by Viterbi Algorithm. Multiplexing technique is applied in the second scenario. It is observed that energy level in the order of 40 dB is required for least error rate. It is also evident from simulation result that maximum of 5% CP can be maintained to attain the least Mean Square Error.
This document provides an introduction to radiographic testing (RT). It discusses how RT works by exposing test objects to radiation like X-rays to produce images. RT is used to inspect items like castings and welds. Advantages include the ability to test most materials and provide permanent records, but it has limitations like requiring access to both sides and difficulty detecting some discontinuities. The document also covers safety considerations, personnel qualifications, testing principles like penetration and image quality, and the physics of X-ray and gamma radiation production.
The document summarizes experiments on various wave phenomena including:
- Water wave reflection showing the angle of reflection equals the angle of incidence.
- Water wave refraction as waves pass from deep to shallow water, decreasing wavelength.
- Sound wave reflection also showing the equality of incident and reflection angles.
- Light wave diffraction seen through single slits of varying widths, showing diffraction patterns.
- Sound and light wave interference seen as alternating loud/soft bands and bright/dark fringes.
The document summarizes an experiment conducted by a group to construct and study the behavior of a Schmitt Trigger circuit. The group used various equipment like a breadboard, function generator, multimeter, oscilloscope and power supply to build the circuit using resistors ranging from 140-1000 ohms and capacitors. They observed the output signal on an oscilloscope and noted that increasing the resistor size increased the time delay of the circuit. Testing different frequencies, they saw noise at higher frequencies. Finally, they estimated the switching speed of their constructed circuit to be about 50 ± 10 μs.
Identify the possibility of predication of seismic activity through the ionos...ashrafrateb1985
The document summarizes research using data from the DEMETER microsatellite to study possible links between seismic activity and ionospheric disturbances. It presents two case studies: 1) Unusual ionospheric observations detected by DEMETER over Japan days before a 2004 earthquake. Spectrograms showed electromagnetic perturbations. 2) Observations by DEMETER of ultra-low and extremely low frequency emissions one day before a 2004 Indonesia earthquake, including anomalies in the electric field and ELF magnetic field variations. The document examines the satellite's scientific objectives, instruments, and operation modes to systematically search for seismic-related signals in the ionosphere.
This document contains the results of 6 tasks measuring electrical signals using an oscilloscope and function generator. In task 1, sinusoidal and square waves were output and analyzed. Task 3 measured inductance over 4 coils. Task 4 examined the relationship between period and time constant for a capacitor and resistor. Task 5 tested voltage readings at varying frequencies. Task 6 measured voltage, current, capacitor resistance, and phase shift between signals at different frequencies.
Axion Dark Matter Experiment Detailed Design Nbsp And OperationsSandra Long
The document discusses the Axion Dark Matter eXperiment (ADMX) and details its recent technological advances that have improved its sensitivity to detecting dark matter axions. Key advances include implementing state-of-the-art quantum amplifiers like a Microstrip SQUID Amplifier (Run 1A) and Josephson Parametric Amplifier (Run 1B) as well as a dilution refrigerator to reduce cavity temperature. These allowed ADMX to set the most stringent limits to date on axion dark matter in the 2.66-3.1 μeV mass range with DFSZ coupling sensitivity. The document also describes the ADMX detector setup and cavity design used to search for axion-photon conversion signals.
1. Edwin Hall discovered the Hall effect in 1879 while working on his doctoral degree at Johns Hopkins University. Through his measurements of a tiny effect produced using apparatus he designed, he published findings about a new interaction between magnets and electric currents eighteen years before the electron was discovered.
2. The Hall effect is the production of a voltage difference across an electrical conductor, perpendicular to both the current in the conductor and an applied magnetic field. This effect can be used to determine various properties of the conductor such as carrier concentration and Hall coefficient.
3. Applications of the Hall effect include speed detection, current sensing, magnetic field sensing as in magnetometers, and position sensing in devices like brushless DC motors.
The document summarizes an experiment to determine the velocity of ultrasonic waves in benzene liquid using an ultrasonic interferometer. It describes the apparatus used, which includes an ultrasonic cell, high frequency generator, and piezoelectric crystal to generate ultrasound. It presents the key formulas for wavelength, velocity, and compressibility. The procedure and observations are provided in tables. The results found the ultrasonic velocity in benzene to be 1204±8 m/s and the compressibility to be 7.9±0.1 N/m2.
Introduction to Oscilloscope and Function generatorcyberns_
This document provides instructions for a lab experiment using an oscilloscope and function generator. It begins with prelab questions about the difference between peak and peak-to-peak voltage, relating period and frequency, and using cursor positions to measure voltages and periods of waveforms. Students are then asked to use the equipment to generate and measure a sinusoidal waveform, explore the effects of frequency, and measure the output of a simple RC circuit driven by the function generator. Reference material is provided explaining the basic functions of an oscilloscope and function generator.
1) The document describes an experiment to determine how mass affects the terminal velocity of falling objects. Terminal velocity occurs when the downward force of gravity equals the upward force of drag.
2) Cupcake holders of varying masses were dropped from a height of 2 meters, and their terminal velocities were measured. Masses ranged from 0.00068kg to 0.00136kg.
3) The results showed a proportional relationship between mass and terminal velocity, supporting the hypothesis. However, uncertainties were too large to have high confidence in the data. Improvements for future experiments are discussed.
The document is a daily lesson log for a Grade 11 physics class. It summarizes the objectives, content, learning resources, and procedures for four class sessions on topics including LC circuits, electric charge, electric fields, and electromagnetic waves. The objectives are for students to understand concepts like inductance, capacitance, Coulomb's law, and properties of waves. Class activities include reviewing concepts, analyzing examples, group problem-solving, and quantitative discussions to reinforce understanding.
