- published: 26 May 2012
- views: 52652
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A description of how different chemicals can produce very specific emission lines or absorption lines in the spectrum of light from a distant object and how each chemical element has its own unique set of spectral lines. Part of an introductory series on astronomy.
Let us know what you think of these videos by filling out our short survey at http://tinyurl.com/astronomy-pulsar. Thank you!
086 - Emission and Absorption Spectra
In this video Paul Andersen explains how the photons emitted from or absorbed by an atom or nuclei is directly related to electrons moving between energy level. Absorption and emission are a direct result of the conservation of energy. Scientists may use the emission spectra of material to determine the atoms or molecules contained within the material.
Do you speak another language? Help me translate my videos:
http://www.bozemanscience.com/translations/
Music Attribution
Title: String Theory
Artist: Herman Jolly
http://sunsetvalley.bandcamp.com/track/string-theory
All of the images are licensed under creative commons and public domain licensing:
English: Colorful Spectrum simulationEspañol: Espectro de Colores de La Luz visibleEsperanto: Koloroj Videblaj中文（简体）: 软件模拟的可见光谱。中文（繁體）: 軟件模擬的可見光譜。, August 27, 2008. Digitally created by Deborah S Krolls, December 13, 2004. http://commons.wikimedia.org/wiki/File:Spectrum4websiteEval.png.
“Gas-Filled Tube.” Wikipedia, the Free Encyclopedia, January 31, 2015. http://en.wikipedia.org/w/index.php?title=Gas-filled_tube&oldid;=634245710.
Kuiper, Pieter. English: Fridge Letters in Natural Light, November 9, 2009. Own work. http://commons.wikimedia.org/wiki/File:Fluorescence_off.jpg.
———. English: Plastic Fridge Letters (from Different Manufacturers) When a Fluorescent Lamp (Labino) Is Switched on, November 9, 2009. Own work. http://commons.wikimedia.org/wiki/File:Fluorescence_on.jpg.
Kurzon. English: A Simple Illustration of Bohr’s Model of the Atom, with an Electron Making Quantum Leaps., April 14, 2014. Own work. http://commons.wikimedia.org/wiki/File:Bohr_atom_animation.gif.
- published: 06 Mar 2015
- views: 91280
This video shows the spectral lines of hydrogen atom, represented by the orbital diagram of an atom.
- published: 02 Jun 2015
- views: 13347
A look at spectral lines from different elements and molecules, and from a thermal emitter.
- published: 22 Jan 2009
- views: 62596
Why are fireworks coloured, how can we tell what elements are in stars just from the light we see? This video explains why physics is all about sunshine and rainbows.
If you would like to see more A Level Physics videos then please Subscribe to my channel to keep updated with new videos and to search the Playlists already created. You can also visit my site 'A Level Physics Online' to see how all the videos relate to your course and for even more resources at http://www.alevelphysicsonline.com/
Thanks for watching,
Mr Matheson
- published: 23 Feb 2015
- views: 22740
Electrons occupying the energy shells in an atom take the form of a cloud
surrounding the much smaller nucleus.
Since only two electrons can fit into each of the energy shells, it is interesting to
look at the characteristics of these different shells or energy states.
These states are defined first by a primary quantum number called “n” and also
by a secondary quantum number called “l”.
And for each state, the electron has a different energy, which results from the
shape of the electron cloud.
For n=1, called the ground state, the shape is a symmetric cloud…the same in all
directions.
For n=2, the shape can take on two forms depending on the value of “l”
…although both shapes have the same energy…
One shape is a double spherical cloud – one sphere inside the other.
While the other shape for n=2 is in the shape of a dumbell
Courtesy of the Cassiopeia project
- published: 03 Jan 2015
- views: 7052
Joseph Fraunhofer, (ennobled in 1824 as Ritter von Fraunhofer) was a German optician.
He is known for the discovery of the dark absorption lines known as Fraunhofer lines in the Sun's spectrum, and for making excellent optical glass and achromatic telescope objectives.
A spectral line is a dark or bright line in an otherwise uniform and continuous spectrum, resulting from a deficiency or excess of photons in a narrow frequency range, compared with the nearby frequencies. Spectral lines are often used as a sort of "atomic fingerprint," as gases emit light at very specific frequencies when exposed to electromagnetic waves, which are displayed in the form of spectral lines. These "fingerprints" can be compared to the previously collected fingerprints of elements, and are thus used to identify the molecular construct of stars and planets which would otherwise be impossible.
- published: 28 Apr 2013
- views: 2572
Video lecture discussion the different types of spectra possible in astronomy.
- published: 18 Feb 2013
- views: 23222
For more information:
http://www.7activestudio.com
info@7activestudio.com
http://www.7activemedical.com/
info@7activemedical.com
http://www.sciencetuts.com/
7activestudio@gmail.com
Contact: +91- 9700061777,
040-64501777 / 65864777
7 Active Technology Solutions Pvt.Ltd. is an educational 3D digital content provider for K-12. We also customise the content as per your requirement for companies platform providers colleges etc . 7 Active driving force "The Joy of Happy Learning" -- is what makes difference from other digital content providers. We consider Student needs, Lecturer needs and College needs in designing the 3D & 2D Animated Video Lectures. We are carrying a huge 3D Digital Library ready to use.
In physics, a continuous spectrum usually means a set of attainable values for some physical quantity (such as energy or wavelength) that is best described as an interval of real numbers. It is opposed to discrete spectrum, a set of attainable values that is discrete in the mathematical sense, where there is a positive gap between each value and the next one.
