... Spectral channels per baseband (16): 32 Number of antennas to be correlated: 5 Polarization (ON): OFF Correlator weighting function (UNIFORM): UNIFORM Distribution tape (DAT): DAT Source positions from: STANDARD Shipping address for correlator output: Steven Tingay Swinburne Hawthorn, Victoria, Australia Correlator Notes: DERIVED INFORMATION FOR CORRELATION: Elapsed time for project: 2.00 hours. Total time in scheduled scans: 2.00 hours. Total time in recording scans: 2.00 hours. ...

... The main periodicity in the Sun 's activity is the 11-year cycle called the solar cycle. ... During the cycle, changes occur in the Sun's internal magnetic field and in the surface disturbance level. ... At the beginning of a cycle the solar magnetic field resembles a dipole which axis is aligned with Sun's rotation axis. ... The sunspot number - and Sun's activity - is at maximum in the middle of a cycle, when the Sun's internal magnetic field is most chaotic. ... Space Physics Text Book of Oulu ...

... From the observed direction of interplanetary magnetic field lines, we believe this field comes from the Sun, carried by magnetic field lines dragged out by the solar wind . ... That is why magnetic field-line loops tend to keep back the solar wind, unlike the outward-bound lines in the "coronal holes" between them. ... The magnetic field at all these points is already so weak that the solar wind overpowers it and shifts its field lines, while its own motion--radially outward--remains unchanged. ...

The pnet, prun, psrv suite of programs . ... pnet -> prun -> psrv -> disc . ... It can forward commands from pnet to psrv and pass back the replies. prun starts the data taking, gets the data from the spectrometer, and passes it via a socket to the psrv program running on the file server. ... There is a psrv task for each prun task (one for each subband on a spectrometer box). prun starts psrv via xinetd by connecting to the well known port address. psrv accepts commands from pnet via prun. ...

Next: Why do Radiopulsars not Up: Ejectors in Massive Binary Previous: The Evolutionary Status of . ... Numerical simulation of the evolution of NS shows (Lipunov and Prokhorov, 1987[ 115 ]) that the fraction of ejecting stars in massive systems with normal components may be as high as several tens of percent of the total number of binary systems (see Figure 27 ). ... Mike E. Prokhorov . ...

The first persistent Web agent that we have created on Actor Prolog is a program that collects information about research groups that develop Prolog and projects in the field of logic programming. The agent looks through a given list of Web sites and calculates some attributes of the sites: the date of recent modification, total size, the number of figures, the number of outside links, the number of error links, the number of given keywords, etc. ... http://www.cplire.ru/Lab144/space/prolog.html . ...

... Content Model: Optional list header (LH), followed by one or more list items (LI) . An ordered list typically is a numbered list of items. ... The numbering style is left to associated style sheets, e.g. whether nested lists contribute to a compound item number, e.g. "3.1.5", or whether numbers are rendered as arabic, upper or lower case roman numerals or using the numbering scheme appropriate to the language context. ... CLASS . ... The CLEAR attribute allows you to move down unconditionally: . ...

Вы находитесь здесь: Каталоги Подключение каталогов к SIMFOV . ... Каталоги для программ-планетариев . ... Для подключения нового каталога, прежде всего, необходимо создать текстовый файл , содержащий по одной строке, на объект, оканчивающейся двухбайтовым символом Enter (если только таковой файл отсутствует). ... В настоящий момент звездная величина в каталогах типа OTHERS программой SIMFOV не используется, но выдавать ее можно из файла *.Dat , включив звездную величину в формат выходной информации. ...

:proposal 12433 :absolute-time 0 :sub-system TRANS :version 20100826 :file-name 12433-03.tv-desc : visit 03 ) ( Visit -Description :number 03 :num-orbits 3 :time 13255 ) ( Orbit -Description :number 1 : visit 03 :visibility 3234 :num-layers 1 ) ( Orbital-Event-Description : orbit 1 : visit 03 : type pcs-acq : sub-type acq : ...

IMPLICIT NONE INTEGER, DIMENSION(1) :: OLD, SEED ! THIS PROGRAM ASSUMES K = 1 INTEGER :: I, K REAL, DIMENSION(3) :: HARVEST SEED(1) = 12345 CALL RANDOM_SEED CALL RANDOM_SEED (SIZE=K) WRITE (*,*) ' Number of integers for starting value = ', K CALL RANDOM_SEED ( GET = OLD (1:K)) WRITE (*,*) ' Old starting value = ', OLD CALL RANDOM _NUMBER( HARVEST ) WRITE (*,*) ' Random numbers : ', HARVEST CALL ...

... In the set of letters below (which you may wish to copy onto a separate sheet far distribution to the class) are hidden a significant number of astronomy related words. ... O P L S C M T M Suggested Scoring: 25 words = Observatory S M A U R E V I Director 21 words = Astrophysics T I B T N Y T Q Professor 15 words = Assistant D E P E O A U P Professor 11 words = Graduate I P R O M R S L Student 9 words = Night J U N I D A T A Assistant Puzzle (c) 1980 Dennis Schatz . ...

