... Астронет | ... планета Астронет | ... Астрономия в России | ... История астрономии . ... Любительская астрономия . ... Кривая блеска GRB 030329 . ... Includes most data through GCN 2276 . Light curve of posted GCN observations of GRB030329, including AAVSO observations, by Melissa Nysewander (UNC-Chapel Hill) . ... Публикации с ключевыми словами: гамма-всплески - оптические ореолы гамма-всплесков . ... Самый далекий, самый желанный . GRB 090423: самый далекий взрыв . ...

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• Astronet > Sky Map, professional edition
• Астронет > К 90-летию Лео Голдберга

... Once the program has run successfully, there should be two output files: 1) rk.dat 2) exact.dat The solution to the numerical Runge-Kutta routine is in 'rk.dat', whereas the exact, analytical solution to the 2nd order ODE is in 'exact.dat'. ... To plot your results, you can use a program called gnuplot. ... From the command line type > plot "exact.dat" using ($1):($2) a window should pop up with a plot of x versus y. Note that you plotted column 1 on the x-axis versus column 2 on the y-axis. ...

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• http://www.mso.anu.edu.au/pfrancis/labskills/datahandling/UsingExcel.pdf
• http://www.mso.anu.edu.au/~brian/A3002/Assignment_Carollo.pdf
• http://www.mso.anu.edu.au/pfrancis/labskills/datahandling/python_reference.pdf

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

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• HSTPOLIMA (V1.00) --- April99 --- HSTPOLIMA (V1.00)
• POLIMPLOT (V1.00) --- April99 --- POLIMPLOT (V1.00)
• HSTPOLSIM (V1.00) --- April99 --- HSTPOLSIM (V1.00)

Organisers: Michel Balazard (CNRS, Laboratoire Poncelet) , Michael Tsfasman (CNRS, Laboratoire Poncelet, Institute for Information Transmission Problems) , Alexey Zykin (Laboratoire Poncelet, State University Higher School of Economics) . ... General Information . ... By comparing several restrictions of Siegel-Eisenstein series of degree 3, B.Heim recently found a remarkable (and somewhat mysterious) formula relating central values of triple L-functions to other critical values. ...

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• Конференция "Дзета функции"
• Conf rence "Zeta Functions"
• Programming: from an Art to a Science

THE RELATIVE MONTHLY MEAN SUNSPOT NUMBER ON OCTOBER 2015 HAS MADE Woct. = 37.1 (old), 61.7 (new) THAT GIVES FOR 75 MONTHS (2015, APRIL) DEVELOPMENT CURRENT 24 CYCLE OF SOLAR ACTIVITY THE SMOOTHED MONTHLY MEAN SUNSPOT NUMBER W*apr. = 50.0 - old; 61.7 - new; W*march = 49.3 - old; 82.7 - new; - On July 1, 2015 Centre in Brussels moved to a new system of cal- culation the relative number of sunspots and practically all of the values were replaced throughout the numbered series of Wolf numbers (see link). ...

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• http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20150704.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2016/obzor20160307.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2016/obzor20160208.en.txt

The most up-to-date information related to atmos 3.0 are collected here due to constantly increasing interest to MASS/DIMM processing software... atmos 3.0 is still beta , so the latest version is 2.97.5 (there is also 2.98.x branch which absorbs new features) . ... M' line: . ... free seeing and its relative error . ... dimm seeing and its relative error (if dimm data are present, zeros otherwise) . ... dimm turbulence power and its relative error (if dimm data are present, zeros otherwise) . ...

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• http://zebu.uoregon.edu/1998/es202/ptable.html
• http://zebu.uoregon.edu/~uochep/talks/talks01/SM01_Ecal.pdf
• http://zebu.uoregon.edu/1998/es202/dispersion.html

... a file that contains codes which are not part of the ASCII character set . ... Recipients cannot see who else has received the message: hence the term "blind". this term derives from `bootstrap loader', a short program that was read in from cards or paper tape, or toggled in from the front panel switches. ... a temporary area of memory which data can be read from and written to. a unit of memory or data consisting of 8 bits which is used to represent one character. ...

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• Fill-Out Forms
• Displaying vi option values
• Mail program files

Download Izmccd (~2.7 MB). ... for 1-5 bytes is number of a numbered minor planet, . ... Positions 1-80 file "mpcreportiz.txt" are similar to positions of file "mpcreport.txt". 83-95 – errors of unit weight, . ... If this tag is " 1 0 " , this record contains results of measurements of an image of object (approximation by "PSF"),  . ... 57-66 – error in X (pixels), for first star in a multicentric image, for subsequent it is error in (distance between first star in the image and this), . ...

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... The particular variables it is concerned with are tick , which is the number of microseconds added to the system time during a clock interrupt, tickadj , which sets the slew rate and resolution used by the adjtime system call, and dosynctodr , which indicates to the kernels on some machines whether they should internally adjust the system clock to keep it in line with time-of-day clock or not. ... Set the kernel variable tickadj to an internally computed "optimal" value. -t tick . ...

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• FTS Dictionary Example
• ntpdate - set the date and time via NTP
• Lighting plug-in

DIGITAL WDC EXCHANGE FORMAT . FOR OBSERVATORY 1.0 MINUTE VALUES 1. ... DATA-1 .. DATA-60 are 1-minute values of the given element for that hour. ... Typically, digital 1-minute values received by WDCs from organizations operating automatic magnetic observatory instruments are averages of more frequendy sampled values, e.g. 10-second point samples. ... If the method used to obtain 1-minute average values is important to a user, the WDC will assist in determining the exact procedure applied. ...