The classical example of a continuous spectrum, from which the name is derived, is the part of the spectrum of the light emitted by excited atoms of hydrogen that is due to free electrons becoming bound to a hydrogen ion and emitting photons, which are smoothly spread over a wide range of wavelengths; in contrast to the discrete lines due to electrons falling from some bound quantum state to a state of lower energy.
As in that classical example, the term is most often used when the range of values of a physical quantity may have both a continuous and a discrete part, whether at the same time or in different situations. In quantum systems, continuous spectra (as in bremsstrahlung and thermal radiation) are usually associated with free particles, such as atoms in a gas, electrons in an electron beam, or conduction band electrons in a metal. In particular, the position and momentum of a free particle have a continuous spectrum, but when the particle is confined to a limited space its spectrum becomes discrete.
Often a continuous spectrum may be just a convenient model for a discrete spectrum whose values are too close to be distinguished, as in the phonons in a crystal.
The continuous and discrete spectra of physical systems can be modeled in functional analysis as different parts in the decomposition of the spectrum of a linear operator acting on a function space, such as the Hamiltonian operator.
- published: 04 Apr 2016
- views: 2261
Spectral line
A spectral line is a dark or bright line in an otherwise uniform and continuous spectrum, resulting from emission or absorption of light in a narrow frequency range, compared with the nearby frequencies. Spectral lines are often used to identify atoms and molecules from their characteristic spectral lines. These "fingerprints" can be compared to the previously collected fingerprints of atoms and molecules, and are thus used to identify the atomic and molecular components of stars and planets which would otherwise be impossible.
Types of line spectra
Spectral lines are the result of interaction between a quantum system (usually atoms, but sometimes molecules or atomic nuclei) and a single photon. When a photon has about the right amount of energy to allow a change in the energy state of the system (in the case of an atom this is usually an electron changing orbitals), the photon is absorbed. Then it will be spontaneously re-emitted, either in the same frequency as the original or in a cascade, where the sum of the energies of the photons emitted will be equal to the energy of the one absorbed (assuming the system returns to its original state).
This page contains text from Wikipedia, the Free Encyclopedia -
https://wn.com/Spectral_line
This article is licensed under the Creative Commons Attribution-ShareAlike 3.0 Unported License, which means that you can copy and modify it as long as the entire work (including additions) remains under this license.
This article is licensed under the Creative Commons Attribution-ShareAlike 3.0 Unported License, which means that you can copy and modify it as long as the entire work (including additions) remains under this license.
A-level
The General Certificate of Education Advanced Level (short form: GCE Advanced Level), or more commonly, the A Level, is a school leaving qualification offered by educational bodies in the United Kingdom and the British Crown dependencies to students completing secondary or pre-university education. A number of countries, including Singapore, Kenya, Mauritius and Zimbabwe have developed qualifications with the same name as and a similar format to the British A Levels. Obtaining A Level or equivalent qualifications is generally required for university entrance.
A Levels are generally worked towards over two years and split into two parts, with one part studied in each year. The first part is known as the Advanced Subsidiary Level, A1 Level or AS Level (the AS Level acronym was previously used for the separate Advanced Supplementary Level qualification). The second part is known as the A2 Level and is more in depth and academically rigorous than the A1 Level. The AS Level is a qualification in its own right, and the AS Level combined with the A2 Level forms the complete A Level qualification. Up to June 2009 a third Special / Advanced Extension Award level was available for the brightest candidates.
This page contains text from Wikipedia, the Free Encyclopedia -
https://wn.com/A-level
This article is licensed under the Creative Commons Attribution-ShareAlike 3.0 Unported License, which means that you can copy and modify it as long as the entire work (including additions) remains under this license.
This article is licensed under the Creative Commons Attribution-ShareAlike 3.0 Unported License, which means that you can copy and modify it as long as the entire work (including additions) remains under this license.