Next: The Optopus session Up: Using the Optopus Previous: Using the Optopus . The commands in the Optopus package have to initialised by setting the Optopus context with the MIDAS command SET/CONTEXT OPTOPUS . ... Since almost all commands in the package work, both in input and in output, on MIDAS tables, another important task of the user at the start of an Optopus session will be to create a MIDAS table from the ASCII file where the data about the objects to be observed are being kept. ...

... Here is a sample parameter file that is set to plot the B filter trace data. ... One can generally get by with the default graph parameters. input = B.a list of images or list files to be graphed (wx1 = 3000.) left world x-coord if not autoscaling ... autoscaling (wy2 = 100.) upper world y-coord if not autoscaling (wcs = logical ) Coordinate system for images (axis = 1) axis along which projection is to be taken (transpose = no) transpose the x and y axes of the plot (pointmode = no) ...

SIMPLE = T / file does conform to FITS standard BITPIX = -32 / number of bits per data pixel NAXIS = 2 / number of data axes NAXIS1 = 1138 / length of data axis 1 NAXIS2 = 1114 / length of data axis 2 TELESCOP= 'UT1 ' PI-COI = 'C. Cesarsky' / Name of PI and COI ORIGIN = 'ESO/EIS ' / Data processed by RA = 53.0917713808546 / RA (J2000) at start (deg). ... RADECSYS= 'FK5 ' / Coordinate reference frame. ... TOT-IMAG= 125 / Total number of images. ... MOSTILES= 21 / Total number of tiles in MOSAICID. ...

... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Programs . ... Currently only works on Unix systems. fcgistarter - c command - p port [ - i interface ] - N num . ... FastCGI program . p port . Port which the program will listen on . i interface . Interface which the program will listen on . ... Questions on how to manage the Apache HTTP Server should be directed at either our IRC channel, #httpd, on Freenode, or sent to our mailing lists . ...

... Calculates a "cube helix" colour map for MATLAB. ... Original written in Fortran77 by Dave Green, 2011 Jan 10 % Transcribed to MATLAB by Philip Graff, 2011 Sept 1 %========================================================== function map = CubeHelix( nlev ,start, rots , hue , gamma ) map =zeros( nlev ,3); A=[-0.14861,1.78277;-0.29227,-0.90649;1.97294,0]; for i=1: nlev fract =(i-1)/( nlev -1); angle =2*pi*(start/3+1+ rots * fract ); fract = fract ^ gamma ; amp= ...

Next: Proposed Facility Up: You are the Institute Previous: You are the Institute . Your main research interests lie in the very first stars and galaxies to form. Ever since those chaps at Caltech started finding large numbers of galaxies at redshifts up to about 6, the astronomical world has been in a frenzy of theoretical and observational activity. ... You, therefore, have turned your interest where nobody else has dared look: to really high redshifts. ...

THE RELATIVE MONTHLY MEAN SUNSPOT NUMBER ON AUGUST 2014 HAS MADE Waug.= 74.7, THAT GIVES FOR 60 MONTHS (2014, FEBUARY) DEVELOPMENT CURRENT 24 CYCLES OF SOLAR ACTIVITY THE SMOOTHED MONTHLY MEAN SUNSPOT NUMBER W*feb. ... Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 25 - 31.08.2014, Forecast on 01 - 08.09.2014, Carrington Rotations 2154 (21,46.08.2014) SUNSPOT-FORMING ACTIVITY OF THE SUN WAS AT THE AVERAGE LEVEL. ... FOR THE PERIOD SEVEN EJECTIONS OF THE SOLAR FILAMENT. ...

SIXTH CREW REQUIRED RESOURCES IMAGES VIDEO . ... EXPEDITION SIX (ISS-6) . REQUIRED RESOURCES . During the ISS-6 mission 79 sessions by 28 experiments are intended to be implemented. ... Allocation of Experiments and Number of Sessions by Research Areas. Research Area . ... Totally . ... Problems of Space Power Systems and Propulsions Systems . ... POWER CONSUMPTION . Permanent Power Consumption . Maximum Power Consumption per Session (during 2 hours) . ... 44 h 10 min . ...

Here are all the plug-ins I have written. ... NOTE: Most of these plug-ins have been updated for the developers-only version of the GIMP, release 0.60. ... Until a new official GIMP version is released, the fix is to insert these two lines at the start of gimp.h : #define RGBA_IMAGE 4 #define GRAYA_IMAGE 5 For Texinfo documentation, look at the bottom of this page. ... Updated for GIMP 0.60. ... Quartic suggests that you try this: engrave an image, blur it slightly, and use it as a bump map. ...