... 22.Reference Frames . ... To derive the motion of a penny dropped inside an airliner moving at 600 miles/hr (about 1000 km/hr)--should we calculate it with respect to the interior of the airliner, or with respect to the ground? ... And if a similar penny is let go inside an orbiting spaceship--should its motion be calculated relative to the interior of the spaceship, or relative to the Earth outside? ... How do observations differ in the two frames--the airliner cabin and the Earth? ...

... casa . casa::AxesMapping . ... Info about mapping array axes to another order. ... AxesMapping (const IPosition &oldToNew) . Construct it with the mapping from old to new axes order. ... Get the mapping of old->new. const IPosition & . ... A value of -1 means that the old axes is ignored in the new one. ... It determines if axes are removed and/or reordered. casa::AxesMapping::AxesMapping . ... const IPosition & casa::AxesMapping::getToNew . ... const IPosition & casa::AxesMapping::getToOld . ...

... To derive the motion of a penny dropped inside an airliner moving at 600 miles/hr (about 1000 km/hr)--should we calculate it with respect to the interior of the airliner, or with respect to the ground? ... And if a similar penny is let go inside an orbiting spaceship--should its motion be calculated relative to the interior of the spaceship, or relative to the Earth outside? ... Each such choice is known as a frame of reference . Some possible frames are -- the interior of the airliner, . ...

... dust_AbsXSec . Absorption Cross section. typedef void . ... Calculates the equilibrium temperature given the absorption cross section and a radiation field. double . ... Calculates the absortion cross section of a species/size of dust grain . ... The grain absorption cross section . ... The absorption cross section of the grain . ... Calculates the equilibrium emission at wavelength lambda from a (large) grain at temperature T and with absorption cross section xsection. double dust_EquiT . ...

Stellarium 0.12.3 . ... Classes . ... SpaceShipObserver Class Reference . An observer which moves from from one position to another one and/or from one planet to another one. ... SpaceShipObserver (const StelLocation &startLoc, const StelLocation &target, double transitSeconds=1.f) . ... Get whether the life of this observer is over, and therefore that it should be changed to the next one provided by the getNextObserver() method. ... Get the next observer to use once the life of this one is over. ...

... The derivation of the reference multiplet is carried out in one of two basic styles: an `internal' style in which a kind of average multiplet is calculated from the values in the image themselves, without reference to any other information, or a `black body' (bb) style in which the reference multiplet is calculated using the widths of the energy bands (in the case of EPIC images) or the filter bandpasses (in the case of the OM). ...

... Reference Data for Calibration and Tools . ... Reference Files . ... Reference files used by the WFC3 calibration pipeline ( calwf3 and PyDrizzle/MultiDrizzle ) are updated on a regular basis. ... If you would like to receive an e-mail every time a new WFC3 reference file is delivered and the database is updated, you can subscribe to the wfc3_reffiles_upd mailing list. ... Linearity Correction Files . ... Detector-to-Image Correction File . ... Non-polynomial Filter Dependent Distortion File . ...

The ntpq and xntpdc utility programs can be used to debug reference clocks, either on the server itself or from another machine elsewhere in the network. The server is compiled, installed and started using the command-line switches described in the xntpd page. ... First, use the pe and as commands to display billboards showing the peer configuration and association IDs for all peers, including the radio clock peers. ... The most useful are the clockstat and commands described in the document page. ...

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Namespaces . ... coordConvWithFP . ... tcc.axis.coordConvWithFP Namespace Reference . ... Convert a coord from one coordinate system to another. ... from coordinate system; a coordConv.CoordSys if one matches, else an object containing getName() and getDate() (for gimage and gprobe coordinates the date is the guide probe number) . ... Definition at line 22 of file coordConvWithFP.py . list tcc.axis.coordConvWithFP.__all__ = ["coordConvWithFP"] . ...