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12:21Properties of Light: Spectral Lines 1
Properties of Light: Spectral Lines 1Properties of Light: Spectral Lines 1
A description of how different chemicals can produce very specific emission lines or absorption lines in the spectrum of light from a distant object and how each chemical element has its own unique set of spectral lines. Part of an introductory series on astronomy. Let us know what you think of these videos by filling out our short survey at http://tinyurl.com/astronomy-pulsar. Thank you! -
5:18Emission and Absorption Spectra
Emission and Absorption SpectraEmission and Absorption Spectra
086 - Emission and Absorption Spectra In this video Paul Andersen explains how the photons emitted from or absorbed by an atom or nuclei is directly related to electrons moving between energy level. Absorption and emission are a direct result of the conservation of energy. Scientists may use the emission spectra of material to determine the atoms or molecules contained within the material. Do you speak another language? Help me translate my videos: http://www.bozemanscience.com/translations/ Music Attribution Title: String Theory Artist: Herman Jolly http://sunsetvalley.bandcamp.com/track/string-theory All of the images are licensed under creative commons and public domain licensing: English: Colorful Spectrum simulationEspañol: Espectro de Colores de La Luz visibleEsperanto: Koloroj Videblaj中文（简体）: 软件模拟的可见光谱。中文（繁體）: 軟件模擬的可見光譜。, August 27, 2008. Digitally created by Deborah S Krolls, December 13, 2004. http://commons.wikimedia.org/wiki/File:Spectrum4websiteEval.png. “Gas-Filled Tube.” Wikipedia, the Free Encyclopedia, January 31, 2015. http://en.wikipedia.org/w/index.php?title=Gas-filled_tube&oldid;=634245710. Kuiper, Pieter. English: Fridge Letters in Natural Light, November 9, 2009. Own work. http://commons.wikimedia.org/wiki/File:Fluorescence_off.jpg. ———. English: Plastic Fridge Letters (from Different Manufacturers) When a Fluorescent Lamp (Labino) Is Switched on, November 9, 2009. Own work. http://commons.wikimedia.org/wiki/File:Fluorescence_on.jpg. Kurzon. English: A Simple Illustration of Bohr’s Model of the Atom, with an Electron Making Quantum Leaps., April 14, 2014. Own work. http://commons.wikimedia.org/wiki/File:Bohr_atom_animation.gif. -
3:49Spectral Lines
Spectral Lines -
2:14Spectral Lines of Hydrogen Atom
Spectral Lines of Hydrogen AtomSpectral Lines of Hydrogen Atom
This video shows the spectral lines of hydrogen atom, represented by the orbital diagram of an atom. -
1:50Spectral Lines Demo
Spectral Lines DemoSpectral Lines Demo
A look at spectral lines from different elements and molecules, and from a thermal emitter. -
5:12A Level Physics - Emission and Absorption Line Spectra
A Level Physics - Emission and Absorption Line SpectraA Level Physics - Emission and Absorption Line Spectra
Why are fireworks coloured, how can we tell what elements are in stars just from the light we see? This video explains why physics is all about sunshine and rainbows. If you would like to see more A Level Physics videos then please Subscribe to my channel to keep updated with new videos and to search the Playlists already created. You can also visit my site 'A Level Physics Online' to see how all the videos relate to your course and for even more resources at http://www.alevelphysicsonline.com/ Thanks for watching, Mr Matheson -
3:49Chemistry - Spectral Lines
Chemistry - Spectral LinesChemistry - Spectral Lines
Electrons occupying the energy shells in an atom take the form of a cloud surrounding the much smaller nucleus. Since only two electrons can fit into each of the energy shells, it is interesting to look at the characteristics of these different shells or energy states. These states are defined first by a primary quantum number called “n” and also by a secondary quantum number called “l”. And for each state, the electron has a different energy, which results from the shape of the electron cloud. For n=1, called the ground state, the shape is a symmetric cloud…the same in all directions. For n=2, the shape can take on two forms depending on the value of “l” …although both shapes have the same energy… One shape is a double spherical cloud – one sphere inside the other. While the other shape for n=2 is in the shape of a dumbell Courtesy of the Cassiopeia project -
14:35Spectral Lines ~ Joseph Fraunhofer
Spectral Lines ~ Joseph FraunhoferSpectral Lines ~ Joseph Fraunhofer
Joseph Fraunhofer, (ennobled in 1824 as Ritter von Fraunhofer) was a German optician. He is known for the discovery of the dark absorption lines known as Fraunhofer lines in the Sun's spectrum, and for making excellent optical glass and achromatic telescope objectives. A spectral line is a dark or bright line in an otherwise uniform and continuous spectrum, resulting from a deficiency or excess of photons in a narrow frequency range, compared with the nearby frequencies. Spectral lines are often used as a sort of "atomic fingerprint," as gases emit light at very specific frequencies when exposed to electromagnetic waves, which are displayed in the form of spectral lines. These "fingerprints" can be compared to the previously collected fingerprints of elements, and are thus used to identify the molecular construct of stars and planets which would otherwise be impossible. -
5:13Introductory Astronomy: Different Types of Spectra
Introductory Astronomy: Different Types of SpectraIntroductory Astronomy: Different Types of Spectra
Video lecture discussion the different types of spectra possible in astronomy. -
3:10CONTINUOUS SPECTRUM
CONTINUOUS SPECTRUMCONTINUOUS SPECTRUM
For more information: http://www.7activestudio.com info@7activestudio.com http://www.7activemedical.com/ info@7activemedical.com http://www.sciencetuts.com/ 7activestudio@gmail.com Contact: +91- 9700061777, 040-64501777 / 65864777 7 Active Technology Solutions Pvt.Ltd. is an educational 3D digital content provider for K-12. We also customise the content as per your requirement for companies platform providers colleges etc . 7 Active driving force "The Joy of Happy Learning" -- is what makes difference from other digital content providers. We consider Student needs, Lecturer needs and College needs in designing the 3D & 2D Animated Video Lectures. We are carrying a huge 3D Digital Library ready to use. In physics, a continuous spectrum usually means a set of attainable values for some physical quantity (such as energy or wavelength) that is best described as an interval of real numbers. It is opposed to discrete spectrum, a set of attainable values that is discrete in the mathematical sense, where there is a positive gap between each value and the next one. The classical example of a continuous spectrum, from which the name is derived, is the part of the spectrum of the light emitted by excited atoms of hydrogen that is due to free electrons becoming bound to a hydrogen ion and emitting photons, which are smoothly spread over a wide range of wavelengths; in contrast to the discrete lines due to electrons falling from some bound quantum state to a state of lower energy. As in that classical example, the term is most often used when the range of values of a physical quantity may have both a continuous and a discrete part, whether at the same time or in different situations. In quantum systems, continuous spectra (as in bremsstrahlung and thermal radiation) are usually associated with free particles, such as atoms in a gas, electrons in an electron beam, or conduction band electrons in a metal. In particular, the position and momentum of a free particle have a continuous spectrum, but when the particle is confined to a limited space its spectrum becomes discrete. Often a continuous spectrum may be just a convenient model for a discrete spectrum whose values are too close to be distinguished, as in the phonons in a crystal. The continuous and discrete spectra of physical systems can be modeled in functional analysis as different parts in the decomposition of the spectrum of a linear operator acting on a function space, such as the Hamiltonian operator.
