Fortran 90 properties already in CF77 . ... Only the old form (fix form) of the source code is available. ... LOGICAL Default KIND number = 8 INTEGER Default int7 int15 KIND number = 6 1 2 digits = 46 7 15 radix = 2 2 2 range = 13 2 4 huge = 70368744177663 127 32767 bit_size = 46 8 16 INTEGER int31 int46 int64 KIND number = 4 6 8 digits = 31 46 63 radix = 2 2 2 range = 9 13 18 huge = 2147483647 70368744177663 9223372036854775807 bit_size = 32 46 46 REAL half Default,single double KIND ...

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• Adding Variables to CONFIG.SYS
• The new precision concept
• Tutorial on Fortran 90, Digital UNIX

... Lets you work with numeric values. The Number object is an object wrapper for primitive numeric values. ... JavaScript 1.3: added toSource method . ... value . ... JavaScript 1.2: Number(x) now produces NaN rather than an error if x is a string that does not contain a well-formed numeric literal. ... The following example uses the Number object's properties to assign values to several numeric variables: biggestNum = Number.MAX_VALUE . ... ECMA-262 JavaScript prints the value Number.NaN as NaN . ...

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• htcacheclean - Clean up the disk cache - Apache HTTP Server
• Top-Level Properties and Functions
• mod_mem_cache - Apache HTTP Server

... Earnshaw's second clock has a 5-bar compensation pendulum of steel and zinc, an 8-day movement, rated at very nearly sidereal time. ... 8 day English regulator in mahogany case, signed by Thomas Earnshaw, London, C179O. Maximum external dimensions (Cms): Height:l84 Width:45 Depth:3O.5 . ... Original five bar Zinc and Steel gridiron pendulum, suspended on a gold painted,cast iron pendulum support, firmly screwed to the backboard of the case. ... The dial is signed: "Earnshaw London" across the centre...

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• Performance
• Why Asteroid 2008 TC3 Represents a Landmark - Dr David Asher, from Armagh
• Hot subdwarfs

... We have compared visualized fields of GSC and USNO A1.0 catalog with unpublished photographic finding charts that were sent by L. Plaut to the compilers of the GCVS. ... 7-15 A9 --- GCVS GCVS or NSV name 17-25 F9.4 --- GSC GSC number 26 A1 --- NoteFlag *Nonstar (GSC) flag 28-29 I2 h RA2000GSC.h Hours RA (GSC), equinox 2000.0 31-32 I2 min RA2000GSC.m Minutes RA (GSC), equinox 2000.0 34-38 F5.2 s RA2000GSC.s Seconds RA (GSC), equinox 2000.0 40 A1 --- DE2000GSC.- ... Plaut, L., 1966, Bull. ...

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• Future Prospects of Variable-Star Catalogues
• General Catalogue of Variable Stars: classification.
• Презентация PowerPoint

... Users . ... Data Collection and Analysis . ... This particular part of the analysis has been disabled since the code is struggling to cope with the number of users seen this year, in particular the large contingent of people who have re-tweeted NASA. ... Order accounts: by user number (effectively random) by number of tweets (includes retweets) by number of followers by number of followers that also tweeted about AAS225 by number of friends that also tweeted about AAS225 . ... by user number . ...

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• A matrix of tweets from #AAS223
• A matrix of tweets from #AAS221
• SAOtng Colormap Considerations

To set a number of options place the set commands in the file .exrc . set ic set number set sh=/usr/local/bin/Tcsh set wm=5 . This sets vi to: . ignore the case of characters in searches . display line numbers . use the TC shell to execute UNIX commands . ... Options can also be set using the environment variable EXINIT. setenv EXINIT 'set ic number sh=/usr/local/bin/Tcsh wm=5' . For the C and TC shell user, this sets the same options as in the example above. ...

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• Examples of using the uniq command
• Changing shell variables
• Special shell variables

... Up: Data Analysis and Processing Techniques . ... Also, a method for quality control of CCD observations is suggested. ... Everyone who observes a celestial object using a CCD detects moving celestial objects as a ``by product''. ... We hope that our investigations may be useful for near-Earth space control and also for searches of the moving celestial objects through analysis of old and new CCD frames obtained at any amateur or professional astronomical observatory. ...

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• Spatial Structure of NGC 6822: An Example for Statistical Modeling of
• Spatial Models and Spatial Statistics for Astronomical Data
• A Method for Visualizing Time Variability in X-Ray Images

Comedi Documentation . ... Right to the source: #include <stdio.h> /* for printf() */ #include <comedilib.h> int subdev = 0; /* change this to your input subdevice */ int chan = 0; /* change this to your channel */ int range = 0; /* more on this later */ int aref = AREF_GROUND; /* more on this later */ int main(int argc,char *argv[]) { comedi_t *it; lsampl_t data; it=comedi_open("/dev/comedi0"); comedi_data_read(it,subdev,chan,range,aref,&data); printf("%d\n",data); return 0; } . ...

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• Further Data Types
• Time Functions
• Integer Functions, Random Number, String Conversion, Searching and Sorting:

Numbering Procedures for APO 2.5m and 3.5m Drawings and Engineering/Drafting Documents . ... Document part numbers are to consist of a 7 character long "base numbe,r" which is coded to provide information about the part's intended first use. The part number becomes complete and unique only with the addition of a revision number. ... Example of a "base number": 25CSA01 . ... PART NUMBER CONVENTION . ... For Example: . ... R = "Revision" . ... Questions contact Larry Carey/University of Washington ...

