OptInt PmWiki : Pm Wiki / Other Variables . ... This variable is an array that is used for defining Page Variables . ... To have the page variable $MyVar produce the contents of the internal variable $myvar , many folks try the following which does not work: . ... There are several correct ways to do this, depending on whether you need the value of the $myvar variable as it was at the time the $FmtPV entry was created, or at the time that a particular instance of $MyVar is being rendered on a page. ...

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• OptInt PmWiki : PmWiki / Fmt Page Name
• OptInt PmWiki : Fmt Page Name
• OptInt PmWiki : Other Variables

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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• Processing the "Face on Mars" Images
• Identities
• Kp Index: Classification of Days

... Since summer 2012 it replaces the MIDAS plot engine which was used in trendPlotter before version 3.0. ... Syntax changes from MIDAS to python: . ... Compute and fit rules (identifies by COMPUTE_RULE and FIT_RULE in the config.tp_ files) have to be rewritten into Python syntax. ... Any Python statement that can be written in one line of code can be used to describe the RULES. ... One can also use multi-valued Python lists to simultaneously plot many lines on a trending plot. ... pylab.plot(ax) . ...

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• Sample Identification
• IPACMAN V2.4 Integration Test Plan
• A visual tour

... GCR and SCR are primary cosmic rays. 10-15 years after the discovery of cosmic radiation (1919) there emerged two main avenues of investigation in the physics of cosmic rays (CR): 1) nuclear - elucidation of the origin of elementary particles and nuclear interactions; and 2) astrophysical (space physics) - solution of the problem related to the origin and variations (changes in intensity) of CR. ... Besides, the CR flux in interplanetary space is, strictly speaking, not isotropic. ...

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SUBROUTINE TAP_ERMES ( TEXT, TEXLEN, STATUS ) . Return an error message associated with a TAP status value. SUBROUTINE TAP_ERROR ( TAP_ROUTN, NAME, TEXT, STATUS ) . Report an error message. ... Report an error message associated with a TAP status value. ... Purpose: return an error message associated with a TAP status value. ... TEXT = CHARACTER * ( * ) (Given) TAP error message text. ... Invocation: CALL TAP_REP( NAME, TEXT, STATUS ) Description: An error message is built in the form: !! ...

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• Observations and Data Reduction
• Simon Jeffery's Software Store: TAP: cosmic abundances
• Simon Jeffery's Software Store: TAP global constants

... ON THE ROLE OF LARGE-SCALE PLASMA IRREGULARITIES AT THE FINAL STAGE OF ANOMALOUS ABSOPTION DEVELOPING UNDER HF HEATING OF THE IONOSPHERE . ... Fig. ... With the aid of numerical statistical modeling based on multiple ray tracing it is shown that in presence of large-scale irregularities the reflected signal amplitude mean value is increased significantly. ... Dependence of the mean amplitude of the reflected from the ionosphere signal on the large-scale (10-50 km) electron density irregularity level...

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• Subsystems of the Galactic halo, figures
• RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, figures
• F-stars in galactic disk, figures

... Optical characteristics of amorphous SiO 2 in the region 1400-200 cm -1 . ... Optical constants: . amorphous SiO 2 Some details: . Reflectance of polarized radiation at the incidence angle 12 deg was measured in the range from 1400 to 200 cm -1 for several samples of amorphous SiO 2 . Special technique applied allowed to reduce the relative errors downto 1% for the reflectance values of 0.005-0.8. The optical constants were obtained by the Kramers-Kronig method. ...

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• Rayleigh and Rayleigh-Gans-Stevenson approximations

... These are just the bare bones--just three basic ideas and rules for handling relations ("equations") involving unknown quantities whose values you are trying to find. In most calculations you try to find a number . ... To get a solution, one must replace the given equation (or equations) with others, containing the same information but cleaner in appearance. ... If you have an equation and modify both its sides in exactly the same way, what you get is also a valid equation. ...

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• Formulas
• Events on January 10-11, 1997 - INTERBALL observations
• mcfile

... Make up at least 5 data points, each with an x value, a y value and an uncertainty in the y value. ... Right-click on the top of the column containing the x-data and drag your mouse to the bottom of the column to select it. ... You must first enter the Positive Error Value (the `up error bars') ­ click at top of the column of y error values and drag down to select all of the values (in the above screenshot the y error values are in the column labeled ). ... Let's try fitting a straight line. ...