-
Properties of Light: Spectral Lines 1
A description of how different chemicals can produce very specific emission lines or absorption lines in the spectrum of light from a distant object and how each chemical element has its own unique set of spectral lines. Part of an introductory series on astronomy. Let us know what you think of these videos by filling out our short survey at http://tinyurl.com/astronomy-pulsar. Thank you!
published: 26 May 2012 -
Emission and Absorption Spectra
086 - Emission and Absorption Spectra In this video Paul Andersen explains how the photons emitted from or absorbed by an atom or nuclei is directly related to electrons moving between energy level. Absorption and emission are a direct result of the conservation of energy. Scientists may use the emission spectra of material to determine the atoms or molecules contained within the material. Do you speak another language? Help me translate my videos: http://www.bozemanscience.com/translations/ Music Attribution Title: String Theory Artist: Herman Jolly http://sunsetvalley.bandcamp.com/track/string-theory All of the images are licensed under creative commons and public domain licensing: English: Colorful Spectrum simulationEspañol: Espectro de Colores de La Luz visibleEsperanto: Koloro...
published: 06 Mar 2015 -
-
Spectral Lines of Hydrogen Atom
This video shows the spectral lines of hydrogen atom, represented by the orbital diagram of an atom.
published: 02 Jun 2015 -
Spectral Lines Demo
A look at spectral lines from different elements and molecules, and from a thermal emitter.
published: 22 Jan 2009 -
A Level Physics - Emission and Absorption Line Spectra
Why are fireworks coloured, how can we tell what elements are in stars just from the light we see? This video explains why physics is all about sunshine and rainbows. If you would like to see more A Level Physics videos then please Subscribe to my channel to keep updated with new videos and to search the Playlists already created. You can also visit my site 'A Level Physics Online' to see how all the videos relate to your course and for even more resources at http://www.alevelphysicsonline.com/ Thanks for watching, Mr Matheson
published: 23 Feb 2015 -
Chemistry - Spectral Lines
Electrons occupying the energy shells in an atom take the form of a cloud surrounding the much smaller nucleus. Since only two electrons can fit into each of the energy shells, it is interesting to look at the characteristics of these different shells or energy states. These states are defined first by a primary quantum number called “n” and also by a secondary quantum number called “l”. And for each state, the electron has a different energy, which results from the shape of the electron cloud. For n=1, called the ground state, the shape is a symmetric cloud…the same in all directions. For n=2, the shape can take on two forms depending on the value of “l” …although both shapes have the same energy… One shape is a double spherical cloud – one sphere inside the other. While the other shape f...
published: 03 Jan 2015 -
Spectral Lines ~ Joseph Fraunhofer
Joseph Fraunhofer, (ennobled in 1824 as Ritter von Fraunhofer) was a German optician. He is known for the discovery of the dark absorption lines known as Fraunhofer lines in the Sun's spectrum, and for making excellent optical glass and achromatic telescope objectives. A spectral line is a dark or bright line in an otherwise uniform and continuous spectrum, resulting from a deficiency or excess of photons in a narrow frequency range, compared with the nearby frequencies. Spectral lines are often used as a sort of "atomic fingerprint," as gases emit light at very specific frequencies when exposed to electromagnetic waves, which are displayed in the form of spectral lines. These "fingerprints" can be compared to the previously collected fingerprints of elements, and are thus used to identif...
published: 28 Apr 2013 -
Introductory Astronomy: Different Types of Spectra
Video lecture discussion the different types of spectra possible in astronomy.
published: 18 Feb 2013 -
CONTINUOUS SPECTRUM
For more information: http://www.7activestudio.com info@7activestudio.com http://www.7activemedical.com/ info@7activemedical.com http://www.sciencetuts.com/ 7activestudio@gmail.com Contact: +91- 9700061777, 040-64501777 / 65864777 7 Active Technology Solutions Pvt.Ltd. is an educational 3D digital content provider for K-12. We also customise the content as per your requirement for companies platform providers colleges etc . 7 Active driving force "The Joy of Happy Learning" -- is what makes difference from other digital content providers. We consider Student needs, Lecturer needs and College needs in designing the 3D & 2D Animated Video Lectures. We are carrying a huge 3D Digital Library ready to use. In physics, a continuous spectrum usually mean...
published: 04 Apr 2016
Properties of Light: Spectral Lines 1
- Order: Reorder
- Duration: 12:21
- Updated: 26 May 2012
- views: 52652
A description of how different chemicals can produce very specific emission lines or absorption lines in the spectrum of light from a distant object and how eac...
A description of how different chemicals can produce very specific emission lines or absorption lines in the spectrum of light from a distant object and how each chemical element has its own unique set of spectral lines. Part of an introductory series on astronomy.
Let us know what you think of these videos by filling out our short survey at http://tinyurl.com/astronomy-pulsar. Thank you!
https://wn.com/Properties_Of_Light_Spectral_Lines_1
A description of how different chemicals can produce very specific emission lines or absorption lines in the spectrum of light from a distant object and how each chemical element has its own unique set of spectral lines. Part of an introductory series on astronomy.