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• field
• DIS Keywords
• coordConv Version History

. F IGURE . 1. Distributions of RR Lyrae stars in distance (a)from the Sun and (b) from the Galactic plane.The shaded part of the histogram corresponds to stars with known proper motions.The curve in the left histogram is a power-law approximation for the growth of the number of stars with distance in the intial sample for R < 1.75 kpc. is the power-law exponent. The dip in the right distribution near Z ? 250 pc is due to selection effects. discussion in the text | next figure .

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• RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, tabl
• T.Borkova, V.Marsakov, Subsystemsof RR Lyrae Variable Stars in Our Galaxy
• F-stars in galactic disk, figures

... M27: Not A Comet . 9.10.1998 . ... Far Side of the Moon . ... These North (left) and South Pole projections are based on SeaWiFS measurements made between September 1997 and July 1998. ... On July 20th, 1969, a human first set foot on the Moon. ... Despite the innocuous sounding name, the launch of the Earth's first "artificial moon", Sputnik 1, by the Soviets on October 4, 1957 shocked the free world, setting in motion events which resulted in the creation of NASA and the race to the Moon. ...

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The revision of the MASS/DIMM star catalogue N. Shatsky, V. Kornilov March 16, 2008 Abstract The compilation of the (updated) version of the MASS (MASS/DIMM) device target catalogue is described. ... Then the list was cleaned according to following criteria: I. Remove stars too faint for a MASS device. ... Here the color equation of the Sternb erg device was taken: M AS S mag = V mag + 0.45 (B - V ); stars with M AS S mag > 3.2 were removed. ... This was made based on the GCVS4.2 catalogue data. ...

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This module provides support for dynamically configured mass virtual hosting . ... Source File: mod_vhost_alias.c . ... For simple name-based virtual hosts you might use the following directives in your server configuration file: UseCanonicalName Off VirtualDocumentRoot /usr/local/apache/vhosts/%0 . A request for http://www.example.com/directory/file.html will be satisfied by the file /usr/local/apache/vhosts/www.example.com/directory/file.html . ... Module: mod_vhost_alias . ...

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• Descriptors and Apache
• Apache module mod_status
• Environment Variables in Apache

Magnetic Stars, 2011, pp. ... 2008). ... The origin of magnetic fields of hot massive stars is explained by the fossil field theory, MAGNETISM OF STARS 451 1-5 Be measurements -> 1278 stars 100 N stars 6-10 Be measurements -> 80 stars 50 11-15 Be measurements -> 47 stars 0 20 40 60 80 100 120 140 160 180 The namber of individual measurements The number of individual measurements Figure 1: The number of stars in a single bin versus the number of individual Be determinations for a single star. ...

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• http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p476.pdf
• http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p153.pdf
• Metagalaxy sector, archive 2005

Rules for natural satellites observation rough data CONTENT file Version 28.06.2000 /Arlot J.-E., Emelianov N./ ------------------------------------------------------------------ Contents. ... IAU code> - <observatory name> <NL> <NL> Reference. ... planet number>-<planet name>[:<quantity>], <NL> <satellite number> [-<temporary name>] [-<satellite name>]:<quantity> , <NL> ... <satellite number> [-<temporary name>] [-<satellite name>]:<quantity> <NL> reference frame: astrometric | ...

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• IDL programs
• ji0005
• Natural Satellites Service. Apparent Encounters of the Tycho-2 Catalogue stars

... Note that the size of the returned array may be greater than the number of slices currently in the stack, with unused elements set to null. public int getSize () . Returns the number of slices in this stack. public java.lang.String[] getSliceLabels () . ... Returns null if the stack is empty or the label of the first slice is null. public java.lang.String getSliceLabel (int n) . ... Returns null if the slice does not have a label. public void setSliceLabel (java.lang.String label, int n) . ...

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• PolygonRoi (ImageJ API)
• Tools (ImageJ API)
• Line (ImageJ API)

The classic solution for homogeneous sphere was suggested in 1899 by A.E.N. Love [ 330 ], in 1908 by G. Mie [ 342 ] and in 1909 by P. Debye [ 199 ]. ... Traditionally the theory of light scattering by a sphere is called the Mie theory. ... The exact solutions of the Mie problem for an optically active sphere (i.e. a sphere of optically active material [ 7 ]) and for a sphere with an optically active mantle were first obtained in 1974-5 by S. Bohren [ 158 , 159 ]. ...

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• Database of Optical Properties -- Level: subpage
• Model realization and some results
• Point matching method

. Full screen versions . Number - magnitude counts . Number - redshift counts . | Front page | . | << - Redshift wedge | Completeness estimates - >> | . Robert J. Smith, ">rsmith@mso.anu.edu.au Last modified: Fri Sep 24 11:39:02 EST 1999 .

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• Dunk Proceedings - 2dF QSO Redshift Survey (Number-Magnitude Relation)

... GCR and SCR are primary cosmic rays. 10-15 years after the discovery of cosmic radiation (1919) there emerged two main avenues of investigation in the physics of cosmic rays (CR): 1) nuclear - elucidation of the origin of elementary particles and nuclear interactions; and 2) astrophysical (space physics) - solution of the problem related to the origin and variations (changes in intensity) of CR. ... Besides, the CR flux in interplanetary space is, strictly speaking, not isotropic. ...

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... Tables for transformation from sidereal to universal time scale. Explanations. This page contains three little tables headed Hours Minutes Seconds respectively. Each the table have two columns: first of them is input column where time in whole time units of sidereal time is given, and second of them is output column where hours:minutes:seconds of universal time is presented. ... Example: transform 02 h 12 m 22.00 s from sidereal to universal time. ...

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• Explanation to tables for transformation from universal to sidereal time.
• Lunar eclipce explanation page of Computer Ephemeris (DE200/LE200).
• Apparent places of fundamental stars for Computer Ephemeris for 2014