... CentralProcessor 0.11 documentation . ChannelAvgTask averages given number of consecutive spectral channels to reduce the spectral resolution of the processed data chunk. ... This section describes the valid parameters. In addition to mandatory parameters which are always required, individual tasks often have specific parameters which need to be defined only if a particular task is used. ... The type of the task defined by tasks. name .type should be set to ChannelAvgTask . Parameter . ...

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• Programme - Abstract
• HIPASS Science meeting
• GEOTRIES

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. ...

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Selected (two) topical problems in solar / stellar modelling Stellar Astrophysics Centre Improving solar physics by studying other stars GЭnter Houdek The effect of the surface layers on the oscillation frequencies Asteroseismic ages and heavy-element abundances of the Sun solar-like stars Courtesy of J. Christensen-Dalsgaard IAU-GA-SP13 ­ Beijing ­ August 2012 Observed solar frequencies m-averaged frequencies from MDI instrument on SOHO Observed ...

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• Mocking the Universe
• Model Fitting
• Contributed Papers

Note: These models for T-receiver are based on measurements for all of the 14 pipelines. download Trx polynomial fit parameters . ... any additional offset to be addded as a correction not incorporated in the model (e.g. the contribution to receiver temperature from beyond the pre-amplifier stages), . ... No. of coefficient pairs, n_harm, associated with the harmonic (Cos & Sin) part of the fit (where the final fit is a simple sum of the two parts).. ... cos(j*pi*X/2) & sin(j*pi*X/2), . ...

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• VLBI at Arecibo Observatory
• Index of /~phil/hardware/vertex/hagenDocmemos/klaus/ATA1A/parameter
• HIPASS parameters Barnes et al (2001), Ryan-Weber et al. (2002), Zwaan et al

Next: cloud Up: Contributed Commands Previous: Contributed Commands . ASTROMETRY/COMPUTE mes option out trail . ... ASTROMETRY/EDIT std plot . Delete/undelete the astrometric standards . ASTROMETRY/POS1 . Interactive procedure for the POS1 astrometry package . ASTROMETRY/TRANS std mes center pla,cat schmidt,blink tol xterm,yterm std . Compute the astrometric transformation parameters of a data . ... Fri Mar 24 17:17:52 MET 1995 ...

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• invent
• Theory

Weaving together Astronomy+Statistics+Computer Science+Engineering+Intrumentation, far beyond the growing borders . ... Archives . ... People . ... To my personal thoughts, the history of astronomy is more interesting than the history of statistics. ... Quintessential Contributions: . ... The contents are only spanned about 100 years and there are great chances that my mind still favors the history of astronomy over the history of statistics. ... Comment ( RSS ) | ... Entries RSS . ... Chandra Blog . ...

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• PAUL J. GREEN - Contributing ConcepTests
• Parameters
• Editing Files and Parameters

... We have observed and studied critical supercurrents, Ic, in cross-type Nb-Cu/Ni-Nb junctions with Josephson layers prepared from diluted ferromagnetic alloys. For suitable values of the exchange energy in the ferromagnet and the F-layer thickness we have observed Ic(T) oscillation with vanishing Ic for the definite values of T and dF. ... Critical supercurrents, Ic, in Nb-Cu(1-x)Ni(x)-Nb Josephson SFS junctions with F-layers prepared from ferromagnetic Cu(1-x)Ni(x) alloys have been studied. ...

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• Yuri A.Ossipyan (1931-2008)

Next: Armagh Observatory New TSN Up: New TSN Action Plan Previous: What We Do Contents . ... The Armagh Observatory seeks to develop this interest by disseminating the results of its scientific research through a programme of public outreach and public understanding of science (PUS). ... partnership with groups and institutions having similar aims and objectives, for example the Astronomical Science Group of Ireland and amateur astronomy organizations; . ...

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• Armagh Observatory
• Sfit Control Language: Classified Listing
• FFIT - Command Syntax

The problem of solar wind data correlation for the observations onboard several spacecraft is very important for three points of view: . ... This problem is studied now in detail by systematic determination of ion flux and ion velocity data correlations by INTERBALL-1 (IKI group), WIND and IMP 8 (both - MIT group). ... Solar wind plasma correlation lengths from IMP 8, WIND and INTERBALL-1. ... Correlation of solar wind observations onboard several spacecraft: INTERBALL-1, IMP 8 and WIND data. ...

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... IONOSPHERIC DATA IN THE INTERACTIVE SPIDR SYSTEM . ... The Ionosphere The ionosphere is that part of the upper atmosphere where free electrons occur in sufficient density to have an appreciable influence on the propagation of radio frequency electromagnetic waves. ... These regions may be further divided into several regularly occurring layers, such as F1 or F2. ... E Region: The region between about 95 and 150km above the Earth that marks the height of the regular daytime E layer. ...