Let us know what you think of these videos by filling out our short survey at http://tinyurl.com/astronomy-pulsar. Thank you!
- published: 26 May 2012
- views: 52652
Emission and Absorption Spectra
- Order: Reorder
- Duration: 5:18
- Updated: 06 Mar 2015
- views: 91280
086 - Emission and Absorption Spectra
In this video Paul Andersen explains how the photons emitted from or absorbed by an atom or nuclei is directly related to...
086 - Emission and Absorption Spectra
In this video Paul Andersen explains how the photons emitted from or absorbed by an atom or nuclei is directly related to electrons moving between energy level. Absorption and emission are a direct result of the conservation of energy. Scientists may use the emission spectra of material to determine the atoms or molecules contained within the material.
Do you speak another language? Help me translate my videos:
http://www.bozemanscience.com/translations/
Music Attribution
Title: String Theory
Artist: Herman Jolly
http://sunsetvalley.bandcamp.com/track/string-theory
All of the images are licensed under creative commons and public domain licensing:
English: Colorful Spectrum simulationEspañol: Espectro de Colores de La Luz visibleEsperanto: Koloroj Videblaj中文（简体）: 软件模拟的可见光谱。中文（繁體）: 軟件模擬的可見光譜。, August 27, 2008. Digitally created by Deborah S Krolls, December 13, 2004. http://commons.wikimedia.org/wiki/File:Spectrum4websiteEval.png.
“Gas-Filled Tube.” Wikipedia, the Free Encyclopedia, January 31, 2015. http://en.wikipedia.org/w/index.php?title=Gas-filled_tube&oldid;=634245710.
Kuiper, Pieter. English: Fridge Letters in Natural Light, November 9, 2009. Own work. http://commons.wikimedia.org/wiki/File:Fluorescence_off.jpg.
———. English: Plastic Fridge Letters (from Different Manufacturers) When a Fluorescent Lamp (Labino) Is Switched on, November 9, 2009. Own work. http://commons.wikimedia.org/wiki/File:Fluorescence_on.jpg.
Kurzon. English: A Simple Illustration of Bohr’s Model of the Atom, with an Electron Making Quantum Leaps., April 14, 2014. Own work. http://commons.wikimedia.org/wiki/File:Bohr_atom_animation.gif.
https://wn.com/Emission_And_Absorption_Spectra
086 - Emission and Absorption Spectra
In this video Paul Andersen explains how the photons emitted from or absorbed by an atom or nuclei is directly related to electrons moving between energy level. Absorption and emission are a direct result of the conservation of energy. Scientists may use the emission spectra of material to determine the atoms or molecules contained within the material.
Do you speak another language? Help me translate my videos:
http://www.bozemanscience.com/translations/
Music Attribution
Title: String Theory
Artist: Herman Jolly
http://sunsetvalley.bandcamp.com/track/string-theory
All of the images are licensed under creative commons and public domain licensing:
English: Colorful Spectrum simulationEspañol: Espectro de Colores de La Luz visibleEsperanto: Koloroj Videblaj中文（简体）: 软件模拟的可见光谱。中文（繁體）: 軟件模擬的可見光譜。, August 27, 2008. Digitally created by Deborah S Krolls, December 13, 2004. http://commons.wikimedia.org/wiki/File:Spectrum4websiteEval.png.
“Gas-Filled Tube.” Wikipedia, the Free Encyclopedia, January 31, 2015. http://en.wikipedia.org/w/index.php?title=Gas-filled_tube&oldid;=634245710.
Kuiper, Pieter. English: Fridge Letters in Natural Light, November 9, 2009. Own work. http://commons.wikimedia.org/wiki/File:Fluorescence_off.jpg.
———. English: Plastic Fridge Letters (from Different Manufacturers) When a Fluorescent Lamp (Labino) Is Switched on, November 9, 2009. Own work. http://commons.wikimedia.org/wiki/File:Fluorescence_on.jpg.
Kurzon. English: A Simple Illustration of Bohr’s Model of the Atom, with an Electron Making Quantum Leaps., April 14, 2014. Own work. http://commons.wikimedia.org/wiki/File:Bohr_atom_animation.gif.
- published: 06 Mar 2015
- views: 91280
Spectral Lines
- Order: Reorder
- Duration: 3:49
- Updated: 17 Sep 2008
- views: 53765
Spectral Lines of Hydrogen Atom
- Order: Reorder
- Duration: 2:14
- Updated: 02 Jun 2015
- views: 13347
This video shows the spectral lines of hydrogen atom, represented by the orbital diagram of an atom.
This video shows the spectral lines of hydrogen atom, represented by the orbital diagram of an atom.
https://wn.com/Spectral_Lines_Of_Hydrogen_Atom
This video shows the spectral lines of hydrogen atom, represented by the orbital diagram of an atom.
- published: 02 Jun 2015
- views: 13347
Spectral Lines Demo
- Order: Reorder
- Duration: 1:50
- Updated: 22 Jan 2009
- views: 62596
A look at spectral lines from different elements and molecules, and from a thermal emitter.
A look at spectral lines from different elements and molecules, and from a thermal emitter.
https://wn.com/Spectral_Lines_Demo
A look at spectral lines from different elements and molecules, and from a thermal emitter.
- published: 22 Jan 2009
- views: 62596
A Level Physics - Emission and Absorption Line Spectra
- Order: Reorder
- Duration: 5:12
- Updated: 23 Feb 2015
- views: 22740
Why are fireworks coloured, how can we tell what elements are in stars just from the light we see? This video explains why physics is all about sunshine and rai...
