... July , 2007 . ... 0.12 0.23 +/- 0.10 +/- 0.06 Internal error of single observation 0.18 0.11 ----------------------Compressed Ephemeris DE200/LE200 -------------- MP Obs Dynamical Time RA (O-C)cosDEC DEC (O-C) h m s " ' " " 78756 094 2007 7 22.891513 20 04 27.767 -0.12 - 9 55 57.80 0.32 78756 094 2007 7 22.899703 20 04 27.348 -0.34 - 9 55 58.00 0.30 78756 094 2007 7 22.907823 20 04 26.959 -0.18 - 9 55 58.20 0.28 78756 094 2007 7 22.914753 20 04 26.618 -0.17 - 9 55 58.30 0.33 Mean of last 4 obs. ...

... Amorphous carbonaceous materials can show a great diversity of optical properties due to the variability in their microstructure. ... The differently pyrolized celluloses are representative for a suit of carbonaceous material ranging from strongly disordered (insulating) to graphitized (conducting) material. Figure: Complex refractive index of hydrogenated amorphous carbon prepared by pyrolysis (annealing) of cellulose at different temperatures. ...

... FILE LIST 1) Collisonal Ionisation Equilibrium cooling functions as a function of metallicity are given in the files: mzero.cie : cie cooling for primordial hydrogen/helium mix log (T) = 4-8.5 m-00.cie : cie cooling for solar abundances mix log (T) = 4-8.5 m-05.cie : [Fe/H] = -0.5, solar /primordial average ratios m-10.cie : [Fe/H] = -1.0, primordial ratios (ie enhanced oxygen) m-15.cie : [Fe/H] = -1.5, primordial ...

N. A. Vavilov Department of Mathematics and Mechanics, State University of Saint-Petersburg St. Petersburg, Russia nikolai-vavilov@yandex.ru Calculations in exceptional groups Let be a reduced irreducible root system, R be a commutative ring with 1. ... The Steinberg group St(, R). ... 2] R. Hazrat, N. Vavilov, K1 of Cheval ley groups are nilpotent, J. Pure Appl. ... 6] N. Vavilov, An A3 -proof of structure theorems for Cheval ley groups of types E6 and E7 , Int. J. Algebra Comput. 17 (2007), no. ...

. The frequency of the spectral maximum f m of the gyrosynchrotron emission vs. the power-law index of the electron spectrum calculated according to Dulk & Marsh (1982). Curves are shown for various column densities LNe of accelerated electrons and magnetic field strengths B . The angle between the line of sight and the magnetic field is 45 degree.

function [EpochMin, Period , Scatter ]=FourierPeriodogram(fname,order,N1st,Pmin,Pmax, delta , epoch ); % % ------------------------------------------------------------------------- % Program calculates Fourier power spectrum of the time series % % Program call: % [EpochMin, Period , Scatter ]=FourierPeriodogram(fname,order,N1st,Pmin,Pmax, delta , epoch ) % or % FourierPeriodogram(fname,order,N1st,Pmin,Pmax, delta , ...

As it is in Ephemerides task, O–C can be calculated with different accuracy. ... It presents three modes of accuracy. One can calculate position of a minor planet by the formulae of elliptic motion starting from the fundamental set of elements for given minor planet. ... Also there is possibility to calculate positions taking into account perturbations from different sets of perturbing bodies by numerical integration ( Integration mode). ... Accuracy of integration is equal to 10**(–10) AU. ...

Computer Ephemeris. Second order reduction quantities. Explanations. This page consist of four little tables. First and second tables contains J a (in 0.000001 s ) and J d (0.0001") for nothern declination, third and fourth contains the same information but for southern declination. Each table have 13 informational columns headed with right ascension values, and some amount of rows, labelled with date. ...

... The first column has the name of the qualifier. ... name of AB (inherited from first raw file, with grouping tag read from <instr>_organisation.h) . ... root name of products (inherited from first raw file and grouping tag read from <instr>_organisation.h) . ... name and value of non-default parameter(s) required to execute the recipe (set by createAB; read from <instr>_association.h) . ... name of waitfor(s) for this AB (relevant for DRS=CON only; set by createAB; read from <instr>_association.h) ....

. OND model values divided by measured values for NOx. Yearly average for each station. (Zero columns named 'Meteo' are accessories to calculation - don't pay attention to them.) . Отношение расчетных значений по модели ОНД к измеренным значениям для NOx. Годовое среднее для каждой станции. (Нулевые столбцы - метеорология - в вычислениях не участуют.)

