The head of laboratory is Prof. Vladimir A. Cherepenin, e-mail: cher@cplire.ru . The main research field of the laboratory is computer simulation of physics processes in radio science and electronics. ... development of numerical models for coherent radiation of relativistic electron beams in open and superdimentional electromagnetic structures; . ... Computational physics laboratory is concerned with organization and development of computer network in the institute. ...

A problem, that can arise when moving from Fortran 77 to Fortran 90, is dependent on a usual deviation from the standard, and has to do especially with user programs. ... With many Fortran 77 implementations we wrote PROGRAM TEST REAL X WRITE(*,10) 10 FORMAT('Give X = ',$) READ(*,*) X WRITE(*,*) X END In Fortran 90 we use "non-advancing I/O" instead. ... In some old Fortran dialects the statement TYPE was used to write on a typewriter terminal and PRINT was used to write on the line printer. ...

Next: Generation from In-Orbit Data Up: BADPIX Previous: Description Contents . In the CSL images there is clear evidence of edge emission. ... Pinhole images are almost free of any background and are not suitable to identify further defects. ... The CCD used in these measurements had an arbitrary location in respect to the intensifier. Two images were taken with the CCD rotated by 90 degree to distinguish between intensifier and CCD defects. ...

. ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

... at the ISSP RAS. ... MSU student Kostretsova N.B. successfully defended her thesis entitled "Investigation of Thermal and Chemial Expansivity of Ceria-Based Solid Solutions". ... V.A. Kolotygin successfully defended his PhD thesis "Perovskite-Like Oxide and Composite Anode Materials for Solid Oxide Fuel Cells: Functional Properties and Electrochemical Behavior in Contact with Gallate- and Silicate-Based Solid Electrolytes" and was awarded PhD degree in the area of Materials Science and Engineering ....

... Science . ... Science Users Information > Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Next generation Fornax Cluster surveys . ... Data Handling and Products . ... Science Data Products Forum . ... An international team, with Dr. Hilker as Co-PI, has started to gather wide-field optical and infrared imaging data as well as spectroscopic data on the whole extent of the Fornax cluster, mainly based on observations with ESO telescopes (VLT, VST, VISTA). ...

... More than 100 circumstellar gas clumps with ionized rims have been detected by HST studies of the Orion Nebula H II region (O'Dell & Wong 1996). Seven additional objects appear as dark oval silhouettes seen against background nebula light (McCaughrean & O'Dell 1996); these are very likely to be protoplanetary disks seen in absorption. ... Eight fields were observed in H and I-band continuum in the nearby H II regions NGC 2024, NGC 2264, and S155. ...

Next: HST Paper Products: A New Way to Look at HST Data . ... After providing on-the-fly re-calibration of HST data to archive users, ST-ECF has embarked on a new project aiming at grouping, cosmic ray cleaning and drizzling images taken by most HST instruments. ... The production of the missing jitter files combined with the extraction of additional engineering parameters will greatly enhance the homogeneity and the scientific value of the entire archive. ... 1995, HST Data Handbook, STScI, 107 . ...

Next: Time Series Analysis Up: No Title Previous: Command Syntax Summary . This manual is intended as a guide to the use of the digital stellar photometry reduction program DAOPHOT II: The Next Generation. ... In DAOPHOT II: The Next Generation all of the major algorithms and actual FORTRAN coding are done by Stetson, with the exception of those Figaro, IRAF, or MIDAS routines which are used for the image input and output. Stetson is solely responsible for bugs and algorithm-related problems. ...

... user-defined data file formats . ... better integration with a user's analysis routines To add such functionality to SAOimage, we developed the XPA Messaging System that allows X programs to define points of public access through which data and commands can be exchanged with external programs. ... We have utilized XPA to develop "SAOimage: The Next Generation" (SAOtng), an extensible image display service that can cooperate with other processes and programs. ... SAOtng help pages . ...

AMD OpteronTM 6200 Series processors AMD OpteronTM 4200 Series processors Compiler Options Quick Reference Guide Open64 Latest release: 4.5.1, December 2011 http://developer. amd .com/open64 Architecture Generate instructions specific to Interlagos Generate instructions for the local machine Optimization Levels Disable all optimizations Local optimizations Global optimizations (default) Additional aggressive ...