Why are fireworks coloured, how can we tell what elements are in stars just from the light we see? This video explains why physics is all about sunshine and rainbows.
If you would like to see more A Level Physics videos then please Subscribe to my channel to keep updated with new videos and to search the Playlists already created. You can also visit my site 'A Level Physics Online' to see how all the videos relate to your course and for even more resources at http://www.alevelphysicsonline.com/
Thanks for watching,
Mr Matheson
https://wn.com/A_Level_Physics_Emission_And_Absorption_Line_Spectra
Why are fireworks coloured, how can we tell what elements are in stars just from the light we see? This video explains why physics is all about sunshine and rainbows.
If you would like to see more A Level Physics videos then please Subscribe to my channel to keep updated with new videos and to search the Playlists already created. You can also visit my site 'A Level Physics Online' to see how all the videos relate to your course and for even more resources at http://www.alevelphysicsonline.com/
Thanks for watching,
Mr Matheson
- published: 23 Feb 2015
- views: 22740
Chemistry - Spectral Lines
- Order: Reorder
- Duration: 3:49
- Updated: 03 Jan 2015
- views: 7052
Electrons occupying the energy shells in an atom take the form of a cloud
surrounding the much smaller nucleus.
Since only two electrons can fit into each of th...
Electrons occupying the energy shells in an atom take the form of a cloud
surrounding the much smaller nucleus.
Since only two electrons can fit into each of the energy shells, it is interesting to
look at the characteristics of these different shells or energy states.
These states are defined first by a primary quantum number called “n” and also
by a secondary quantum number called “l”.
And for each state, the electron has a different energy, which results from the
shape of the electron cloud.
For n=1, called the ground state, the shape is a symmetric cloud…the same in all
directions.
For n=2, the shape can take on two forms depending on the value of “l”
…although both shapes have the same energy…
One shape is a double spherical cloud – one sphere inside the other.
While the other shape for n=2 is in the shape of a dumbell
Courtesy of the Cassiopeia project
https://wn.com/Chemistry_Spectral_Lines
Electrons occupying the energy shells in an atom take the form of a cloud
surrounding the much smaller nucleus.
Since only two electrons can fit into each of the energy shells, it is interesting to
look at the characteristics of these different shells or energy states.
These states are defined first by a primary quantum number called “n” and also
by a secondary quantum number called “l”.
And for each state, the electron has a different energy, which results from the
shape of the electron cloud.
For n=1, called the ground state, the shape is a symmetric cloud…the same in all
directions.
For n=2, the shape can take on two forms depending on the value of “l”
…although both shapes have the same energy…
One shape is a double spherical cloud – one sphere inside the other.
While the other shape for n=2 is in the shape of a dumbell
Courtesy of the Cassiopeia project
- published: 03 Jan 2015
- views: 7052
Spectral Lines ~ Joseph Fraunhofer
- Order: Reorder
- Duration: 14:35
- Updated: 28 Apr 2013
- views: 2572
Joseph Fraunhofer, (ennobled in 1824 as Ritter von Fraunhofer) was a German optician.
He is known for the discovery of the dark absorption lines known as Fraunh...
Joseph Fraunhofer, (ennobled in 1824 as Ritter von Fraunhofer) was a German optician.
He is known for the discovery of the dark absorption lines known as Fraunhofer lines in the Sun's spectrum, and for making excellent optical glass and achromatic telescope objectives.
A spectral line is a dark or bright line in an otherwise uniform and continuous spectrum, resulting from a deficiency or excess of photons in a narrow frequency range, compared with the nearby frequencies. Spectral lines are often used as a sort of "atomic fingerprint," as gases emit light at very specific frequencies when exposed to electromagnetic waves, which are displayed in the form of spectral lines. These "fingerprints" can be compared to the previously collected fingerprints of elements, and are thus used to identify the molecular construct of stars and planets which would otherwise be impossible.
https://wn.com/Spectral_Lines_~_Joseph_Fraunhofer
Joseph Fraunhofer, (ennobled in 1824 as Ritter von Fraunhofer) was a German optician.
He is known for the discovery of the dark absorption lines known as Fraunhofer lines in the Sun's spectrum, and for making excellent optical glass and achromatic telescope objectives.
A spectral line is a dark or bright line in an otherwise uniform and continuous spectrum, resulting from a deficiency or excess of photons in a narrow frequency range, compared with the nearby frequencies. Spectral lines are often used as a sort of "atomic fingerprint," as gases emit light at very specific frequencies when exposed to electromagnetic waves, which are displayed in the form of spectral lines. These "fingerprints" can be compared to the previously collected fingerprints of elements, and are thus used to identify the molecular construct of stars and planets which would otherwise be impossible.
- published: 28 Apr 2013
- views: 2572
Introductory Astronomy: Different Types of Spectra
- Order: Reorder
- Duration: 5:13
- Updated: 18 Feb 2013
- views: 23222
Video lecture discussion the different types of spectra possible in astronomy.
Video lecture discussion the different types of spectra possible in astronomy.
https://wn.com/Introductory_Astronomy_Different_Types_Of_Spectra
Video lecture discussion the different types of spectra possible in astronomy.
