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Pressure at the core
"I.N. Galidakis" wrote in message news:1224602447.956577@athprx04... OG wrote: "I.N. Galidakis" wrote in message news:1224581136.871203@athprx04... Mike Dworetsky wrote: "I.N. Galidakis" wrote in message news:1224527030.287674@athprx03... OG wrote: [snip] Page updated to include Mass distribution, Luminosity and Pressure, Units for density updated to SI units. http://www.astd60.dsl.pipex.com:80/structure_of_sun.htm Sorry for nitpicking, but is your "Log(P)" meant to be base 10? We (the abominable mathematicians) usually denote by "Log(x)" the natural logarithm (base e). If I use log base 10 for P as per the page, the polytrope n=3 model seems to agree with the data fairly well. If I use the natural log, the results are awry. -- I.N. Galidakis Unless otherwise specified, in astrophysics log means base 10, and ln means base e. The Sun's basic structure isn't all that different (in order of magnitude terms) from an n=3 polytrope, as I recall from dim and distant stellar structure courses. It looks like even the magnitudes can be adjusted to a pretty good match. I was able to extract some results which agree fairly well with the data in the links OG and Sam provided. For those interested: http://ioannis.virtualcomposer2000.c...Polytrope.html Many thanks to all who replied. -- Can I nitpick in return and point out the lack of units in your discussion :-) Hehe! Added now. Well done otherwise. Thanks. Did you look at the detailed working in the QUB notes ? http://star.pst.qub.ac.uk/~sjs/teach...ecture%208.pdf No, but now that I looked, I see that my assumption to normalize the radius with respect to the point xi where the density falls to 0, was on the reasonable side. I better collect all those links and add them as refs at the end of the article. I think it would look better that way. I assume that since you changed the contents of ref [6], this web resource is yours, but I cannot find any other data except "Owen's Spare Webpages". If you'd like me to put something more meaningful there (for ref [6]), please tell me so. No need, I just use my webspace as a place where I can upload informal collections of 'stuff'. Feel free to take the data and make it your own - though I'm sure the Athlone Press would appreciate it if the acknowledgement stayed :-). What I have just noticed is the link on page 13 of the QUB document (your ref #5) that takes you to this collection of 16 standard models dating between 1982 and 2005 http://www.sns.ias.edu/~jnb/SNdata/solarmodels.html One day astrophysicists will use SI units too! |
#12
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Pressure at the core
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In article 1224507902.533497@athprx04, "I.N. Galidakis" writes: http://en.wikipedia.org/wiki/Polytrope Wiki does not mention what the constants are in its expression for K. Article edited. There's some useful information about solutions at http://www.scientificarts.com/laneemden/laneemden.html Searching on "Lane Emden" equation (i.e., three words, the first two in quotes) produced lots of hits, but I didn't examine them. -- Steve Willner Phone 617-495-7123 Cambridge, MA 02138 USA (Please email your reply if you want to be sure I see it; include a valid Reply-To address to receive an acknowledgement. Commercial email may be sent to your ISP.) |
#13
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Pressure at the core
In article ,
"Mike Dworetsky" wrote: snip Unless otherwise specified, in astrophysics log means base 10, and ln means base e. Not just in astrophysics IME; it seems to be the general convention in North American science and math textbooks -- up to the undergraduate level at least -- for "log" to mean the common logarithm and "ln" the natural. There's also "lg" for the base-2 logarithm (octaves), less often seen than the other two. -- Odysseus |
#14
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Pressure at the core
"Odysseus" wrote in message news In article , "Mike Dworetsky" wrote: snip No he didn't. You wrote snip. What's up, afraid to present his argument, chicken ****? |
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