King 13 2.5700 +61.1775 10.0 0.56 0.04 12.36 0.27 2960 400 8.85 0.05 NGC 136 7.8858 +61.5083 4.0 0.70 0.09 13.59 0.14 5220 350 8.40 0.05 Berkeley 19 81.0117 +29.5711 5.0 0.61 0.05 0.72 12.38 0.40 3000 600 9.25 0.05 Czernik 21 81.6708 +36.0136 6.0 0.72 0.02 0.56 11.82 0.20 2300 200 9.55 0.05 Stock 8 82.0367 +34.4314 8.0 1.21 0.04 0.57 9.84 0.20 900 110 7.50 Kronberger 1 82.0917 +34.7733 5.0 0.43 ...

0.3 =0.11 s=0.03 s/y = 0.7 0.25 matrix model tracking 0.2 0.15 +s 0.1 -s 0.05 0 0 Coherent synchro-betatron mode tunes vs. the beam-beam parameter . Comparison of matrix calculation and tracking with Gaussian distribution in the synchrotron phase space. 0.02 0.04 0.06 0.08 0.1 0.12

... The extinction in terrestrial atmosphere. ... A star was observed at different zenith distances during one night at the Engelgardt's Astronomical Observatory in the program of atmospheric extinction study at blue. ... Calculate the air mass for given zenith distances in 1st 54.9 11800 column, and write the result into the 2nd column. ... Spectral observations. ... Calculate the radial velocity Vr of the star on each date, the results of measurements and write calculations into the table. ...

... Meade Instruments Corporation . ... How to Calculate Power . How to Calculate Power: The magnification, or power, at which a telescope is operating is a function of the focal length of the telescope's main (objective) lens (or primary mirror) and the focal length of the eyepiece employed. ... Example: The Meade DS-2070AT telescope has an objective lens focal length of 700mm; when this telescope is used with a 25mm eyepiece, a power of 700/25 = 28 power (written as "28x") results. ... about meade | ...

Blackholes Forum Message . ... So How Can We Calculate The Mass Of The BH? ... Posted by Lukas on January 25, 2005 14:00:31 UTC . ... Gravity is the weakest force of all - secretary - January 25, 2005 - 18:53 UTC . Singularity - bazukaz - January 25, 2005 - 23:19 UTC . Only in theory - secretary - January 26, 2005 - 02:15 UTC . ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

... Classes . ... gTime Class Reference . This class implements time calculations. ... gTime (double ai_jDays=0) . ... gTime (const gTime &timeSrc) . ... Set the time value of the time object to the julian day of year, day. ... operator= (const gTime &timeSrc) . ... Returns the time GMT value in Julian days. ... Returns the time_t value of the gTime Object. ... Returns a gTime object setted with the actual machine time. ... gTime Object assigned with real machine time. double gTime::getGmtTm . ...

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The algorithm and appropriate program for decametric radiosignal propagation conditions prediction for paths from 500 to 9000 km have been developed at ISTP SB on the basis of normal wave method (AltyntsevaB.I,Iliyin N.V., Kurkin V.I. and others //Decameters channel simulation on the base of normal wave method . ... Solar activity indices are chosen automatically from the prediction date from the database . ...

sw@newmail.ru THE PROBE LAYER METHOD IN THE CALCULATIONS OF CONTRIBUTION AND RESPONSE FUNCTIONS S.G.Mozharovsky Ussuriysk Astrophysical Observatory of FEB RAS, Ussuriysk, Russia sw@newmail.ru The method of probe layer for the calculation of response and contribution functions is discussed. ... This allows us to turn from the response functions to the contribution functions calculated with help of the probe layer (CFPL). ... V- VMAX . ... Solar Phys., v.136, p.239-250. ... Solar Phys., v.35, p.11-29. ...

MATSYM - symbolic matrix processor . ... To use the program you will need a MAT file (liked CIR file: "User manual for CIRSYM program") of your system. ... In first string of MAT file enter any text you want to be the title of your system. ... Starting from string 2 (if is not comments - "*") enter the system element name, incident row and column and, optionally, its value. ... To generate a solution, run MATSYM.exe and enter "system_file_name.CIR" or click on the "ENTER" (in "MAT" case). ...

... The SDSS 2.5-m primary mirror is supported in a manner similar to the Apache Point Observatory 3.5-m telescope primary. ... The axial support is provided by 48 air pistons. The pistons have the same diameter thereby applying equal forces with the same air pressure. ... Each group supports a 120њ sector of the mirror. ... Figure 1: CAD drawing showing the 2.5-m primary mirror and the locations of actuators (green circles) These actuators apply forces (10*cos2 N) to correct astigmatism. ...