... Reference ID: CHU . Driver ID: CHU . Serial Port: /dev/chu u ; 300 baud, 8-bits, no parity . ... Unlike the NIST time services, whose timecode requires quite specialized hardware to interpret, the CHU timecode can be received directly via a serial port after demodulation. ... The time1 fudge option can be used to set the CHU propagation delay, compensate for inherent latencies in the serial port hardware and operating system. ... Not used by this driver. stratum number . ...

GIPSY programs do not interact with the user directly, but do this through the GIPSY user interface, Hermes . If for instance a program needs some input from the user, it will send a request to Hermes which will then prompt the user for the required parameters. ... If a program wants to inform the user that the integrated flux density of a source is x Janskys, it will not do this with an ordinary WRITE statement, but via a library routine which sends a request to Hermes. ... The default level . ...

PCI interface and backplane of NGC NGC Backplane General purpose Board features CompactPCI connector Ground and Power planes Bending of the backplane di Different backplane size Leander Mehrgan Backplane General purpose Designed to achieve requirements and specifications for: achie Excellent power distribution High speed differential pairs Mechanical specification Board features CompactPCI ... PCI controller done by the XILINX FPGA (IP core). ...

... Previous: Accessing Astronomical Data over the WWW using datOZ . ... Robust, distributed searching of networked-based astronomical databases requires an investment not only by individual data providers, but also by the astronomical community as a whole. ... Designing a distributed, networked-based astronomical information system requires a four-step approach including original data source analysis, modeling the system, profiling the system, and implementation of the system. ...

... GPI Data Pipeline 1.0 documentation . GPI Data Pipeline User?s Guide . ... Appendix: Rarely-Used and/or Nonsupported Advanced Features . ... IDL> gpi_launch_pipeline, single='my_recipe.xml',/noexit [IDL processes that recipe file and then returns to the IDL command line] . ... There exist various tools for interacting with the GPI pipeline from Python, including editing and manipulating recipe files, creating new recipes, checking pipeline configuration settings, and working with GPI data. ...

... This guide will provide the basic procedure for a "standard" wview install. ... If a package requires installation, you should use the package management utility appropriate for your OS and distribution. ... If they are, you should install the devel version in order to get the development libraries that radlib/wview needs. libz - compression library - normally included in OS distribution . ... libgd2 - graphics drawing library - may require installation - http://www.boutell.com/gd/ . ...

... Installing the NVIDIA Driver . ... NVIDIA distributes the source code to this kernel interface layer, as well as precompiled versions for many of the kernels provided by popular Linux distributions. ... You must have the source code for your kernel installed for compilation to work. ... After the correct kernel interface has been identified (either included in the .run file or compiled from source code), the kernel interface will be linked with the closed-source portion of the NVIDIA kernel module. ...

... The SF does not contain all the information required to process the ODF with the SAS. odfingest extends the SF with data extracted from the instrument housekeeping data files and the calibration database. It creates a new summary file: the SAS ODF Summary File (SOSF). ... The user need not have write access to the ODF directory. odfingest uses the parameter outdir to learn where to write the SOSF. ... Alternatively, the name of the SOSF can be passed to odfingest with the parameter summaryfile . ...

Astronomical Data Analysis Software and Systems VII ASP Conference Series, Vol. ... Distributed Searching of Astronomical Databases with Pizazz K. Gamiel, R. McGrath and R. Plante National Center for Supercomputing Applications, University of Illinois, Urbana, IL 61801 Abstract. ... In such a model, one would build a distributed searching gateway that would o#er a single user interface, but would map the user's query to each and every original data source in its native protocol and interaction style. ...

FEATURES OF THE HYDROGEN DISTRIBUTION AROUND LUNAR CRATERS PROCLUS AND KEPLER. ... In result of analysis of the data Lawrence and Feldman constructed the hydrogen distribution on the lunar surface [1]. ... However, the authors shown, that EN flux data features may be explained by other element abundance in the lunar soils, namely: Si, Ca, Gadolinium (Gd), Samarium (Sm) and Fe. ... Using of the Feldman's interpretation of the Lunar Prospector data [8], we constructed hydrogen distribution map (Fig.1). ...

