Waves in Motion
... where p is momentum in kg*m/s, h is Planck’s constant = 6.63 x 10-34 J, and λ is the wavelength in meters ...
... where p is momentum in kg*m/s, h is Planck’s constant = 6.63 x 10-34 J, and λ is the wavelength in meters ...
Physics 30 Lesson 24 Electromagnetic Waves
... deceleration of very high energy particles from accelerators bombardment of Earth's atmosphere by very high energy particles from outer space ...
... deceleration of very high energy particles from accelerators bombardment of Earth's atmosphere by very high energy particles from outer space ...
Lecture1(SynchrotronRadiationI) - Indico
... Layout of a synchrotron radiation source (I) Electrons are generated and accelerated in a linac, further accelerated to the required energy in a booster and injected and stored in the storage ring The circulating electrons emit an intense beam of synchrotron radiation which is sent down the beamlin ...
... Layout of a synchrotron radiation source (I) Electrons are generated and accelerated in a linac, further accelerated to the required energy in a booster and injected and stored in the storage ring The circulating electrons emit an intense beam of synchrotron radiation which is sent down the beamlin ...
CHAPTER 2 STRUCTURE OF ATOM • Atom is the smallest
... Properties of electromagnetic radiations: a. Oscillating electric and magnetic field are produced by oscillating charged particles. These fields are perpendicular to each other and both areperpendicular to the direction of propagation of the wave. b. They do not need a medium to travel. That means t ...
... Properties of electromagnetic radiations: a. Oscillating electric and magnetic field are produced by oscillating charged particles. These fields are perpendicular to each other and both areperpendicular to the direction of propagation of the wave. b. They do not need a medium to travel. That means t ...
Physics 30 - Structured Independent Learning
... at a meeting of the Royal Society of London. Unfortunately, Wheatstone had a bad case of stage fright and took off just before his lecture was to begin. As a result, Faraday was forced to give an unprepared lecture to the Royal Society of London. Faraday always gave well-prepared lectures punctuated ...
... at a meeting of the Royal Society of London. Unfortunately, Wheatstone had a bad case of stage fright and took off just before his lecture was to begin. As a result, Faraday was forced to give an unprepared lecture to the Royal Society of London. Faraday always gave well-prepared lectures punctuated ...
Dalton`s Atomic Theory Discovery of Electron Properties of Cathode
... Sir William Crooks (1895 performed experiments by passing electric current through gas in the discharge tube at very low pressure. He observed that at 10-4 (-4 is power to 10) atmosphere pressure, shining rays are emitted from cathode. These rays were named cathode rays. Cathode rays are material pa ...
... Sir William Crooks (1895 performed experiments by passing electric current through gas in the discharge tube at very low pressure. He observed that at 10-4 (-4 is power to 10) atmosphere pressure, shining rays are emitted from cathode. These rays were named cathode rays. Cathode rays are material pa ...
3. The Experimental Basis of Quantum Theory
... nucleus absorbs very little energy, and it can be ignored. The final energy of the electron is determined from the conservation of energy to be: ...
... nucleus absorbs very little energy, and it can be ignored. The final energy of the electron is determined from the conservation of energy to be: ...
PHY 108 – Atoms to Galaxies
... discovered that Io didn't always appear where it was supposed to be. c = 300 000 km/s 1888, H. Hertz generated EM waves in his lab. ...
... discovered that Io didn't always appear where it was supposed to be. c = 300 000 km/s 1888, H. Hertz generated EM waves in his lab. ...
t 1/2
... plates connected to a battery provide the electric field. Two current-carrying coils (not shown) produce a magnetic field perpendicular to the electric field. The sizes of the deflections, as noted on the fluorescent screen, can be used to determine the charge-to-mass ratio of the electron. Fig. 13- ...
... plates connected to a battery provide the electric field. Two current-carrying coils (not shown) produce a magnetic field perpendicular to the electric field. The sizes of the deflections, as noted on the fluorescent screen, can be used to determine the charge-to-mass ratio of the electron. Fig. 13- ...