The team detected signals from the Magellanic Stream using the 4.5m radio telescope at Leuschner Observatory. Images of the observed region in galactic coordinates showed high-velocity gases from -100 to -350 km/s, consistent with the Magellanic Stream. A velocity map matched previous studies, and higher intensities near the galactic pole aligned with expectations. Issues with intensity calibration and single polarization data collection impacted accuracy but detection of the stream was achieved.
Tingting Xu has experience with several biomedical research projects involving experiments and image processing. These include:
1. Using cellulose acetate electrophoresis to separate serum proteins as a teaching assistant. This involved designing and conducting the experiment, then teaching other students.
2. Preparing E. coli for competence and transforming it with plasmid DNA to learn the process. Control experiments showed successful transformation.
3. Linking concanavalin A to quantum dots via bovine serum albumin as a bridge. Electrophoresis showed successful conjugation.
4. Developing a method to visualize the propagating speed of cortical spreading depression in rat cortex in 2D using optical imaging and correlation analysis. Control experiments validated
Resource list for Noora Aabad's AI presentation. Ethical AI is a shared responsibility. Students, teachers, users, programmers, investors, regulators, and others all play a role in determining the future of AI technology development and use. This session will feature an innovative and interactive approach to a virtual panel, giving both panelists and attendees the opportunity to interact and respond to various AI scenarios and activities. While the moderator and panelists demonstrate and discuss on-screen, attendees also have the opportunity to share their own insights, observations, and questions in a moderated chat.
ALDI is working to make its business more sustainable through reducing plastic usage, increasing recyclability, cutting carbon emissions, reducing food waste, and sourcing products responsibly. Some key initiatives include committing to eliminate all plastic shopping bags by 2023, making over 60% of exclusive packaging reusable/recyclable, offsetting 100% of energy usage with renewable sources, and requiring 53% of coffee to come from sustainable sources. ALDI also donates food to food banks and other charitable causes to support communities.
Cosmic rays originate from outside Earth's atmosphere and are detected using scintillators coupled to photomultiplier tubes (PMTs). The authors characterized each PMT by measuring detection rates while varying threshold levels and applied voltages to determine optimal operating parameters. Threshold scans revealed the minimum voltage required to detect particles above noise, while voltage scans showed detection peaks used to set the high voltage for each PMT. Statistical analysis accounted for measurement uncertainties. Data acquisition software converted pulse readings to binary for computer analysis, with words identifying run numbers and detection channels. Overall, adjusting PMT thresholds and voltages improved the quality of cosmic ray energy data collected.
1. The document describes an experiment to verify Faraday's law of electromagnetic induction by measuring the induced electromotive force in a coil as it passes through a changing magnetic field.
2. The experiment varies both the velocity of the coil by changing the angle it swings through the magnetic field, and the strength of the magnetic field by adjusting the distance between magnet poles.
3. Data on the induced voltage, magnetic field, and angular velocity of the coil is recorded and analyzed to understand the relationships between these variables as described by Faraday's law.
The document describes a lab experiment to measure the Hall effect using an Indium Arsenide sample. Students will apply a magnetic field perpendicular to the current flow and measure the resulting Hall voltage. This will allow them to determine properties like the Hall coefficient, carrier mobility, and doping density. Additionally, the Hall device can be used as a magnetic field sensor by measuring the Hall voltage produced by varying currents through an electromagnet.
Optical interferometery to detect sound waves as an analogue for gravitationa...Thomas Actn
This document describes an experiment using a Michelson interferometer to detect sound waves as an analogue for gravitational waves. A tuning fork resonating at 440Hz and a piezoelectric crystal were used to generate sound waves near one arm of the interferometer. An Arduino and oscilloscope measured the resulting interference patterns. The Arduino detected the tuning fork frequency accurately but the oscilloscope only detected around half the frequency due to its limited sampling. Multiple constituent frequencies were detected from hand claps, mimicking bursts from supernovae. While the setup could detect these 'fake' gravitational waves, its low sampling rate limited the detectable frequency window.
The engineering team measured acceleration data from an elevator in the MEEM building to validate an AMESim model of the elevator. They found the simulation results did not match the experimental data, so the AMESim model was not validated. To improve performance, they increased the proportional gain in the model to 45, which increased the deceleration rate. However, their recommendation was based on an invalid model that did not accurately represent the real elevator.
Ethan conducted a photoelectric effect experiment to calculate Planck's constant. The experiment involved measuring the stopping potential of electrons emitted from a metal surface under monochromatic light of varying wavelengths. Plotting average stopping potential versus the reciprocal of wavelength produced a straight line, from which Planck's constant could be calculated using the slope. Ethan's calculated value of Planck's constant had a 36% error compared to the accepted value, which was within an acceptable range for the experiment.
Performance analysis of bio-Signal processing in ocean Environment using soft...IJECEIAES
Wireless communication has become an essential technology in our day-to-day life both in air and water medium. To monitor the health parameter of human begins, advancement techniques like internet of things is evolved. But to analyze underwater living organisms health parameters, researchers finding difficulties to do so. The reason behind is underwater channels has drawbacks like signal degradation due to multipath propagation, severe ambient noise and Attenuation by bottom and surface loss. In this paper Artificial Neural Networks (ANN) is used to perform data transfer in water medium. A sample EEG signal is generated and trained with 2 and 20 hidden layers. Simulation result showed that error free communication is achieved with 20 hidden layers at 10th iteration. The proposed algorithm is validated using a real time watermark toolbox. Two different modulation scheme was applied along with ANN. In the first scenario, the EEG signal is modulated using convolution code and decoded by Viterbi Algorithm. Multiplexing technique is applied in the second scenario. It is observed that energy level in the order of 40 dB is required for least error rate. It is also evident from simulation result that maximum of 5% CP can be maintained to attain the least Mean Square Error.
