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1. DIGITAL WDC EXCHANGE FORMAT FOR OBSERVATORY 1.0 MINUTE VALUES
DIGITAL WDC EXCHANGE FORMAT . FOR OBSERVATORY 1.0 MINUTE VALUES 1. ... DATA-1 .. DATA-60 are 1-minute values of the given element for that hour. ... Typically, digital 1-minute values received by WDCs from organizations operating automatic magnetic observatory instruments are averages of more frequendy sampled values, e.g. 10-second point samples. ... If the method used to obtain 1-minute average values is important to a user, the WDC will assist in determining the exact procedure applied. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/HTML/WDCFORM.HTM -- 6.6 Кб -- 03.07.2001
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2. The AstroStat Slog Blog Archive P Values: What They Are and How to Use Them
... Archives . ... ArXiv] 3rd week, Sept. 2007 . ... P Values: What They Are and How to Use Them by Luc Demortier emerged from my mind. ... Comment ( RSS ) | ... Algorithms arXiv Astro Bad AstroStat Bayesian CHASC Cross-Cultural Data Processing Fitting Frequentist Galaxies gamma-ray High-Energy Imaging Jargon Job Languages MC MCMC Meta Methods Misc News Nuggets Objects Optical Physics Quotes Spectral Stars Stat Timing Uncertainty X-ray . ... Chandra Blog . ... Entries (RSS) and Comments (RSS) . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2007/p-values-what-they-are-and-how-to-use-them/index.html -- 19.9 Кб -- 01.03.2014
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3. The Galaxy Gallery: Messier Objects
M1 image More About M1 Nice Color Picture . ... M16 image More About M16 HST image . ... M31 image More About M31 Nice Color Picture . ... M42 image ; M43 image More About M42/43 Nice Color CCD Picture . M51 image More About M51 Color Image of M51 M51 Supernova . M57 image More About M57 Nice Color CCD Picture Very Deep M57 Image . ... M81 image More About M81 M81 Supernova Ultraviolet Image of M81 More about Ultraviolet Imaging . M82 image More About M82 M82 False Color M82 True Color . ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/messier.html -- 7.0 Кб -- 23.07.2004
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4. Explanations for solar physics computing page
This document explains values, tables and other matters on solar physics computing pages. ... is040423.ete : SAHA-S tables, interpolation values: T, rho, X. Z is fixed at 0.02. See reference above. opal2005.etf : OPAL EOS, interpolation values: T, rho, X, Z. Downloaded from OPAL site , marked there as "2005", seems to be unpublished. opal2001.etf : OPAL EOS, interpolation values: T, rho, X, Z. Rogers F.J., Nayfonov A. Astrophys. ... The following values can be calculated: . ... dimensionless . ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/physics/phys-help.html -- 8.0 Кб -- 21.10.2009
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5. Value at histogram fraction
... Meta Index / Home Page / General-purpose array-processing utilities / Array or vector scalar . ... If is outside the range 0 to 1, the smallest or largest element , whichever is appropriate, is returned. interface valueAtHistoFraction real ( single ) function valueAtHistoFractionVector(vector, binFraction , maskVector) real ( single ), intent (in) :: vector(:), binFraction logical(bool), intent (in), optional :: maskVector(:) end function valueAtHistoFractionVector real ( single ) ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/ssclib/node18.html -- 4.6 Кб -- 01.07.2008
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6. Clumpy dust disks
... Abstract: We present Monte Carlo radiative transfer simulations for spiral galaxies modelled as a stellar disk and a two-phase clumpy dust distribution. ... As a general result, clumpy models are less opaque than the corresponding homogeneous models. ... 0.00 0.15 0.50 0.1 0.5 1.0 2.0 5.0 10.0 0.25 X . ... We have also produced several homogeneous models, to compare to the clumpy models. ... Homogeneous and clumpy models with the same tauV have the same dust mass. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~sbianchi/clumping.html -- 14.5 Кб -- 29.03.2002
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7. Symbol Substitution in Command Procedures
Next: DO Loops Up: MIDAS Command Language Previous: Passing Parameters in . As mentioned before, the Monitor performs symbol substitutions on MIDAS command lines in the first pass by replacing symbol names in the command line with their current value. For character symbols just the string is put in; for symbols of other types the binary data are converted to ASCII using the formats specified in the SET/FORMAT command. ... Example 6, MIDAS procedure exa6.prg . ... WRITE/KEYWORD VAR/R/1/1 0. ! ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol1/node40.html -- 12.2 Кб -- 23.02.1996
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8. Elements of Algebra
... These are just the bare bones--just three basic ideas and rules for handling relations ("equations") involving unknown quantities whose values you are trying to find. In most calculations you try to find a number . ... To get a solution, one must replace the given equation (or equations) with others, containing the same information but cleaner in appearance. ... If you have an equation and modify both its sides in exactly the same way, what you get is also a valid equation. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/mirrors/stern/stargaze/Ialgeb1.htm -- 8.4 Кб -- 03.12.2003
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/mirrors/stern/stargaze/Ialgeb1.htm -- 8.4 Кб -- 22.12.2007
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9. Calibration of the total infrared luminosity of nearby galaxies from Spitzer
When combined with infrared observations with the Spitzer telescope (3 to 160 ЮМm), the Herschel Space Observatory now fully samples the thermal dust emission up to 500 ЮМm and enables us to better estimate the total infrared-submm energy budget (LTIR) of nearby galaxies. We present new empirical calibrations to estimate resolved and integrated total infrared luminosities from Spitzer and Herschel bands used as monochromatic or combined tracers. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2013MNRAS.431.1956G.html -- 5.5 Кб -- 21.01.2016
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10. Elements of Nearby Spiral M33
... Elements of Nearby Spiral M33 . ... 27.09.2001 . ... Mayall Telescope , KPNO , NOAO , NSF Explanation: Spiral galaxy M33 is a mid-sized member of our Local Group of Galaxies . M33 is also called the Triangulum Galaxy for the constellation in which it resides. ... It was taken to help separate stars from emission nebulae, and therefore help study how galaxies form stars. ... September 2001 . ... Publications with keywords: M 33 - spiral galaxy . Publications with words: M 33 - spiral galaxy . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/apod/2001-09-27 -- 14.6 Кб -- 09.10.2004
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11. Values of asteroid masses
In the Table below the masses of some asteroids which were determined during the last years are listed. ... The listed values were determined from observations of many test bodies by the weighted least square fit for one perturbing mass and corrections to the orbit elements of all used test bodies. ... based on the observations of 98 asteroids (including 50278) with the values of standard error of mass determination less than 3.0 10 -11 M Sun . ... Mass . ... 3) Mass 121 : 0.74 x 10 -11 M Sun ; . ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/engmasses.htm -- 12.4 Кб -- 09.04.2016
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12. APOD: 2001 September 27 - Elements of Nearby Spiral M33
... 2001 September 27 . Elements of Nearby Spiral M33 . ... Explanation: Spiral galaxy M33 is a mid-sized member of our Local Group of Galaxies . ... M33 's proximity to M31 causes it to be thought by some to be a satellite galaxy of this more massive galaxy. M33 's proximity to our Milky Way Galaxy causes it to appear more than twice the angular size of the Full Moon , and be visible with a good pair of binoculars. ... About APOD | ...
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