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• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/h' F2
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fb Es
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fo E

Topics covered by the IAU Symp. ... Do all galaxies have stellar halos? ... Stellar tracers of the MW halo and nearby galaxies; the stellar population of star clusters and their contribution to the galaxy halos . ... NEW: Scientific program of the IAU Symposium 317 can be downloaded here . ... GLOBAL PROPERTIES OF STELLAR HALOS FROM THE MILKY WAY TO EXTERNAL GALAXIES . ... DISCRETE CONSTITUENTS OF STELLAR HALOS IN THE MILKY WAY AND IN EXTERNAL GALAXIES : PLANETARY NEBULAE and GLOBULAR CLUSTERS . ...

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• ESO - esaeso-2003
• Preparation of parameter file
• ESO - cosmology2002

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

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• ADASS 2003 Conference Proceedings
• The SRON-HeaD Data Analysis System
• Recent Advances in Parameter Estimation in Astronomy with Poisson-Distributed

... In these pages we have collected contributions by fellow amateurs supernovae hunters. These contributions concern mainly the discoveries they made and their searching activity. ... External link) . The discovery of SN1997bp in NGC 4680 (from TA Magazine, vol34, n.397) - text and images. Visual Supernova Searching With The 40 inch Telescope at Siding Spring Observatory . ... A web page on SN1995G in NGC 1643 (external link to the South Australia Astronomical Society) - text and images. ...

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• Contributions by amateurs: SN1996bk.
• Contributions by amateurs: SN1995G.
• Contributions by amateurs: SN1996ai.

... 8, ``Celestial Mechanics'', 2002 Selenodynamical parameters from analysis of LLR observations of 1970--2001 G. A. Krasinsky Institute of Applied Astronomy, St.Petersburg, Russia LLR observations of 1969--2001 are processsed to estimate a set of parameters of the Earth--Moon system. The dynamical model accounts for effects of elasticity of the lunar body, tidal dissipation in the Moon, and friction coupling between the lunar mantle and its fluid core. ...

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• http://www.ipa.nw.ru/conference/wpltn2012/docs/24/1100%20shargorodsk.pdf
• Table of Minor planet lightcurve parameters
• Parameters of lightcurves of minor planets

Proceedings of the XXVIIth Young European Radio Astronomers Conference (YERAC). ... Please Note: e-mail addresses and external links in these contributions were correct when these papers were written in 1995, but may no longer be valid. ... In addition to the hypertext version of each paper, indicated by the link from the title of the paper, there are links to postscript versions of each paper, which are suitable for printing if you want a hardcopy of a given paper. ... Sandor Frey (or postscript ) . ...

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• Astrophysics Group STFC announces бе119 million contribution to The Square
• Contributing to casata Bojan Nikolic web pages (r. 329)
• Detailed Schedule of IAU 201

One of the prominent scientists of the 20th century Gamow was born in Odessa on March 4, 1904 in the family of a secondary school teacher. ... In 1994, in the year of his 90-th anniversary, an International Conference "Astrophysics and cosmology after Gamow" was held in Odessa and St.Petersburg. The idea of this conference is supported by the UNESCO representation in Russia and by the International Renaissance Foundation (Odessa branch) (affiliation of the Soros Foundation). ...

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• Influence of onboard events onto spin parameters
• AZ Key parameters, 1997
• AZ Key parameters, 1998

... Публикации и издания Публикации профессорско-преподавательского состава СГАУ Издания проф. Сосниной Т.Н. Biosphere: Analysis of Value Parameters . ... Besides, the ways of saving the use value and value properties of biosphere are analyzed. The expediency of transformation of two-criterion theory of value into the three- criterion theory of the balance of value, where the ecologic component performs the function of the key criterion has been founded. ... BIOSPHERE USE VALUE OF THE PRODUCT: MAIN . ...

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Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

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• Where are the tunable parameters of the kernel?
• Kernel tunable parameters
• Tunable Kernel Parameters?

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Here we present the ionospheric parameters variations for quiet conditions. ...

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• East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary
• East Siberian Center for the Earth's Ionosphere Research. Capabilities and
• East Siberian Center for the Earth's Ionosphere Research. Specific character

... Guider functions . ... Guide Sensor Performance . ... Guide Sensor Sky Coverage/ Star Availability . Guide Star Selection Criteria . ... Guide fiber organization and reach at plug plate . ... Plug plate holes for guide stars are identical to those for science FO . ... FOV for each of 9 guide stars is 7.4 arcsec dia. (0.45 mm FO, Sumitomo IGN-05/10) . ... Selected guide stars must have no neighbor stars within TBD (5 arcsec) radius that have a brightness within TBD (5 mag.) of guide stars . ...

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• Telescope Parameters
• what to do with the trace data
• Echelle for Beginners