This document provides an introduction to radiographic testing (RT). It discusses how RT works by exposing test objects to radiation like X-rays to produce images. RT is used to inspect items like castings and welds. Advantages include the ability to test most materials and provide permanent records, but it has limitations like requiring access to both sides and difficulty detecting some discontinuities. The document also covers safety considerations, personnel qualifications, testing principles like penetration and image quality, and the physics of X-ray and gamma radiation production.
The document summarizes experiments on various wave phenomena including:
- Water wave reflection showing the angle of reflection equals the angle of incidence.
- Water wave refraction as waves pass from deep to shallow water, decreasing wavelength.
- Sound wave reflection also showing the equality of incident and reflection angles.
- Light wave diffraction seen through single slits of varying widths, showing diffraction patterns.
- Sound and light wave interference seen as alternating loud/soft bands and bright/dark fringes.
The document summarizes an experiment conducted by a group to construct and study the behavior of a Schmitt Trigger circuit. The group used various equipment like a breadboard, function generator, multimeter, oscilloscope and power supply to build the circuit using resistors ranging from 140-1000 ohms and capacitors. They observed the output signal on an oscilloscope and noted that increasing the resistor size increased the time delay of the circuit. Testing different frequencies, they saw noise at higher frequencies. Finally, they estimated the switching speed of their constructed circuit to be about 50 ± 10 μs.
Identify the possibility of predication of seismic activity through the ionos...ashrafrateb1985
The document summarizes research using data from the DEMETER microsatellite to study possible links between seismic activity and ionospheric disturbances. It presents two case studies: 1) Unusual ionospheric observations detected by DEMETER over Japan days before a 2004 earthquake. Spectrograms showed electromagnetic perturbations. 2) Observations by DEMETER of ultra-low and extremely low frequency emissions one day before a 2004 Indonesia earthquake, including anomalies in the electric field and ELF magnetic field variations. The document examines the satellite's scientific objectives, instruments, and operation modes to systematically search for seismic-related signals in the ionosphere.
This document contains the results of 6 tasks measuring electrical signals using an oscilloscope and function generator. In task 1, sinusoidal and square waves were output and analyzed. Task 3 measured inductance over 4 coils. Task 4 examined the relationship between period and time constant for a capacitor and resistor. Task 5 tested voltage readings at varying frequencies. Task 6 measured voltage, current, capacitor resistance, and phase shift between signals at different frequencies.
Axion Dark Matter Experiment Detailed Design Nbsp And OperationsSandra Long
The document discusses the Axion Dark Matter eXperiment (ADMX) and details its recent technological advances that have improved its sensitivity to detecting dark matter axions. Key advances include implementing state-of-the-art quantum amplifiers like a Microstrip SQUID Amplifier (Run 1A) and Josephson Parametric Amplifier (Run 1B) as well as a dilution refrigerator to reduce cavity temperature. These allowed ADMX to set the most stringent limits to date on axion dark matter in the 2.66-3.1 μeV mass range with DFSZ coupling sensitivity. The document also describes the ADMX detector setup and cavity design used to search for axion-photon conversion signals.
1. Edwin Hall discovered the Hall effect in 1879 while working on his doctoral degree at Johns Hopkins University. Through his measurements of a tiny effect produced using apparatus he designed, he published findings about a new interaction between magnets and electric currents eighteen years before the electron was discovered.
2. The Hall effect is the production of a voltage difference across an electrical conductor, perpendicular to both the current in the conductor and an applied magnetic field. This effect can be used to determine various properties of the conductor such as carrier concentration and Hall coefficient.
3. Applications of the Hall effect include speed detection, current sensing, magnetic field sensing as in magnetometers, and position sensing in devices like brushless DC motors.
The document summarizes an experiment to determine the velocity of ultrasonic waves in benzene liquid using an ultrasonic interferometer. It describes the apparatus used, which includes an ultrasonic cell, high frequency generator, and piezoelectric crystal to generate ultrasound. It presents the key formulas for wavelength, velocity, and compressibility. The procedure and observations are provided in tables. The results found the ultrasonic velocity in benzene to be 1204±8 m/s and the compressibility to be 7.9±0.1 N/m2.
Introduction to Oscilloscope and Function generatorcyberns_
This document provides instructions for a lab experiment using an oscilloscope and function generator. It begins with prelab questions about the difference between peak and peak-to-peak voltage, relating period and frequency, and using cursor positions to measure voltages and periods of waveforms. Students are then asked to use the equipment to generate and measure a sinusoidal waveform, explore the effects of frequency, and measure the output of a simple RC circuit driven by the function generator. Reference material is provided explaining the basic functions of an oscilloscope and function generator.
1) The document describes an experiment to determine how mass affects the terminal velocity of falling objects. Terminal velocity occurs when the downward force of gravity equals the upward force of drag.
2) Cupcake holders of varying masses were dropped from a height of 2 meters, and their terminal velocities were measured. Masses ranged from 0.00068kg to 0.00136kg.
3) The results showed a proportional relationship between mass and terminal velocity, supporting the hypothesis. However, uncertainties were too large to have high confidence in the data. Improvements for future experiments are discussed.
The document is a daily lesson log for a Grade 11 physics class. It summarizes the objectives, content, learning resources, and procedures for four class sessions on topics including LC circuits, electric charge, electric fields, and electromagnetic waves. The objectives are for students to understand concepts like inductance, capacitance, Coulomb's law, and properties of waves. Class activities include reviewing concepts, analyzing examples, group problem-solving, and quantitative discussions to reinforce understanding.