Semiconductor detectors
... ionising particle is easily detected • poor performance because: - small contact potential (~1 V): slow-moving charges can be trapped, resulting in incomplete charge collection - depletion layer is thin: - high capacitance ! large electronic noise - small sensitive volume cannot detect high-energy r ...
... ionising particle is easily detected • poor performance because: - small contact potential (~1 V): slow-moving charges can be trapped, resulting in incomplete charge collection - depletion layer is thin: - high capacitance ! large electronic noise - small sensitive volume cannot detect high-energy r ...
Lecture 11 February 4, 2002 Chapter 3 The Particlelike Properties of
... course, is not known in the 19th century. The emitted energetic electrons will then collide with atoms in the tube and excite the atoms into high energy levels causing subsequent emission of electromagnetic radiation. When the tube is filled with a certain gas, such as H2 or He, sustained glow with ...
... course, is not known in the 19th century. The emitted energetic electrons will then collide with atoms in the tube and excite the atoms into high energy levels causing subsequent emission of electromagnetic radiation. When the tube is filled with a certain gas, such as H2 or He, sustained glow with ...
Basic concepts in electron and photon beams
... i is the numerical aperture of focusing system Reducing pinhole size until dss ~ l/2 since di ~ l /(2i) reaches diffraction limit. A even smaller pinhole does not reduce the image size but only hurts the photon flux Diffraction limited source does not require a pinhole and provide the most cohere ...
... i is the numerical aperture of focusing system Reducing pinhole size until dss ~ l/2 since di ~ l /(2i) reaches diffraction limit. A even smaller pinhole does not reduce the image size but only hurts the photon flux Diffraction limited source does not require a pinhole and provide the most cohere ...
Radiation
In physics, radiation is the emission or transmission of energy in the form of waves or particles through space or through a material medium. This includes: electro-magnetic radiation (also known as ""continuum radiation"") γ such as radio waves, visible light, and x-rays particle radiation such as α, β, and neutron radiation (discrete energy per particle) acoustic radiation such as ultrasound, sound, and seismic waves. (dependent on intervening mass for transmission)Radiation is often categorized as either ionizing or non-ionizing depending on the energy of the radiated particles. Ionizing radiation carries more than 10 eV, which is enough to ionize atoms and molecules, and break chemical bonds. This is an important distinction due to the large difference in harmfulness to living organisms. A common source of ionizing radiation is radioactive materials that emit α, β, or γ radiation, consisting of helium nuclei, electrons or positrons, and photons, respectively. Other sources include X-rays from medical radiography examinations and muons, mesons, positrons, neutrons and other particles that constitute the secondary cosmic rays that are produced after primary cosmic rays interact with Earth's atmosphere.Gamma rays, X-rays and the higher energy range of ultraviolet light constitute the ionizing part of the electromagnetic spectrum. The lower-energy, longer-wavelength part of the spectrum including visible light, infrared light, microwaves, and radio waves is non-ionizing; its main effect when interacting with tissue is heating. This type of radiation only damages cells if the intensity is high enough to cause excessive heating. Ultraviolet radiation has some features of both ionizing and non-ionizing radiation. While the part of the ultraviolet spectrum that penetrates the Earth's atmosphere is non-ionizing, this radiation does far more damage to many molecules in biological systems than can be accounted for by heating effects, sunburn being a well-known example. These properties derive from ultraviolet's power to alter chemical bonds, even without having quite enough energy to ionize atoms.The word radiation arises from the phenomenon of waves radiating (i.e., traveling outward in all directions) from a source. This aspect leads to a system of measurements and physical units that are applicable to all types of radiation. Because such radiation expands as it passes through space, and as its energy is conserved (in vacuum), the intensity of all types of radiation from a point source follows an inverse-square law in relation to the distance from its source. This law does not apply close to an extended source of radiation or for focused beams.