... Available at http://www.hike.te.chiba-u.ac.jp/ikeda/CIE/publ/abst/15-2-86.html . ... Available at http://www.w3.org/TR/REC-CSS1-961217.html. ... HTML 4.0 Specification", D. Raggett, A. Le Hors, I. Jacobs, 8 July 1997. ... Available at ftp://ftp.internic.net/rfc/rfc1700.txt. ... Available at ftp://ds.internic.net/rfc/rfc1808.txt . ... Available at ftp://ds.internic.net/rfc/rfc2070.txt . ... Available at ftp://ds.internic.net/rfc/rfc2119.txt . ... Available at ftp://ds.internic.net/rfc/rfc2318.txt . ...

exp. energy levels: Martin,W.C., Sugar,J., Musgrove,A., Dalton, G.R., 2000, NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61. %exp. energy levels (1s2p 3P): Curdt, W., Landi, E., Wilhelm, K., Feldman, U., 2000, Phys.Rev.A, in press %Comment: the 1s2p 3P energies are calculated using the 1s2s 3S level as reference. ... Comment: 1s2p 3P1 energy has been calculated from the 1s2s 3P0 level using the NIST level separation. Thu Jul 20 13:42:29 2000 ...

... VIII/16 Molonglo Reference Catalogue of Radio Sources (Large+ 1991) ================================================================================ Molonglo Reference Catalogue of Radio Sources Large M.I., Cram L.E., and Brugess A.M. <The Observatory, 111, 72 (1991)> = 1991Obs.. ... The MRC was re-issued in 1990 with the original B1950 coordinates supplemented by J2000 values, and an additional cross-reference flag `J' added to denote (extended) sources imaged at 843-MHz by P.A. Jones. ...

... Web Links . ... Link . ... Python . http://www.python.org/doc . ... http://docs.python.org/tut/tut.html . ... an excellent tutorial for data analysis with Python (focus on astronomy) . ... an excellent cookbook (lots of examples) for scientific Python . ... an excellent set of example function available with numerical Python . http://www.python.org/ . ... introduction to datatables (java library used for smart HTML tables used on AB monitor) . ... homepage of the American Society for Quality . ...

... We have calculated the binary coalescence rate with time using the ``Scenario Machine'' code, which allows us to simulate evolution of large ensembles of binary stars in an artificial galaxy using a Monte Carlo method (see Lipunov 1992, Lipunov et al 1994, 1995 and references therein). ... The source evolution in a galaxy with given star formation rate is thus calculated as , where is the redshift at the turn-on of star formation, which is the second important parameter of the model. ...

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

... A Front of line M-G Goto a line ^E End of line ^N Next line M-N Front of paragraph ^P Previous line M-P End of paragraph ----------------------------------------------------------------------------- = (2) DELETING INSERTING -- Delete previous character ^D or DELETE Delete next character ^C or INSERT Insert a space M- -- Delete previous word M-D Delete next word ^K Close ( ... The KILL BUFFER is the text which has been most recently saved or deleted. ...

... Previous: Background Fluctuation Analysis from the Multiscale Entropy . ... A new measure of information is defined which is based on noise modeling and incorporates resolution scale. Properties of this measure are discussed. ... Additionally it allows for image noise modeling, and subsequent noise removal. ... Hence information- and entropy-based processing technologies will be necessary for the effective design and implementation of large, future generation, image databases. ...

Download Izmccd (~2.7 MB). ... a) a choice of the best mode of measurements of stars and objects ("Properties/Measurement"), . b) a choice of reference stars. ... 1) necessity of presence on an image of a plenty of stars (we recommend to apply this mode, if on the frame of reference stars is more 100) . ... Sx and Sy depend from residuals at all reference stars (reference stars are marked by blue color). ... These residuals are the image of the star a minus function of a profile for each pixel. ...

... Good detailed technical description of ISDN, somewhat more detailed than the Stallings book in some areas. ... Dan Kegel's ISDN Page - This is basically the center of the ISDN web, mentioned most commonly as a good place to start. comp.dcom.isdn Frequently Asked Questions (FAQ) - A great bunch of information, mostly consumer-oriented. ... NIST's High Speed Networks Group Home Page . ... Bellcore ISDN Home Page - National ISDN . ... Ascend Communications Home Page - they make ISDN equipment. ...