The team detected signals from the Magellanic Stream using the 4.5m radio telescope at Leuschner Observatory. Images of the observed region in galactic coordinates showed high-velocity gases from -100 to -350 km/s, consistent with the Magellanic Stream. A velocity map matched previous studies, and higher intensities near the galactic pole aligned with expectations. Issues with intensity calibration and single polarization data collection impacted accuracy but detection of the stream was achieved.
Tingting Xu has experience with several biomedical research projects involving experiments and image processing. These include:
1. Using cellulose acetate electrophoresis to separate serum proteins as a teaching assistant. This involved designing and conducting the experiment, then teaching other students.
2. Preparing E. coli for competence and transforming it with plasmid DNA to learn the process. Control experiments showed successful transformation.
3. Linking concanavalin A to quantum dots via bovine serum albumin as a bridge. Electrophoresis showed successful conjugation.
4. Developing a method to visualize the propagating speed of cortical spreading depression in rat cortex in 2D using optical imaging and correlation analysis. Control experiments validated
Resource list for Noora Aabad's AI presentation. Ethical AI is a shared responsibility. Students, teachers, users, programmers, investors, regulators, and others all play a role in determining the future of AI technology development and use. This session will feature an innovative and interactive approach to a virtual panel, giving both panelists and attendees the opportunity to interact and respond to various AI scenarios and activities. While the moderator and panelists demonstrate and discuss on-screen, attendees also have the opportunity to share their own insights, observations, and questions in a moderated chat.
ALDI is working to make its business more sustainable through reducing plastic usage, increasing recyclability, cutting carbon emissions, reducing food waste, and sourcing products responsibly. Some key initiatives include committing to eliminate all plastic shopping bags by 2023, making over 60% of exclusive packaging reusable/recyclable, offsetting 100% of energy usage with renewable sources, and requiring 53% of coffee to come from sustainable sources. ALDI also donates food to food banks and other charitable causes to support communities.
A Mexican scientist discusses his background in biology and palaeontology. He became interested in computer science through secondary school classes and seeing his father work as a programmer. As a palaeontologist, he applies computer science concepts like data science and artificial intelligence to digitize fossils. He emphasizes embracing frustration when learning and believes communication and listening are important for diversity in universities.
Effective CS teachers demonstrate thorough knowledge of CS concepts and integrate them with computational thinking practices. They understand how CS concepts progress across grade levels. Effective CS teachers advocate for equity and inclusion, examine biases, and use student data to improve equity. They also continuously develop their own skills and collaborate with others. Effective CS teachers design engaging, standards-aligned learning experiences that meet student needs and build self-efficacy in CS through inquiry-based learning and student collaboration.
The document provides a list of 14 resources related to STEM education and careers. These include the website and social media accounts for the STEM Impressionists Program (SIP), links to SIP members' LinkedIn profiles, extracurricular activities, competitions, scholarships, college application portals, top employability skills, coding resources, funding opportunities, SIP member resumes, STEM-related holidays, information on ethics in technology, and organizations that support women in STEM.
The document announces a one-day virtual event hosted by the STEM Impressionists Program on August 14th from 10am to 3pm EST for middle and high school girls. It will feature introductory classes on Scratch programming, machine learning, and intro to Python to encourage participation in STEM fields. Interested students can register for the event at the provided link.
Tanisha Dhami has extensive experience in STEM fields such as programming, mathematics, and physics competitions and courses. She has a strong academic background graduating near the top of her class from Vidyashilp Academy in 2020 and is currently studying at Mallya Aditi International School. Her resume highlights leadership roles in math clubs, organizing coding competitions, and simulation projects that demonstrate her skills and passion for STEM subjects.
Pallab Layak is a recent high school graduate with extensive experience in STEM fields such as mathematics, computer science, and data analytics. He has achieved high scores on standardized tests and placed in several international and national competitions in mathematics. Pallab has taken numerous online courses through platforms like Coursera and Wharton covering topics like machine learning, data analytics, programming, and physics. He has held leadership positions in math and coding clubs and has experience mentoring others and organizing programming.
Noora Aabed is a 2022 graduate of Henry Ford Early College in Detroit, Michigan with a 3.95 GPA. She has extensive experience in STEM fields through coding courses and camps, presenting at hackathons and seminars, competing in STEM competitions, and volunteering for various STEM and humanitarian organizations. Her experience includes projects in quantum computing, international ambassadorship, and rotations at Henry Ford Health System. References are available upon request.
This document lists various science, technology, engineering, arts, and math (STEAM) related days and weeks that occur throughout the year. Some of the notable events mentioned include Environment Day on June 5th, International Women in Engineering Day on June 23rd, the anniversary of the Moon Landing on July 20th, National Robotics Week from April 4-10th, Earth Day on April 22nd, and National Pluto isn't a Planet Day on June 24th. The document also notes that February is National Inventors Month and the week of February 21st is National Engineering Week.
Starting With Scratch is a block-based programming course provided by the CodeTigers and STEM Impressionists Program collaboration. Over the course of 10 weeks, students will practice programming on Scratch while simultaneously learning fundamental computer science concepts. Each week will be taught by two student mentors who will walk participants through different lessons that will overtime build their understanding of coding through the Scratch platform. Throughout the course, students will be provided with resources to further their exploration of computer science in addition to preparing them to continue on to other coding platforms such as Python, micro:bit, and HTML/CSS. YouTube class: https://www.youtube.com/watch?
Register for the Coolest Project Competition!Angela DeHart
This document lists the details of how to register for Raspberry Pi's International competition. All of the information was obtained from their website. Please double-check the website as the information that is covered in this document may have changed since it was posted. We do not want you to miss out on the competition! (Document posted April 25, 2021).