First Name . Last Name . ... A contributed talk . A poster . ... Tentative title of your oral contribution/poster . Required if ask for a Poster or Talk . ... Required if you are member of a collaboration . Short abstract of your oral contribution/poster . Required if you ask for a Poster or Talk . Options . ... Please select additional options . ... Please check the required fields. Powered by jqueryform.com . ...

... Welcome to the X-Ray World Wide Web Server! This server has been operational since April 1994. ... It is the repository of the COREX bibliography and database, the Henke atomic scattering factors, and other information of interest to x-ray spectroscopists. It provides links to additional locations for information about x-ray research, including conferences , synchrotron radiation laboratories , and other x-ray related Web or FTP sites . ... UW Synchrotron Radiation Center (Stoughton, WI USA) . ...

. md5 [ -0123456789 ] [ -h] file . This program generates the message digest of the given file using the RSA Message Digest 5 (MD5) and other selected algorithms. If file is not given, the program uses the standard input. -0123456789 . Select algorithm from the following list . -0 null . -1 MD5 . -2 SNEFRU . -3 CRC32 . -4 CRC16 . -5 MD4 . -6 MD2 . -7 SHA . -8 HAVAL . -9 null . -h . Display the result in hex; the default is base-64 . David L. Mills (mills@udel.edu)

... Imaging spectrometer for atmosphere and ionosphere spectral investigation consist the static Michelson interferometer and CCD camera. The prototype of the onboard CCD camera for the spectrometer used the Toshiba 2048 pixels CCD linear array (TCD 1201D) with FPGA-based controller. The controller is building on ACTEL A1020A field programmable gates array with maximum data rate 40 MHz and can be used with linear and area array CCD. ... Toshiba CCD Linear Image Sensor Data Book, 1997. ...

Observations of stellar magnetic fields is a powerful method to study of different non-stationary effects in our Galaxy and behavior of plasma under astrophysical conditions. ... Investigations of stellar magnetism by means of Zeeman measurements of polarized spectra of different stars are one of the most significant observational programme on the 6-m telescope BTA of our Observatory. ... Laboratory for the Stellar Magnetism Study . ... Laboratory for the Stellar Magnetism Study of SAO of the RAS . ...

... Samara State Aerospace University Staff Karpeev Sergey Vladimirovich . ... Paranin V.D. , Karpeev S.V. , Khonina S.N. Control of the formation of vortex Bessel beams in uniaxial crystals by varying the beam divergence // Quantum Electronics . ... Khonina S. N. , Karpeev S.V. , Alferov S.V. and others. ... Khonina S.N., Karpeev S.V. , Alferov S.V. Polarization converter for higher-order laser beams using a single binary diffractive optical element as beam splitter // Optics Letters. ... S.V. Karpeev ...

The HAWAII detector is an array of HgCdTe photodiodes whose junction capacity collects a charge proportional to the number of photons that they receive. ... The array detector is read by an electronic system based on the controller developed by the CCD Working Group of TNG, modified to speed up the read-out time, and on a fast 16 bit conversion board (2 Mb/s). ... The signal read on each pixels is buffered by electronics located on the same board that hosts the detector. ...

... Department address: . ... Battcock Centre for Experimental Astrophysics, . Cavendish Laboratory, . ... Cambridge CB3 0HE. Telephone: (+44) (0)1223 337297 . Fax: (+44) (0)1223 337563 . College address: . Emmanuel College, . ... Cambridge. Email name : donald (email to name@mrao.cam.ac.uk) . Cavendish | Astrophysics Home ] . ...

... The Miriad task uvgen can be used to simulate a variety of observing modes. ... Simulating a telescope approximately, let alone in some detail, requires a good many parameters. uvgen takes an appreciable number of parameters and input files to describe the telescope, correlator and source. Fortunately keyword and set-up files for some common situations exist ( e.g. simulating the ATCA and VLA). ... For example, to load typical parameters for the ATCA, use miriad% source $MIRCAT/uvgen.def.atca . ...