DIMM=Dual Inline Memory Module . ... 168 PIN DIMM at the computer. Front Side (left side 1-42, right side 43-84) Back Side (left side 85-126, right side 127-168) . Pin . ... VSS . ... Data 0 . ... VDD . ... Serial Data . ... 168 . ...

DIMM=Dual Inline Memory Module . ... 168 PIN DIMM at the computer. Front Side (left side 1-42, right side 43-84) Back Side (left side 85-126, right side 127-168) . Pin . ... VSS . ... Data 0 . ... Serial Data . ... 168 . ...

The original files with the data were in different formats. ... Such files were named "standard data files" and linked to the database. They can be easily transformed to any desirable format by a code. Here we present two simple computer programs of this kind. ... When running the code, you can specify columns in the output file: wavelength, energy (eV) or wavenumber (cm -1 ) as the first column, and complex refractive index or dielectric function as the second and third columns. ...

... Q. May I connect my laptop (PDA) to MCCME local network? ... If you are going to use our network several times, please write a letter to the system administrator (Sergey Dubov, <dubov (at) mccme.ru>). Please mention your name, your login name on mccme.ru (if any), the version of the operating system you are using, and the MAC address of the network card. ... Q. What settings should I use (IP address, network mask, gateway)? ... Q. May I connect my computer to the network using 802.11 protocol? ...

... Each box has 5 digital output cards and each card holds 16 bits (80 bits in total). ... They go to things that are not duplicated in the two polarization chassis (e.g. cal source ). Schem : The reference number on the schematic (see schematic pdf file). ... ref numbers 9-12 : page 3 of 3 260 to 30 mhz converter (.pdf) . ... in). if Input . ... selects the input path thru the iflo . mix1inp . ... Selects the source input to the mixer . ... see mix1inp . ... syn1 dest . ... same as syn1 dest . ...

A computer controlled low light photometer for nightglow observations. Hardware units of portable photometer for low light measurements, especially night glow emission is described. ... Interface card contain three channels of 24 bit counter, 4 channels of 12 bit ADC and the buffer bus for the controlled motors of the altazimuthal fork mounting and filters wheel, the position encoders. ... Where N( ) is output signal photometer generated input light flux F( l ) . ... PMT # . 599 . ...

... User Guide ] Task: impol Purpose: Compute polarized intensity and position angle from Q and U Categories: image analysis IMPOL computes the total linearly polarized intensity (optionally debiasing it) and position angle images from Stokes Q and U images. Position angle is positive N -> E. Key: in Up to three values; the Q, U and I images, respectively. ... Key: poli Up to two values; the output polarized intensity image and optionally, its associated error image (which will be constant). ...

To contrast two files: sdiff -w 80 email addresses Mike erpl08@ed | ... This contrasts the two files email on the left and addresses on the right. The option -w 80 is used to set the width of the output from the command to 80 characters - the most that will fit across most computer terminals. The default is 130 characters. The first line in each file is different and is marked with a | Lines 3 and 4 of the file addresses are unique as is line 6 of the file email . ...

... Here is some programming information for common ports that can be directly used for general-purpose TTL (or CMOS) logic I/O. If you want to use these or other common ports for their intended purpose (e.g., to control a normal printer or modem), you should most likely use existing drivers (which are usually included in the kernel) instead of programming the ports directly as this HOWTO describes. ... The game port has a quad one-shot multivibrator (a 558 chip) connected to the four inputs. ...

Motif and X-Windows . It is possible to execute a Motif application on a computer around the corner or around the world and redirect the input and output for the application to your workstation. There are files located on the Science Cluster to help you position and display windows from a remote VMS system. ... Copy two command files: . ... From one of the workstation windows, have the remote system execute the x command file and create the display on your workstation by using this command: . ...

This note outlines how to configure the computers needed to run DIMMWIT. ... dimmwit : ICE (single-board computer in a box) that runs the Starlight Express CCD camera, to which it is connected by a USB interface. dimmwithost : displays the finder application via the X protocol (finder actually runs on dimmwit). Acts as a file server; both the finder software and the DIMM data are stored on dimmwithost. ... mkdir -p /data/oberon/data/finder . chown coast:coast /data/oberon/data/finder . ...

... The satellite ephemeris is used to compute arrival time corrections from the satellite to the solar system barycenter, appropriate to an input celestial position. ... output files: rp110590n00_cor.tab, rp110590n00_ephem.tab ti> calc_bary input ephemeris table : xdata$rp110590_eph.tab # A Rev. 0 file root name for output file(s) [root_cor(ephem).tab] : . ... Output file: ./rp110590_ephem.tab Output ephemeris table: ./rp110590_ephem.tab Computing Correction table .. ...

... Standard Commands . ... TclActor is core code for writing an actor: an instrument control computer (ICC) or hub-based script that does something useful. This manual describes the standard commands and keywords that any actor based on TclActor will support. ... All actors based on TclActor typically support the following standard commands (plus additional device-specific commands documented in that actor's manual). ... Connect one or more devices (if not already connected). ... Added ping command . ...

... PSF2_CORR - The point-spread function correction that may have been applied to extrapolate the corrected count rate from 12 to 35 unbinned pixels, defined by (corrected counts at 35 pixels / corrected counts at 12 pixels) * 100. ... MAG The instrumental magnitude computed using the corrected count rate and using the appropriate calibration constants for the filter. MAG_ERR The error in the computed instrumental magnitude. ...

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 . ...

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . Founded in 1983, COPI is an innovator in the design of optical encoders. ... Listed Since July 15, 1998 . ... 818) 882-0424 . ... 818) 882-0492 . Web Site . ... Web . www.astronomy.net . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

Armagh Observatory, 21 December 2001: . ... The Armagh Observatory's contribution, led by astronomers Simon Jeffery and Gerry Doyle , is to develop new computational tools to study the atmosphere of the Sun and other stars. ... Computers will communicate with one another using the grid, and computing power will become a commodity just like electricity. ... FOR FURTHER INFORMATION CONTACT: Simon Jeffery or Mark Bailey at the Armagh Observatory (Tel.: ... WWW contact: webmaster@star.arm.ac.uk . ...

... To introduce you to the Python programming language, and its Visual module (VPython), which allows 3D simulation. The computer labs are held in room BOZO 112, not in the usual physics lab. ... This lab will use the Python programming language. ... Click on the Windows button in the bottom left, select "Programs", then the "A-Z" list of programs. ... Later in the course you will need to write your own VPython programs for assessment - this lab is your chance to make sure you can do this. ...

SXG Data Center . ... SXG instruments models . Data archive . ... SXG Scientific Data Output Modelling . The task of SPECTRUM-XG Scientific Data Output Modelling is multifold: Utilization of experiment data output computer simulations in pre-flight calibration of mission instruments. ... Utilization of computer simulations in the data analysis software development. The prototype of SXG X-model project is being realized at IKI. ...

... Dr. Ravil Nazirov is the head of the workshop, and Andrew Ananjev is the secretary of the workshop. ... The workshop is used to be held in the last decade of the month, preferably on Tuesdays. ... The next session will take place October 29, 1996 . ... There is "CONPAS" mailing list which you can join to discuss issues of problem solving and to be automatically notified of important dates and decisions with respect to the coming sessions. ... Secretary of the Workshop: Andrew Ananjev . ...