Starting With Scratch is a block-based programming course provided by the CodeTigers and STEM Impressionists Program collaboration. Over the course of 10 weeks, students will practice programming on Scratch while simultaneously learning fundamental computer science concepts. Each week will be taught by two student mentors who will walk participants through different lessons that will overtime build their understanding of coding through the Scratch platform. Throughout the course, students will be provided with resources to further their exploration of computer science in addition to preparing them to continue on to other coding platforms such as Python, micro:bit, and HTML/CSS. YouTube class: https://www.youtube.com/watch?
Starting With Scratch is a block-based programming course provided by the CodeTigers and STEM Impressionists Program collaboration. Over the course of 10 weeks, students will practice programming on Scratch while simultaneously learning fundamental computer science concepts. Each week will be taught by two student mentors who will walk participants through different lessons that will overtime build their understanding of coding through the Scratch platform. Throughout the course, students will be provided with resources to further their exploration of computer science in addition to preparing them to continue on to other coding platforms such as Python, micro:bit, and HTML/CSS. YouTube class: https://www.youtube.com/watch?
Coolest Projects online is the world’s leading technology showcase for young people. If you enjoy making things with technology, Coolest Projects online is an amazing opportunity to get creative, have fun, and celebrate what you have made.
Your creation will be showcased in the Coolest Projects online gallery, for people all over the world to see! Coolest Projects online is free, it is open to anyone up to the age of 18, and you can join in wherever you are in the world.
Abia Zahir is a 2021 graduate of Annandale High School interested in studying computer science. She has extensive experience in computer science and robotics through numerous online courses and certifications. She has organized and participated in many STEM outreach and competition events. She also has leadership experience through involvement with clubs like NSBE and internships like planning a STEM conference for parents and children. Her resume demonstrates strong qualifications for computer science through academic achievement, projects, and recognition.
Starting With Scratch is a block-based programming course provided by the CodeTigers and STEM Impressionists Program collaboration. Over the course of 10 weeks, students will practice programming on Scratch while simultaneously learning fundamental computer science concepts. Each week will be taught by two student mentors who will walk participants through different lessons that will overtime build their understanding of coding through the Scratch platform. Throughout the course, students will be provided with resources to further their exploration of computer science in addition to preparing them to continue on to other coding platforms such as Python, micro:bit, and HTML/CSS. YouTube class: https://www.youtube.com/watch?
Gender and Mental Health - Counselling and Family Therapy Applications and In...PsychoTech Services
A proprietary approach developed by bringing together the best of learning theories from Psychology, design principles from the world of visualization, and pedagogical methods from over a decade of training experience, that enables you to: Learn better, faster!
Main Java[All of the Base Concepts}.docxadhitya5119
This is part 1 of my Java Learning Journey. This Contains Custom methods, classes, constructors, packages, multithreading , try- catch block, finally block and more.
Communicating effectively and consistently with students can help them feel at ease during their learning experience and provide the instructor with a communication trail to track the course's progress. This workshop will take you through constructing an engaging course container to facilitate effective communication.
Chapter wise All Notes of First year Basic Civil Engineering.pptxDenish Jangid
Chapter wise All Notes of First year Basic Civil Engineering
Syllabus
Chapter-1
Introduction to objective, scope and outcome the subject
Chapter 2
Introduction: Scope and Specialization of Civil Engineering, Role of civil Engineer in Society, Impact of infrastructural development on economy of country.
Chapter 3
Surveying: Object Principles & Types of Surveying; Site Plans, Plans & Maps; Scales & Unit of different Measurements.
Linear Measurements: Instruments used. Linear Measurement by Tape, Ranging out Survey Lines and overcoming Obstructions; Measurements on sloping ground; Tape corrections, conventional symbols. Angular Measurements: Instruments used; Introduction to Compass Surveying, Bearings and Longitude & Latitude of a Line, Introduction to total station.
Levelling: Instrument used Object of levelling, Methods of levelling in brief, and Contour maps.
Chapter 4
Buildings: Selection of site for Buildings, Layout of Building Plan, Types of buildings, Plinth area, carpet area, floor space index, Introduction to building byelaws, concept of sun light & ventilation. Components of Buildings & their functions, Basic concept of R.C.C., Introduction to types of foundation
Chapter 5
Transportation: Introduction to Transportation Engineering; Traffic and Road Safety: Types and Characteristics of Various Modes of Transportation; Various Road Traffic Signs, Causes of Accidents and Road Safety Measures.
Chapter 6
Environmental Engineering: Environmental Pollution, Environmental Acts and Regulations, Functional Concepts of Ecology, Basics of Species, Biodiversity, Ecosystem, Hydrological Cycle; Chemical Cycles: Carbon, Nitrogen & Phosphorus; Energy Flow in Ecosystems.
Water Pollution: Water Quality standards, Introduction to Treatment & Disposal of Waste Water. Reuse and Saving of Water, Rain Water Harvesting. Solid Waste Management: Classification of Solid Waste, Collection, Transportation and Disposal of Solid. Recycling of Solid Waste: Energy Recovery, Sanitary Landfill, On-Site Sanitation. Air & Noise Pollution: Primary and Secondary air pollutants, Harmful effects of Air Pollution, Control of Air Pollution. . Noise Pollution Harmful Effects of noise pollution, control of noise pollution, Global warming & Climate Change, Ozone depletion, Greenhouse effect
Text Books:
1. Palancharmy, Basic Civil Engineering, McGraw Hill publishers.
2. Satheesh Gopi, Basic Civil Engineering, Pearson Publishers.
3. Ketki Rangwala Dalal, Essentials of Civil Engineering, Charotar Publishing House.
4. BCP, Surveying volume 1
How to Make a Field Mandatory in Odoo 17Celine George
In Odoo, making a field required can be done through both Python code and XML views. When you set the required attribute to True in Python code, it makes the field required across all views where it's used. Conversely, when you set the required attribute in XML views, it makes the field required only in the context of that particular view.
