. Ceilidh Notes 1 --- Introduction . Ceilidh Notes 2 --- Basics . Ceilidh Notes 3 --- If and Switch . Ceilidh Notes 4 --- Loops . Ceilidh Notes 5 --- Array and structures . Ceilidh Notes 6 --- Pointers . Ceilidh Notes 7 --- Functions . Ceilidh Notes 8 --- File I/O . Ceilidh Notes 9 --- Process management . Ceilidh Notes 10 --- Questionaire . Dave.Marshall@cm.cf.ac.uk . Wed Sep 14 10:06:31 BST 1994

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• Programming in C

... Display (spectra, total power). ... Using the data archive. ... entering cmds, editing cmd lines, input from files, batch, run. constants, variables,arrays, structures, operators, procedures, functions. programming in idl . ... A user would call arch_gettbl() to input the table (or a subset of it). corfindpat() can create subsets of the table. arch_getdata() or arch_getonoff() can be used to read in the spectra. ... input the data (spectra) for a subset of the archive table: arch_getdata () . ...

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• byu phased array feed.
• system Performance
• T2874 meteors on moon.

... Up: Science Data Pipelines . ... Real-time Linux is a set of extensions to the kernel that provides hard real-time functionality with low, bounded latencies and deterministic response. ... This paper, presents the fifos and shared memory virtual interface (VIs) that allow LabVIEW to communicate and share (bulk) data with the real-time core. The cardinal programming rule of real-time Linux is to do as much as possible in user space with only critical sections of code in the real-time core. ...

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• A Generic Data Exchange Scheme Between FITS Format and C Structures
• Spatial Structure of NGC 6822: An Example for Statistical Modeling of
• Heuristic Estimates of Weighted Binomial Statistics for Use in Detecting Rare

WCSLIB љ 5.15 . ... Memory management . The initialization routines for certain of the WCSLIB data structures allocate memory for some of their members: . wcsini() optionally allocates memory for the crpix , pc , cdelt , crval , cunit , ctype , pv , ps , cd , crota , colax , cname , crder , and csyer arrays in the wcsprm struct (using linini() for certain of these). Note that wcsini() does not allocate memory for the tab array - refer to the usage notes for wcstab() in wcshdr.h . ...

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• WCSLIB: disprm Struct Reference
• Package: dsproc
• Package: dsra

As it was already mentioned, the idea behind File Juggler is rather simple: using CGI scripts as processing tools and WWW browser as user interface, display the structure and content of typical anonymous FTP server in a convenient, easily navigated form. ... My P5-133 spends about 0.025 ms on one file when doing linear search with simple criterion (690 ms for 27,000 files, search for substring among file names/descriptions with 70 hits). ... Let's now look whether we can handle 1,000,000 files. ...

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• Dos32QuerySysState API
• INTRODUCTION
• Pointers

... Perform basic two-dimensional image reduction. Reject cosmic rays from CCD data. Process the contemporaneously obtained wavecal data to obtain the zeropoint shifts in the spectral and spatial directions. ... Subtract science image from wavecal . ... For each image in the science file, this task selects the wavecal in the wavecal file that is closest in time to the science image, and it copies the keyword values for the spectral shift from that wavecal header to the science header. calstis12 . ...

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• Rodger Doxsey - How HST Works
• CALSTIS V1.9 Release Notes
• STIS Data Handbook

Next: *.imh and *.qp Extensions Up: IRAF/PROS Files Previous: IRAF Image Arrays . The x-ray data are stored in QPOE files (Quick Position-Ordered Events, *.qp ) rather than image arrays. ... Note that, unlike IRAF images, QPOE files have no associated header file, and are always stored in the current directory, unless explicitly specified otherwise. Non-PROS IRAF tasks can also access QPOE data files in place of image arrays. ... rp110590.qp[pi=2:30] . ... The ROSAT PSPC qp file images are . ...

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• Chandra Supernova Remnants Catalog - Note on Data Processing
• The AstroStat Slog spatial statistics
• The AstroStat Slog poisson point process

spaceweb@oulu.fi - last update: 20 September 1998, 2020 UT (RR) . Traveling Convection Vortex (TCV) is a name given to a specific type of daytime magnetic impulsive events observed by high-latitude ground-based magnetometer arrays. Since the most likely source for TCVs is the solar wind , they are considered to be important processes in transfering energy from the solar wind into the magnetosphere . ... For example, one AMPTE Lithium release in the solar wind caused a TCV event . ...

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• Lagrangian Points
• Magnetic Fields -- History
• The Wind Spacecraft

. XMM-Newton Science Analysis System . dataconv (sas-1.443) [xmmsas_20050815_1803-6.5.0] . Meta Index / Home Page / Dataset structure / Images . Should the associated arrays immediately follow the data array they refer to? . XMM-Newton SOC/SSC -- 2005-08-15

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• Dataset structure

... The Plug-in Guide is your introduction to using Netscape's Plug-in Application Programming Interface (API) to develop plug-ins for Communicator 4.0. ... If you decide to use Netscape's LiveConnect to allow your plug-in to communicate with Java and JavaScript, your next step after reading this guide is LiveConnecting Plug-ins with Java . ... The Plug-in Software Development Kit . ... The Plug-in Guide is designed for the C or C++ developer who wants to extend the capabilities of Netscape Communicator...