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• Kp Index: Classification of Days
• Processing the "Face on Mars" Images
• Geomagnetic Indices Kp, ap, Ap, Cp and C9

ON-LINE STATIC EIT RECONSTRUCTION SERVER . ... Static image reconstruction from the data measured in vivo is still intriguing problem in EIT. ... dipole (adjacent) current injection and voltage measurements on pairs of adjacent electrodes (like in Sheffield systems) . ... You can view examples of the text files for polar , dipole and trigonometric injection, use them for testing the server and find more details on HOW TO PREPARE INPUT FILE FOR THE ON-LINE EIT RECONSTRUCTION SERVER page. ...

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• Getting Started in Actor Prolog. 3D Web Site.
• EIT Server Input File Format
• Getting Started in Actor Prolog. Underdetermined Sets.

First, we'll set up values for Mail :: Bulkmail # #################### define package Mail :: Bulkmail # server _class stores the server object that we're going to use. #uncomment the DummyServer line and comment out the Server line for debugging server _class = Mail :: Bulkmail :: Server # server _class = Mail :: Bulkmail :: DummyServer #log our errors ERRFILE = / Mail::Bulkmail might as well use it. ...

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• INTEGRAL 9-year Galactic Survey

... FIELD | ... public class Menus . ... ImageJ . ... static char . ... static int . ... Returns the size (in points) used for the fonts in ImageJ menus. static java.lang.String . ... Returns a list of the plugins in the plugins menu. static java.lang.String . ... Field Detail public static final char PLUGINS_MENU . ... public static final char IMPORT_MENU . ... public static int installPlugin (java.lang.String plugin, char menuCode, java.lang.String command, java.lang.String shortcut, ImageJ ij) . ...

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• FileInfo (ImageJ API)
• Measurements (ImageJ API)
• CurveFitter (ImageJ API)

... Appropriate values of DIT the integration time (DIT secs) for each individual integration, are lmited by various considerations. N.B. Ndit individual Integration s each of DIT secs are coadded to form a single Exposure of time Ndit*DIT]. The recommended minimum DIT is one sec (the minimum possible exposure time) or the value at which the noise becomes sky (rather than detector) limited. ... The recommended maximum DIT is such as to keep the detector wells less than half full. ... 40 sec . ...

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spectrum1d - compute auto- [and cross- ] spectra from one [or two] timeseries. spectrum1d [ x [ y ] file ] -S segment _ size ] [ -C ] [ -D dt ] [ -N name _ stem ] [ -V ] [ -W ] [ -bi [ s ][ n ] ] [ -bo [ s ] ] spectrum1d reads X [and Y] values from the first [and second] columns on standard input [or x [ y ] file ]. ... Units same as ypower. name _ stem .npower Power spectral density of the noise output. Units same as ypower. name _ stem .gain Gain spectrum, or modulus of the transfer function. ...

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• B light curve (Shugarov, 1976)
• Dependence on the Scenario Parameters and Initial Distributions
• Notes on Monte-Carlo Simulations

... arXiv.org . astro-ph . ... Query was: SELECT last_value FROM authors_id_seq;' in /home/karpov/postgres/arxiv/arxiv.php:30 Stack trace: #0 /home/karpov/postgres/arxiv/arxiv.php(39): Arxiv->query('SELECT last_val...') #1 /home/karpov/postgres/arxiv/request.php(509): Arxiv->singleQuery('SELECT last_val...') #2 /home/karpov/postgres/arxiv/index.php(107): handleStatsQuery() #3 {main} thrown in /home/karpov/postgres/arxiv/arxiv.php on line 30 . ...

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... The less then 5 degree value of the relative geocentric angular distance between the footprints of the SC is used as a criterion of the magnetic conjugation. ... On the last column of the file is shown the magnetic field model version ( MOD IOPT ) used during magnetic mapping. ... The difference between CMLT values of the Sat.1 and Sat.2 (see as well column 11) . ... dcorlat = dla (deg) . The difference between CORLAT values of the Sat.1 and Sat.2 (see as well column 12) . ... AnD (deg) . ...

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• The INTERBALL Tail PROBE orbital elements
• The INTERBALL Auroral PROBE orbital elements
• Elements of Algebra

. Distance Conversion Calculator . by Matt Oltersdorf 2000 04 02 2225 UTC . Type the known value into the appropriate units field, click the . calculate button and the program will show all values for . related unit properties. Kilometers . Meters . mm . Inches . Feet . Yards . Miles . Astronomical Units (A.U.) . Light Year (LY) . Parsec (pc) . Kilometers . Miles .

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Subject of Celestial Mechanics. ... Differential Absolute Coordinates Equations of the Problem. ... General Integral of Non-Perturbed Motion. ... General Equation of Non-Perturbed Orbit. ... Other Integration Methods of Non-Perturbed Motion Differential Equations; Bine Equation for Case of Non-Perturbed Motion. ... Ellipsical Motion, Kepler Equation. ... Motion Differential Equations in Absolute Coordinates. ... Equation of System of Bodies Motion in Barycentric Coordinates, in Relative Coordinates. ...

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• General Astrometry
• Stellar Astronomy
• Practical Astrophysics