- published: 18 Feb 2013
- views: 23222
CONTINUOUS SPECTRUM
- Order: Reorder
- Duration: 3:10
- Updated: 04 Apr 2016
- views: 2261
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7 Active Technology Solutions Pvt.Ltd. is an educational 3D digital content provider for K-12. We also customise the content as per your requirement for companies platform providers colleges etc . 7 Active driving force "The Joy of Happy Learning" -- is what makes difference from other digital content providers. We consider Student needs, Lecturer needs and College needs in designing the 3D & 2D Animated Video Lectures. We are carrying a huge 3D Digital Library ready to use.
In physics, a continuous spectrum usually means a set of attainable values for some physical quantity (such as energy or wavelength) that is best described as an interval of real numbers. It is opposed to discrete spectrum, a set of attainable values that is discrete in the mathematical sense, where there is a positive gap between each value and the next one.
The classical example of a continuous spectrum, from which the name is derived, is the part of the spectrum of the light emitted by excited atoms of hydrogen that is due to free electrons becoming bound to a hydrogen ion and emitting photons, which are smoothly spread over a wide range of wavelengths; in contrast to the discrete lines due to electrons falling from some bound quantum state to a state of lower energy.
As in that classical example, the term is most often used when the range of values of a physical quantity may have both a continuous and a discrete part, whether at the same time or in different situations. In quantum systems, continuous spectra (as in bremsstrahlung and thermal radiation) are usually associated with free particles, such as atoms in a gas, electrons in an electron beam, or conduction band electrons in a metal. In particular, the position and momentum of a free particle have a continuous spectrum, but when the particle is confined to a limited space its spectrum becomes discrete.
Often a continuous spectrum may be just a convenient model for a discrete spectrum whose values are too close to be distinguished, as in the phonons in a crystal.
The continuous and discrete spectra of physical systems can be modeled in functional analysis as different parts in the decomposition of the spectrum of a linear operator acting on a function space, such as the Hamiltonian operator.
https://wn.com/Continuous_Spectrum
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http://www.7activestudio.com
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info@7activemedical.com
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7activestudio@gmail.com
Contact: +91- 9700061777,
040-64501777 / 65864777
7 Active Technology Solutions Pvt.Ltd. is an educational 3D digital content provider for K-12. We also customise the content as per your requirement for companies platform providers colleges etc . 7 Active driving force "The Joy of Happy Learning" -- is what makes difference from other digital content providers. We consider Student needs, Lecturer needs and College needs in designing the 3D & 2D Animated Video Lectures. We are carrying a huge 3D Digital Library ready to use.
In physics, a continuous spectrum usually means a set of attainable values for some physical quantity (such as energy or wavelength) that is best described as an interval of real numbers. It is opposed to discrete spectrum, a set of attainable values that is discrete in the mathematical sense, where there is a positive gap between each value and the next one.
The classical example of a continuous spectrum, from which the name is derived, is the part of the spectrum of the light emitted by excited atoms of hydrogen that is due to free electrons becoming bound to a hydrogen ion and emitting photons, which are smoothly spread over a wide range of wavelengths; in contrast to the discrete lines due to electrons falling from some bound quantum state to a state of lower energy.
As in that classical example, the term is most often used when the range of values of a physical quantity may have both a continuous and a discrete part, whether at the same time or in different situations. In quantum systems, continuous spectra (as in bremsstrahlung and thermal radiation) are usually associated with free particles, such as atoms in a gas, electrons in an electron beam, or conduction band electrons in a metal. In particular, the position and momentum of a free particle have a continuous spectrum, but when the particle is confined to a limited space its spectrum becomes discrete.
Often a continuous spectrum may be just a convenient model for a discrete spectrum whose values are too close to be distinguished, as in the phonons in a crystal.
The continuous and discrete spectra of physical systems can be modeled in functional analysis as different parts in the decomposition of the spectrum of a linear operator acting on a function space, such as the Hamiltonian operator.
- published: 04 Apr 2016
- views: 2261
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12:21
Properties of Light: Spectral Lines 1
A description of how different chemicals can produce very specific emission lines or absor...
published: 26 May 2012
Properties of Light: Spectral Lines 1
Properties of Light: Spectral Lines 1
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- published: 26 May 2012
- views: 52652
5:18
Emission and Absorption Spectra
086 - Emission and Absorption Spectra
In this video Paul Andersen explains how the photon...
published: 06 Mar 2015
Emission and Absorption Spectra
Emission and Absorption Spectra
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- published: 06 Mar 2015
- views: 91280
3:49
Spectral Lines
Find out what Spectral Lines are?
published: 17 Sep 2008
Spectral Lines
Spectral Lines
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- published: 17 Sep 2008
- views: 53765
2:14
Spectral Lines of Hydrogen Atom
This video shows the spectral lines of hydrogen atom, represented by the orbital diagram o...
published: 02 Jun 2015
Spectral Lines of Hydrogen Atom
Spectral Lines of Hydrogen Atom
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- published: 02 Jun 2015
- views: 13347
1:50
Spectral Lines Demo
A look at spectral lines from different elements and molecules, and from a thermal emitter...
published: 22 Jan 2009
Spectral Lines Demo
Spectral Lines Demo
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- published: 22 Jan 2009
- views: 62596
5:12
A Level Physics - Emission and Absorption Line Spectra
Why are fireworks coloured, how can we tell what elements are in stars just from the light...
published: 23 Feb 2015
A Level Physics - Emission and Absorption Line Spectra
A Level Physics - Emission and Absorption Line Spectra
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- published: 23 Feb 2015
- views: 22740
3:49
Chemistry - Spectral Lines
Electrons occupying the energy shells in an atom take the form of a cloud
surrounding the ...
published: 03 Jan 2015
Chemistry - Spectral Lines
Chemistry - Spectral Lines
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- published: 03 Jan 2015
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14:35
Spectral Lines ~ Joseph Fraunhofer
Joseph Fraunhofer, (ennobled in 1824 as Ritter von Fraunhofer) was a German optician.