... Star Atlas . ... stars . ... Nuclear fusion of hydrogen into helium powers stars, but fusion requires a lot of energy. Where does this energy come from? ... You re in good company: This question also stumped the physicists who first tried to understand nuclear fusion in stars. In a star s core, all atomic nuclei have been separated from their electrons, so each hydrogen atom is really just a proton and thus holds a positive charge. ... Get instant access to subscriber content on Astronomy.com! ...

... Contains properties describing the display screen and colors. ... JavaScript 1.2 The JavaScript runtime engine creates the screen object for you. ... Specifies the height of the screen, in pixels, minus permanent or semipermanent user interface features displayed by the operating system, such as the Taskbar on Windows. availLeft . ... Specifies the width of the screen, in pixels, minus permanent or semipermanent user interface features displayed by the operating system, such as the Taskbar on...

XmCCD ----- XmCCD has been tested most recently on Suse 10.1 and Suse 10.3 and it will probably run on most other recent Linux distributions. ... This distribution includes source code to utilize the Santa Barbara Instrument Group (SBIG) shared library libsbigudrv.so with a Motif-based graphical user interface program to control SBIG astronomical CCD cameras. ... The sources for these programs are available from the XmCCD home at http://www.astro.louisville.edu/moore/software. ...

... SGML . The text/html content type . In this section, we begin the specification of HTML 4.0, starting with the contract between authors, documents, users, and user agents. ... These recommendations are not normative and conformance with this specification does not depend on their realization. ... An HTML document is an SGML document that meets the constraints of this specification. ... A user is a person who interacts with a user agent to view, hear, or otherwise use a rendered HTML document. ...

... Kernel . ... This article is part of the LWN Porting Drivers to 2.6 series . Much of the core network driver API has not been changed between the 2.4 and 2.6 kernels. ... Instead, your driver should disable any further "packet available" interrupts and tell the networking subsystem to poll your driver shortly to pick up all available packets. ... The next step is to create a poll() method for your driver; it's job is to obtain packets from the network interface and feed them into the kernel. ...

As of 1.3, the Apache source directories have been re-organised. This re-organisation is designed to simplify the directory structure, make it easier to add additional modules, and to give module authors a way of specifying compile time options or distribute binary modules. ... The non-module source files have moved from src into src/main . ... Configure . ... For example, say it is called mod_demo.c. The archive for this module should consist of two files, in a suitable directory name. ...

http://hea-www.harvard.edu/AstroStat/slog/2008/ tests -of- fit -for-the- poisson - distribution / Weaving together Astronomy+ Statistics +Computer Science+Engineering+Intrumentation, far beyond the growing borders Fri, 01 Jun 2012 18:47:52 +0000 hourly 1 http://wordpress.org/?v=3.4 http://hea-www.harvard.edu/AstroStat/slog/2008/ tests -of- fit -for-the- poisson - distribution /comment-page-1/#comment-267 ... Abstract: Improved №З2 statistics are defined for both Poisson and multinomial data sets. ...

... Unlike clients such as Shout and IceDJ this permits the broadcast of live audio, rather than prerecorded mp3's. LiveIce was developed after the appearance of IceCast to provide the Real Time streaming functionality which makes it a viable solution for broadcasting. It is based on the guts of 2 of my previous works - Mp3Serv, the first mp3 broadcasting system & Mp3Mixer, a toy which allows the user to 'Mix' with mp3 streams. ... LiveIce XMMS sourcecode is available here . ...

... Calculations of at least two runs with different values of a parameter are required in order to discover to what extent the results depend on the , if at all. ... In order to study how the final statistical distributions depend on the initial functions, the method of Green functions is used. ... Then we can restore any distribution on this parameter (with a certain accuracy) by summing the results for each interval with the appropriate weight. ...

MRO Delay Line ICD Delay Line to Vacuum System ICD INT-406-VEN-0011 The Cambridge Delay Line Team rev 0.2 18 Jan 2008 Cavendish Laboratory JJ Thomson Avenue Cambridge CB3 0HE UK 1 ICD Description Sub-systems Delay line Vacuum system Org MRAO Owner MF Brief description and preliminary contents Defines the mechanical interfaces on the delay line pipe required to connect to the vacuum system. ... Figure 2: An exploded view of the proposed assembly which connects to each delay line pipe. ...