1. Issues with Plateauing
Our Adventure with Data Collection
Team: Angela DeHart, Joe Boettcher, Ray Hodges, Starre Williams
08/16-17/2018
2018, Angela DeHart
This work is licensed under a Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International License
Cosmic RaysA K-12 Physics Document for teachers
Credit: Simon Swordy (U. Chicago), NASA Image by A. Chantelauze, S. Staffi, and L. Bret
2. QuarkNet Teacher Training
Teaching STEM has inspired me to make myself open to new possibilities. This summer, inspired by the
amazing after-school physics seminar George Mason University shared with the students at Glasgow
Middle School I applied and was accepted into a summer teacher training with Catholic University’s
QuarkNet.
What is QuarkNet? (https://en.wikipedia.org/wiki/QuarkNet)
QuarkNet is a long-term, research-based teacher professional development program in the United States jointly funded by
the National Science Foundation and the US Department of Energy. Since 1999, QuarkNet has established centers at
universities and national laboratories conducting research in particle physics (also called high-energy physics) across the
United States.
Mentor physicists and physics teachers collaborate to bring cutting-edge physics to (middle and) high school classrooms.
QuarkNet offers research experiences for teachers and students, teacher workshops and sustained follow-on support.
Through these activities, teachers enhance their knowledge and understanding of scientific research and transfer this
experience to their classrooms, engaging students in both the substance and processes of contemporary physics research.
3. QuarkNet Teacher Training
This summer we were introduced to QuarkNet’s Cosmic Ray Study.
(https://en.wikipedia.org/wiki/QuarkNet)
The main QuarkNet student investigations supported at the national level are cosmic ray studies. Working with
Fermilab technicians and research physicists, QuarkNet staff has developed a classroom cosmic ray muon detector
that uses the same technologies as the largest detectors at Fermilab and CERN.
To support interschool collaboration, QuarkNet collaborates with the Interactions in Understanding the Universe
Project (I2U2) to develop and support the Cosmic Ray e-Lab.
An e-Lab is a student-led, teacher-guided investigation using experimental data. Students have an opportunity to
organize and conduct authentic research and experience the environment of a scientific collaboration. Participating
schools set up a detector somewhere at the school. Students collect and upload the data to a central server located
at Argonne National Laboratory. Students can access data from all of the detectors in the cluster and use these data
for studies, such as determining the (mean) lifetime of muons, the overall flux of muons in cosmic rays, or a study of
extended air showers.
4. QuarkNet Teacher Training
This document is a summation of project I, and three
other QuarkNet teachers worked on as our culminating
project.* I am going to use this presentation to tell my
students “what I did this summer.”
The purpose of my participation in QuarkNet is to offer
students traditionally underrepresented in STEM an
opportunity to build a cosmic ray muon detector. Collecting
data on the detector will allow the students a chance to
conduct authentic research as well as the opportunity to
collaborate with the other students involved in QuarkNet’s
Cosmic Ray Study. Not only is this opportunity invaluable to
the development of the 7 essential skills needed for the 21st
century learner, it introduces them to the world of global
scientific collaboration.
https://santamariatimes.com/news/local/education/st-century-learning-sailing-
the-seven-c-s/article_0e50cdb0-3c8d-11df-b267-001cc4c002e0.html
* This summation is solely the work of Angela DeHart and may not express the views or understandings of my team
5. Abstract
Cosmic rays1 are still a mystery to us. While we know that cosmic rays they are
coming from outer space and that Earth is being bombarded by thousands of
muons2 every second we have not yet been able to determined the full extent of
the impact muons have on the human body, man-made objects, and/or the
weather. The objective of this paper is to configure our cosmic ray detector so that
we can see muons. By establishing our ability to count muons we can conduct
different experiments to extend our understanding of the effect of cosmic rays.
6. Introduction
The goal of our experiment is to learn the mechanics involved in plateauing3 a
cosmic ray detector4.
In order to achieve our task we have to find the minimum voltage5 necessary
to maximize the signal rate6 while also minimizing the least amount of “noise7”
running through the channel8
8. Procedure
Set Channel 2 at a rate of 2400/minute
-Channel 2 is the reference channel
-2400/minute is the single rate reference value
STEP #1
9. Procedure
A. We need one channel to plateau. We chose to plateau channel 1
-We could have chosen channel 3 or 4
-Any channel, except the reference channel would work
STEP #2
B. We need to choose a starting voltage and then increase the voltage on the multimeter by 0.05 volts
until the coincidence rate remains constant. We choose to start at .50 volts
C. We used a multimeter with the power distribution unit (PDU) to set the voltage of channel 1 to 0.5
volts.
D. We recorded the rates for channel 1, channel 2, and the two fold coincidence rate. We increased
the voltage of channel 1 by 0.05 volts and repeated the measurements of the rates.
E. We continued increasing in the manner until the coincidence rate remained nearly constant (i.e.
reached a plateau).
10. Procedure
A. We need one channel to plateau. We chose to plateau channel 1
-We could have chosen channel 3 or 4
-Any channel, except the reference channel would work
STEP #2
B. We need to choose a starting voltage and then increase the voltage on the multimeter9 by
0.05 volts until the coincidence rate remains constant. We choose .50 volts
C. We used a multimeter with the power distribution unit (PDU)9 to set the voltage of channel 1
to 0.5 volts.
D. We recorded the rates for channel 1, channel 2, and the two fold coincidence rate. We increased
the voltage of channel 1 by 0.05 volts and repeated the measurements of the rates.
E. We continued increasing in the manner until the coincidence rate remained nearly constant (i.e.
reached a plateau).