He i...
published: 28 Apr 2013
Spectral Lines ~ Joseph Fraunhofer
Spectral Lines ~ Joseph Fraunhofer
- Report rights infringement
- published: 28 Apr 2013
- views: 2572
5:13
Introductory Astronomy: Different Types of Spectra
Video lecture discussion the different types of spectra possible in astronomy.
published: 18 Feb 2013
Introductory Astronomy: Different Types of Spectra
Introductory Astronomy: Different Types of Spectra
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- published: 18 Feb 2013
- views: 23222
3:10
CONTINUOUS SPECTRUM
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published: 04 Apr 2016
CONTINUOUS SPECTRUM
CONTINUOUS SPECTRUM
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Properties of Light: Spectral Lines 1...
Emission and Absorption Spectra...
Spectral Lines...
Spectral Lines of Hydrogen Atom...
Spectral Lines Demo...
A Level Physics - Emission and Absorption Line Spe...
Chemistry - Spectral Lines...
Spectral Lines ~ Joseph Fraunhofer...
Introductory Astronomy: Different Types of Spectra...
CONTINUOUS SPECTRUM...
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Edit The Guardian 01 Jun 2017
The annual gathering of government and industry elites will include a ‘progress report’ on the Trump administration. Will it get a passing grade?. Donald Trump. Bilderberg 2017. secret meeting of global leaders could prove a problem for Trump. The annual gathering of government and industry elites will include a ‘progress report’ on the Trump administration. Will it get a passing grade? ... Bilderberg ... Twitter ... “The Trump Administration ... ....
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Edit WorldNews.com 31 May 2017
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Edit Hindustan Times 01 Jun 2017
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China Completes World's Largest Floating Solar Power Plant
Edit WorldNews.com 01 Jun 2017
China is emerging as a world leader in sustainable energy with the completion of the world’s largest floating solar farm, IFL Science reports.Sungrow Power Supply announced this month that it has finished construction on a 40-megawatt solar power plant, which is sitting on an appropriate setting ... At full capacity, this will provide 2 gigawatts of power, enough to electrify 750,000 modern homes ... WN.com, Jim Berrie ....
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World War 3 Update: Japan Urges U.S. To ‘End Dialogue’ And Take Action Against North Korea
Edit Inquisitr 31 May 2017
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Viavi Solutions Introduces Scalable RF Monitoring for Heterogeneous Networks
Edit Market Watch 01 Jun 2017
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Global Hyperspectral Imaging Cameras Market Size 2017 Industry Trend and Forecast 2022
Edit Community news 01 Jun 2017
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Global Biochemical Analyzer Sales Market Research, Scope, Demand, Size and Forecast to 2022
Edit Community news 31 May 2017
Albany, New York, May 31, 2017. Market Research Hub's report split global into several key Regions, with sales (K Units), revenue (Million USD), market share and growth rate of Biochemical Analyzer for these regions, from 2012 to 2022 (forecast), covering. United States. China. Europe. Japan. Southeast Asia. India ... Beckmancoulter. Hitachi. Roche-diagnostics. Toshiba. Dirui. Mindray. KHB ... Grating Spectral ... Hospital ... 1.2.4 Grating Spectral ... ... Tel ... ....
The best TVs 2017: which TV should you buy?
Edit TechRadar 31 May 2017
We loved the consistency of its images, the eye-popping vibrancy of its wide color gamut panel and its easy-to-watch HDR – you get spectral highlights without accompanying eye fatigue. ... The bottom line, though, the JS8500's superb color, awesome 4K detail and sublime depth make this one special TV and remains a good value way to sample Samsung's impressive SUHD TVs even now, two years later....
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Edit Market Watch 30 May 2017
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Edit Wireless Week 30 May 2017
AT&T is gearing up for the latest round of fixed 5G tests, this time aiming for real-world trials in three states ... “These technologies are expected to result in higher spectral efficiencies, reduce latency to 1-5 milliseconds, and enable gigabit per second (Gbps) mobile and fixed broadband services, significantly faster than today’s average 4G speeds using LTE,” the carrier wrote in its application ... ....
Global Semiconductor Photolithography Market Projected to be Worth USD 8.19 Billion by 2021: Technavio
Edit Market Watch 30 May 2017
LONDON, May 30, 2017 (BUSINESS WIRE) -- According to the latest market study released by Technavio, the global semiconductor photolithography equipment marketis projected to grow to USD 8.19 billion by 2021, at a CAGR of more than 9% over the forecast period ... Mercury lamp ... From the early 1960s through the mid-1980s, mercury lamps dominated the photolithography market and were used for their spectral lines at 436 nm, 405 nm, and 365 nm....
Anesthesia Monitoring Devices Market Research, Growth Opportunities, Analysis and Forecasts Report 2016
Edit Community news 30 May 2017
Anesthesia in basic term is insensitivity to pain. It is used to induce unconsciousness during a surgery. The anesthesia monitoring devices, are used to check a patient’s response toward anesthesia during a surgical process ... Anesthesia can be monitored with different methods, such as EEG Monitors, ECG, bi-spectral index (BIS) obtained from EEG, oxygen and carbon dioxide analyzers, and temperature monitors ... Competitive insights ... About Us....
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