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• Notes on specific commands
• Apache 2.0 Hook Functions - Apache HTTP Server
• CCD Technical Note

Previous Next Table of Contents . Increasing the Threshold value will have dramatic effects on the time it takes to process and image. ... Increases in Flare Intensity and Spike Points will also significantly increase processing time, although probably not as much so as the increase in Threshold. Changing the Spike Color from white to either background or foreground will increase the time to process the image, but the increase is not significant. ...

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• Zen: spgist dev
• Oleg Bartunov's Home Page
• Zen: Tsearch V2 in Brief

... Bojan Nikolic web pages (r. 329) . ... http://carma.astro.umd.edu/wiki/index.php/Installing_Developer_CASA . Building CCMTools as required by CASA . ... Building . ... Notes related to building CASA . A prototype build system for CASA using SCons . ... Generating IDL files . ... Notes on the classic CASA build . ... Writing the tool XML file . ... Automatically generated IDL files from the files describing each of the tools of CASA. ... Building CASA . ... Building the casa-core libraries . ...

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• OptInt PmWiki : Tech Meet 12 | History
• A prototype build system for CASA using SCons Bojan Nikolic web pages (r. 329)
• OptInt PmWiki : Other Variables

... Current APO Weather . ... Search Site . ... Information for New Users . ... Technical Staff pages . Night Logs and Mailing Lists (maintained by APO) . ... Technical Documents and Database Search . ... Observer's Documentation and Procedures . ... Problem Reporting and APO Technical Documents Database Search . ... APO Drawing/Document Management Procedures . ... APO Technical Documents Database Search . Home Astrophysical Research Consortium . ... Mail Lists (maintained by APO) . ...

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• Pointing error budget
• Primary mirror support
• Apache Point Obs. on-site detectors

... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Developer Documentation . ... In general, a hook function is one that Apache will call at some point during the processing of a request. ... Use the AP_DECLARE_HOOK macro, which needs to be given the return type of the hook function, the name of the hook, and the arguments. ... During initialisation, the server will call each modules hook registering function, which is included in the module structure: . ...

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• Hook Functions in the Apache HTTP Server 2.x - Apache HTTP Server
• Sitemap - Apache HTTP Server
• Developer Documentation for Apache 2.x - Apache HTTP Server

... Imaging of the core of the OMC-1 region using NICMOS camera 2 through the F212N and F215N filters shows a wide variety of interesting structure on scales of 0.2" at a very high dynamic range (Stolovy et al. ... The application of image restoration techniques, including multi-channel variants of the Richardson-Lucy technique, offers the chance to enhance structure on the finest scales and also to suppress the prominent and richly structured point-spread functions of the many bright stars in the...

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... Summary of reduced ISAAC fields . ... This data release includes eight fully reduced VLT/ISAAC fields in J,H,K s bands covering 50 arcmin 2 of the GOODS region in the Chandra Deep Field South (CDFS). ... 8 ISAAC fields) . ... The 8 ISAAC fields which are part of this data release are superimposed onto a SOFI image (J+K) (part of a previous EIS data release). ... In one case (GOODS field 11/J-band), for which not enough standard stars were available, the ZP was boostrapped from previous SOFI/EIS data...

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• Organization of data
• The Very Large Telescope Project
• DFS department intranet: welcome !

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

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• Formation of the Earth's Moon
• Formation of the Earth's Atmosphere and Oceans

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... ClassљIndex . ... StelVertexBuffer< V > Class Template Reference . Vertex buffer interface. ... Destroy the vertex buffer. ... addVertex (const V &vertex) . ... getVertex (const int index) const . Return vertex at specified index in the buffer. ... setVertex (const int index, const V &vertex) . Set vertex at specified index in the buffer. ... Each StelRenderer backend might have a different vertex buffer buffer implementation. ...

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• Stellarium: StelQGLInterleavedArrayVertexBufferBackend Class Reference
• StelVertexArray Struct Reference
• Stellarium: StelQGLArrayVertexBufferBackend Class Reference

... Class . ... SUMMARY: NESTED | FIELD | ... METHOD . DETAIL: FIELD | ... java.lang.Object ij.process.FloatPolygon . public class FloatPolygon . ... Used by the Roi classes to return float coordinate arrays and to determine if a point is inside or outside of spline fitted selections. ... float[] . ... Field Detail public int npoints . ... Constructor Detail public FloatPolygon (float[] xpoints, float[] ypoints, int npoints) . ... Method Detail public boolean contains (float x, float y) . ...

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• MaximumFinder (ImageJ API)
• RankFilters (ImageJ API)
• GaussianBlur (ImageJ API)

... For Teachers . ... Since no math is involved, they can be presented in a 9th grade Earth Sciences course, and even to younger students. ... Permanent magnetism and the magnetism of the Earth. Magnetism caused by electric currents . ... You may send comments, questions and corrections to my home address, earthmag("at" symbol)phy6.org . ... The teacher may skirt this area when the subject of the origin and reversal of the Earth's magnetic field comes up, by simply stating the bare facts, namely . ...

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• FAQ: "The Great Magnet, the Earth"
• The Sun--Introduction
• Magnetism