11. Procedure
A. We need one channel to plateau. We chose to plateau channel 1
-We could have chosen channel 3 or 4
-Any channel, except the reference channel would work
STEP #2
B. We need to choose a starting voltage and then increase the voltage on the multimeter9 by 0.05 volts
until the coincidence rate remains constant. We choose to start at .50 volts
C. We used a multimeter with the power distribution unit (PDU) 9 to set the voltage of channel 1 to 0.5
volts.
D. We recorded the rates for channel 1, channel 2, and the two fold coincidence rate. We
increased the voltage of channel 1 by 0.05 volts and repeated the measurements of the rates.
E. We continued increasing in the manner until the coincidence rate remained nearly constant (i.e.
reached a plateau).
12. **ISSUE!
STEP #2
1) We encountered some unusual data. The channel rate number was
inconsistent
a) The single rate data for channel 1 jumped dramatically – twice.
-1st occurrence: it jumped over 200,000
-2nd occurrence: It jumped over 10,000,000
x confirmation that we had a problem
You can hear us
discussing the
problem in this 42:27
minute video
13. **ISSUE!
STEP #2
2) What was the problem?
a) In order to focus on high probably theories we consulted with our teacher
i. We know that the number of photons produced by muons cannot generate these large
numbers
ii. We know that the tape abound scintillator number 1, where the occurrence happened,
was slightly unglued
iii. We know that the scintillator has to be “light-tight”
iv. So we decided to check the accuracy of the “light-tightness” by covering the scintillator
with a coat
i. If we were correct the single rate data for detector number 1 should immediately
and dramatically drop
http://quarknet.fnal.gov/toolkits/ati/fnaldet.html
14. **ISSUE!
STEP #2
2) Result?
a) We were right!
i. The single rate data for detector number 1
immediately and dramatically dropped
ii. We re-taped the scintillator
iii. We re-tested the data rate – and while it
was still a little high it was accurate enough
for us to continue our experiment
iv. We started collecting data - from scratch
15. **ISSUE!
STEP #2
2) Result?
a) We were right!
i. The single rate data for detector number 1
immediately and dramatically dropped
ii. We re-taped the scintillator
iii. We re-tested the data rate – and while it
was still a little high it was accurate enough
for us to continue our experiment
iv. We started collecting data - from scratch 5,858 increase
12,812 increase
16. Procedure
A. We need one channel to plateau. We chose to plateau channel 1
-We could have chosen channel 3 or 4
-Any channel, except the reference channel would work
STEP #2
B. We need to choose a starting voltage and then increase the voltage on the multimeter9 by 0.05 volts
until the coincidence rate remains constant. We choose to start at .50 volts
C. We used a multimeter with the power distribution unit (PDU) 9 to set the voltage of channel 1 to 0.5
volts.
D. We recorded the rates for channel 1, channel 2, and the two fold coincidence rate. We increased
the voltage of channel 1 by 0.05 volts and repeated the measurements of the rates.
E. We continued increasing in the manner until the coincidence rate remained nearly constant
(i.e. reached a plateau).
17. A. We found the coincidence rate plateau level and
created a plot of the data
B. We then tested voltages at increments smaller than 0.05
volts to get a more precise value for the beginning of the
plateau
C. We determined that the plateau value occurred at 0.692
volts with a rate
D. Then we adjusted the voltage of each of the other 3
channels to obtain a rate of nearly 2960
E. We collected data over night
Procedure
STEP #3
http://physics.ucr.edu/~owen/quarknet/6000CRMD_How_to_Plateau.pdf
18. Procedure
A. We found the coincidence rate plateau level and created
a plot of the data
B. We then tested voltages at increments smaller than
0.05 volts to get a more precise value for the
beginning of the plateau
C. We determined that the plateau value occurred at 0.692
volts with a rate
D. Then we adjusted the voltage of each of the other 3
channels to obtain a rate of nearly 2960
E. We collected data over night
STEP #3
19. Procedure
A. We found the coincidence rate plateau level and created
a plot of the data
B. We then tested voltages at increments smaller than 0.05
volts to get a more precise value for the beginning of the
plateau
C. We determined that the plateau value occurred at
0.692 volts with a rate (NOTE: the final rate is a choice
between a set of close numbers not a numeric default)
D. Then we adjusted the voltage of each of the other 3
channels to obtain a rate of nearly 2960
E. We collected data over night
STEP #3
20. Procedure
A. We found the coincidence rate plateau level and created
a plot of the data
B. We then tested voltages at increments smaller than 0.05
volts to get a more precise value for the beginning of the
plateau
C. We determined that the plateau value occurred at 0.692
volts with a rate
D. Then we adjusted the voltage of each of the other 3
channels to obtain a rate of nearly 2960
(NOTE: You no longer need a reference channel. You now have “the
answer” so ALL the channels are plateaued to the same rate)
E. We collected data over night
STEP #3
21. Procedure
A. We found the coincidence rate plateau level and created
a plot of the data
B. We then tested voltages at increments smaller than 0.05
volts to get a more precise value for the beginning of the
plateau
C. We determined that the plateau value occurred at 0.692
volts with a rate
D. Then we adjusted the voltage of each of the other 3
channels to obtain a rate of nearly 2960
E. We collected data over night
STEP #3
22. Procedure
A. We went to look at our data results:
ISSUE!
B. We uploaded the data we had but made a
“note to file” because of the “high” read of
channel #1
C. DONE!
STEP #4
23. Procedure
A. We went to look at our data results:
ISSUE!
B. We uploaded the data we had but made a
“note to file” because of the “high” read of
channel #1
C. DONE!
STEP #4
24. **ISSUE!
