Temperature (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "Temperature" in English language version.

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aip.org (Global: 2,204th place; English: 1,735th place)

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  • Peak temperature for a bulk quantity of matter was achieved by a pulsed-power machine used in fusion physics experiments. The term bulk quantity draws a distinction from collisions in particle accelerators wherein high temperature applies only to the debris from two subatomic particles or nuclei at any given instant. The >2 GK temperature was achieved over a period of about ten nanoseconds during shot Z1137. In fact, the iron and manganese ions in the plasma averaged 3.58±0.41 GK (309±35 keV) for 3 ns (ns 112 through 115). Ion Viscous Heating in a Magnetohydrodynamically Unstable Z Pinch at Over 2×109 Kelvin, M.G. Haines et al., Physical Review Letters 96 (2006) 075003. Link to Sandia's news release. Archived 2010-05-30 at the Wayback Machine

journals.aps.org

  • Germer, L.H. (1925). 'The distribution of initial velocities among thermionic electrons', Phys. Rev., 25: 795–807. here

archive.org (Global: 6th place; English: 6th place)

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  • Bryan, G.H. (1907). Thermodynamics. An Introductory Treatise dealing mainly with First Principles and their Direct Applications, B.G. Teubner, Leipzig, p. 3. "Thermodynamics by George Hartley Bryan". Archived from the original on 2011-11-18. Retrieved 2011-10-02.
  • Bryan, G.H. (1907). Thermodynamics. An Introductory Treatise dealing mainly with First Principles and their Direct Applications, B.G. Teubner, Leipzig, p. 5: "... when a body is spoken of as growing hotter or colder an increase of temperature is always implied, for the hotness and coldness of a body are qualitative terms which can only refer to temperature." "Thermodynamics by George Hartley Bryan". Archived from the original on 2011-11-18. Retrieved 2011-10-02.

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  • Core temperature of a high–mass (>8–11 solar masses) star after it leaves the main sequence on the Hertzsprung–Russell diagram and begins the alpha process (which lasts one day) of fusing silicon–28 into heavier elements in the following steps: sulfur–32 → argon–36 → calcium–40 → titanium–44 → chromium–48 → iron–52 → nickel–56. Within minutes of finishing the sequence, the star explodes as a Type II supernova. Citation: Holland, Arthur; Williams, Mark. "Stellar Evolution: The Life and Death of Our Luminous Neighbors". GS265. University of Michigan. Archived from the original on 2009-01-16. More informative links can be found here "Chapter 21 Stellar Explosions". Archived from the original on 2013-04-11. Retrieved 2016-02-08., and here "Trans". Archived from the original on 2011-08-14. Retrieved 2016-02-08., and a concise treatise on stars by NASA is here "NASA - Star". Archived from the original on 2010-10-24. Retrieved 2010-10-12..

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  • Turvey, K. (1990). 'Test of validity of Maxwellian statistics for electrons thermionically emitted from an oxide cathode', European Journal of Physics, 11(1): 51–59. here

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  • Core temperature of a high–mass (>8–11 solar masses) star after it leaves the main sequence on the Hertzsprung–Russell diagram and begins the alpha process (which lasts one day) of fusing silicon–28 into heavier elements in the following steps: sulfur–32 → argon–36 → calcium–40 → titanium–44 → chromium–48 → iron–52 → nickel–56. Within minutes of finishing the sequence, the star explodes as a Type II supernova. Citation: Holland, Arthur; Williams, Mark. "Stellar Evolution: The Life and Death of Our Luminous Neighbors". GS265. University of Michigan. Archived from the original on 2009-01-16. More informative links can be found here "Chapter 21 Stellar Explosions". Archived from the original on 2013-04-11. Retrieved 2016-02-08., and here "Trans". Archived from the original on 2011-08-14. Retrieved 2016-02-08., and a concise treatise on stars by NASA is here "NASA - Star". Archived from the original on 2010-10-24. Retrieved 2010-10-12..

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  • The 350 MK value is the maximum peak fusion fuel temperature in a thermonuclear weapon of the Teller–Ulam configuration (commonly known as a hydrogen bomb). Peak temperatures in Gadget-style fission bomb cores (commonly known as an atomic bomb) are in the range of 50 to 100 MK. Citation: Nuclear Weapons Frequently Asked Questions, 3.2.5 Matter At High Temperatures. Link to relevant Web page. Archived 2007-05-03 at the Wayback Machine All referenced data was compiled from publicly available sources.

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  • Core temperature of a high–mass (>8–11 solar masses) star after it leaves the main sequence on the Hertzsprung–Russell diagram and begins the alpha process (which lasts one day) of fusing silicon–28 into heavier elements in the following steps: sulfur–32 → argon–36 → calcium–40 → titanium–44 → chromium–48 → iron–52 → nickel–56. Within minutes of finishing the sequence, the star explodes as a Type II supernova. Citation: Holland, Arthur; Williams, Mark. "Stellar Evolution: The Life and Death of Our Luminous Neighbors". GS265. University of Michigan. Archived from the original on 2009-01-16. More informative links can be found here "Chapter 21 Stellar Explosions". Archived from the original on 2013-04-11. Retrieved 2016-02-08., and here "Trans". Archived from the original on 2011-08-14. Retrieved 2016-02-08., and a concise treatise on stars by NASA is here "NASA - Star". Archived from the original on 2010-10-24. Retrieved 2010-10-12..

sandia.gov (Global: low place; English: low place)

  • Peak temperature for a bulk quantity of matter was achieved by a pulsed-power machine used in fusion physics experiments. The term bulk quantity draws a distinction from collisions in particle accelerators wherein high temperature applies only to the debris from two subatomic particles or nuclei at any given instant. The >2 GK temperature was achieved over a period of about ten nanoseconds during shot Z1137. In fact, the iron and manganese ions in the plasma averaged 3.58±0.41 GK (309±35 keV) for 3 ns (ns 112 through 115). Ion Viscous Heating in a Magnetohydrodynamically Unstable Z Pinch at Over 2×109 Kelvin, M.G. Haines et al., Physical Review Letters 96 (2006) 075003. Link to Sandia's news release. Archived 2010-05-30 at the Wayback Machine

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  • Core temperature of a high–mass (>8–11 solar masses) star after it leaves the main sequence on the Hertzsprung–Russell diagram and begins the alpha process (which lasts one day) of fusing silicon–28 into heavier elements in the following steps: sulfur–32 → argon–36 → calcium–40 → titanium–44 → chromium–48 → iron–52 → nickel–56. Within minutes of finishing the sequence, the star explodes as a Type II supernova. Citation: Holland, Arthur; Williams, Mark. "Stellar Evolution: The Life and Death of Our Luminous Neighbors". GS265. University of Michigan. Archived from the original on 2009-01-16. More informative links can be found here "Chapter 21 Stellar Explosions". Archived from the original on 2013-04-11. Retrieved 2016-02-08., and here "Trans". Archived from the original on 2011-08-14. Retrieved 2016-02-08., and a concise treatise on stars by NASA is here "NASA - Star". Archived from the original on 2010-10-24. Retrieved 2010-10-12..

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  • Measurement was made in 2002 and has an uncertainty of ±3 kelvins. A 1989 measurement Archived 2010-02-11 at the Wayback Machine produced a value of 5,777.0±2.5 K. Citation: Overview of the Sun (Chapter 1 lecture notes on Solar Physics by Division of Theoretical Physics, Dept. of Physical Sciences, University of Helsinki).

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