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• http://www.mso.anu.edu.au/~brian/A3002/Assignment_Carollo.pdf
• http://www.mso.anu.edu.au/~wood/lectures/2007/assignment_2.pdf

... Equinox of object coordinates BJ = 18.87 / bJ magnitude UMBJ = -0.69 / u - bJ colour BJMR = 0.22 / bJ - r colour NOBS = 1 / Number of 2dF observations available IS_ BEST = 'TRUE ' / TRUE if this file contains the best 2dF observa DATEBEST= '24/09/00' / Date of best 2dF observation (DD/MM/YY) ID_ BEST = 'QSO ' / ID from best 2dF observation QUALBEST= 11 / Data quality flag from best 2dF observation Z_ ...

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In the Table below the masses of some asteroids which were determined during the last years are listed. ... The listed values were determined from observations of many test bodies by the weighted least square fit for one perturbing mass and corrections to the orbit elements of all used test bodies. ... based on the observations of 98 asteroids (including 50278) with the values of standard error of mass determination less than 3.0 10 -11 M Sun . ... Mass . ... 3) Mass 121 : 0.74 x 10 -11 M Sun ; . ...

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• (Untitled)
• AY2006 (preface)
• AY2008 (preface)

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/1996/ph199/hw1.html
• Comparing Means and Deviations

... AstroAsciiData is a Python module to handle ASCII tables. ... The idea to develop this Python module emerged from the fact that ASCII tables continue to be one of the most popular and widely used data exchange formats in astronomy and probably science in general. ... To load this ASCII table, go into Python, load the AstroAsciiData module and read in the table with: . ... demo = asciidata.open('webexa.txt') . ... Users who only want to work with ASCII tables neeed no further python modules. ...

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

Below is a Visual Basic sub-procedure which will allow sending the Get RA-Dec command to any model of NexStar. ... Wait 0.25 Comm1.Output = E Wait 1.5 varInputBuffer = Comm1.Input Comm1.PortOpen = False If ScopeType = Little Then RA1 = Asc ( Mid ( varInputBuffer , 2, 1)) RA2 = Asc ( Mid ( varInputBuffer , 3, 1)) Dec1 = Asc ( Mid ( varInputBuffer , 5, 1)) Dec2 = Asc ( Mid ( varInputBuffer , 6, 1)) RA = RA1 * 256 + RA2 RA = RA / 1.011358 / 3 / 15 Dec = Dec1 * 256 + ...

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• http://www.astro.louisville.edu/software/xmtel/archive/xmtel-3.1/docs/nexstar/GotoRA-Dec.txt
• PlotWindow (ImageJ API)
• Toolbar (ImageJ API)

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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. Organisers: Philippe Lebacque (Laboratoire de Math matiques de Besan on ) , Michael Tsfasman (CNRS, Laboratoire Poncelet, Institute for Information Transmission Problems) , Alexey Zykin (Laboratoire Poncelet, State University Higher School of Economics, IITP) . About . General Information . Participants . Program . Practical details . Don Zagier (Bonn) . Wednesday 26 October, 18:00 - 19:00 . Poncelet Laboratory web page .

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• Конференция "Дзета функции"
• Conf rence "Zeta Functions"
• Conference "Zeta Functions"

... On Monday, August 31 SSAU Rector Evgeniy Shakhmatov within the framework of an extended meeting of the Academic Council presented a report on the results of the university activities in the academic year 2014/2015, as well as outlined the prospects for the university development. ... In the academic year 2014/2015 students training in SSAU has been conducted on 67 Bachelor s programs, 45 Specialist s programs, 29 Master's educational programs and 6 fields of secondary vocational education. ...

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• Summer School on engine building took place in SSAU
• Summer School of Innovation Management took place in SSAU
• A meeting of SSAU Supervisory Board took place

... Comments, Opinions Publications Dnepr Program . Dnepr launch record 17 August 2011. Cluster Launch of Dnepr LV 22 August 2013 KOMPSAT-5 Launch 21 November 2013. Dnepr Cluster Mission 2013 19 June 2014. ... ISC Kosmotras announces signing of a launch contract with T B?TAK Space Technologies Research Institute (T B?TAK UZAY) for injection of RASAT spacecraft - the first Earth observation satellite designed and manufactured in Turkey by Dnepr LV in 2010. ... Dnepr LV Performance . ...

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• The national Earth remote sensing spacecraft of Ukraine will be placed into

... Subject and Problems of Stellar Astronomy. ... Plane of Galaxy, Methods of Its Location Determination. ... Stars Distances. ... Other Methods of Stars Distances Determination. ... Tangential Velocities, Their Determination by Self-Motions. ... Determination of Solar Apex and Spatial Velocity by Radial and Spatial Velocities of Stars. ... Features of Orientation and Parameters of Peculiar Stellar Velocities Ellipsoid. ... General and Selective Light Absorption in Galaxy. ... Darc Clouds in Galaxy. ...

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• Celestial Mechanics
• General Astrometry
• Second order reduction quantities. Explanations for Computer Ephemeris.