STEP #4
1) We review the possibilities
a. Yesterday there was a “spike” in our data readings around
2:30am (different experiment)
b. The computer was not collecting data when we arrived into
work. The screen was black. We had to wait for the owner
to come and sign in on the computer to see what was going
on
2) We concluded that the electricity must have temporarily stopped
- long enough that the computer, which had no battery, turned
off and went back to the “sign in” screen. With no one to revive
it our data was limited to a 4-hour window
25. Procedure
A. We went to look at our data results:
ISSUE!
B. We uploaded the data we had but made a
“note to file” because of the “high” read of
channel #1
C. DONE!
STEP #4
26. Procedure
A. We went to look at our data results:
ISSUE!
B. We uploaded the data we had but made a
“note to file” because of the “high” read of
channel #1
C. DONE!
STEP #4
27. Procedure
A. We went to look at our data results:
ISSUE!
B. We uploaded the data we had but made a
“note to file” because of the “high” read of
channel #1
C. DONE!
STEP #4
28. Procedure
A. We went to look at our data results:
ISSUE!
B. We uploaded the data we had but made a
“note to file” because of the “high” read of
channel #1
C. DONE!
STEP #4
29. Results
A. The calibration of channel #1 might need to be refined. Results indicated a possible light leak
Experiment:
Experience:
A. The team ended up with challenges that offered us an opportunity to learn:
1. The process for plateauing 4 channels
2. How to use the data feed to determine and resolve a problem with the detector paddle
3. How to write up the non-compliance so that others are aware of non-compliance with our data
4. A list of practical do’s and don’ts when we start the plateauing process again
i. Have a computer with a battery in it so that if the power goes out the battery back up will allow data
to continue to be collected over night
ii. Establishing the initial plateauing number takes about 1.5 hours. Plateauing the remaining paddles
only takes about ½ hour
30. Discussion and Conclusions
Conclusions:
A. When plateauing channels the first time have support
B. The amount of time it takes to plateauing a channel, especially with the amount of down time that is built into
the process, makes it an after school project for dedicated students not an in class project
C. Researching cosmic rays is an amazing, real-world opportunity for middle and high schools students to add
to science’s body of knowledge. It also offers students a fun way to look at and interact with concepts directly
related to physics
D. Internet research has offered an alternative to the 4 channel tool ($4,000). Given the price ($100) differential
and the source of the information (Massachusetts Institute of Technology [MIT]) it is worth trying
1. http://news.mit.edu/2017/handheld-muon-detector-1121
2. http://cosmicwatch.lns.mit.edu/
3. https://github.com/spenceraxani/CosmicWatch-Desktop-Muon-Detector-v2/blob/master/Instructions.pdf
31. Bibliography
Abstract
1. Cosmic Rays
a. https://en.wikipedia.org/wiki/Cosmic_ray
i. Cosmic rays are high-energy radiation, mainly originating outside the Solar System and even from distant
galaxies
2. Muons
a. https://en.wikipedia.org/wiki/Muon
i. Muons arriving on the Earth's surface are created indirectly as decay products of collisions of cosmic rays
with particles of the Earth's atmosphere.
ii. About 10,000 muons reach every square meter of the earth's surface a minute; these charged particles
form as by-products of cosmic rays colliding with molecules in the upper atmosphere. Traveling at
relativistic speeds, muons can penetrate tens of meters into rocks and other matter before attenuating as
a result of absorption or deflection by other atoms.
iii. When a cosmic ray proton impacts atomic nuclei in the upper atmosphere, pions are created. These
decay within a relatively short distance (meters) into muons (their preferred decay product), and muon
neutrinos. The muons from these high energy cosmic rays generally continue in about the same direction
as the original proton, at a velocity near the speed of light.
When a cosmic ray proton impacts atomic nuclei in the upper
atmosphere, pions are created. These decay within a relatively
short distance (meters) into muons (their preferred decay product),
and muon neutrinos. The muons from these high energy cosmic
rays generally continue in about the same direction as the original
proton, at a velocity near the speed of light.
32. Bibliography
Introduction
3. Plateauing
a. reach a state of little or no change after a time of activity or progress
b. a period or state of little or no growth or decline
c. to calibrate/prepare the equipment so that you can conduct an experiment while ensure the validity of your
data
4. Cosmic Ray Muon Detector
a. http://quarknet.fnal.gov/toolkits/ati/crdetectors.html
b. https://www.sciencedaily.com/releases/2017/11/171120174502.htm
c. a tool used to detect/count muons in different environments/locations on earth
5. Voltage
a. https://www.explainthatstuff.com/electricity.html
b. The voltage is a kind of electrical force that makes electricity move through a wire and we measure it in volts.
The bigger the voltage, the more current will tend to flow. So a 12-volt car battery will generally produce
more current than a 1.5-volt flashlight battery.
33. Bibliography
Introduction
6. Signal rate
a. http://viewpure.com/SNR
b. a measure of signal strength relative to background noise
7. Noise
a. http://cosmic.lbl.gov/documentation/UsingtheDetector.pdf
b. unwanted sounds, interference to the signal you are trying to listen to/hear
8. Channel
a. https://en.wikipedia.org/wiki/Communication_channel
b. a physical transmission medium such as a wire, or to a logical connection over a multiplexed medium such
as a radio channel in telecommunications and computer networking
34. Bibliography
Procedure
9. Multimeter
a. https://www.sciencebuddies.org/science-fair-
projects/references/how-to-use-a-multimeter#qmultimeter
b. http://viewpure.com/MultiMeter
c. A multimeter is a handy tool that you use to measure electricity, just
like you would use a ruler to measure distance, a stopwatch to
measure time, or a scale to measure weight.
i. The neat thing about a multimeter is that unlike a ruler, watch,
or scale, it can measure different things — kind of like a multi-
tool
ii. There are many different multimeter models
10. Noise
a. http://cosmic.lbl.gov/documentation/UsingtheDetector.pdf
b. unwanted sounds, interference to the signal you are trying to listen
to/hear