... Meta Index / Home Page This section documents the parameters recognized by this task (if any). Parameter . ... Constraints . ... in equation 1 must exceed this value for a source to pass. mindetml . ... For a source to pass, ii_DET_ML must be mindetml and ii_MASKFRAC must be minmaskfrac for at least one of the instruments ii. minmaskfrac . ... For a source to pass, ii_DET_ML must be mindetml and ii_MASKFRAC must be minmaskfrac for at least one of the instruments ii. numhexchar . ... 3.5 1.0 1.0 . ...

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• Description
• Diagnostic mode

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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• Arecibo Observatory L-Wide Band Receiver
• VLBI at Arecibo Observatory

... 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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• Department of Solid State Physics MIPT

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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• Herschel Images and Results for the Magellanic Clouds
• Model Fitting
• Contributed Papers

... 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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I'm glad you're interested in collaborating on the ConcepTests for Astronomy WWW database project! ... I'm looking forward to your contributions! ... a) high luminosity, high temperature to low luminosity, low temperature . b) high luminosity, low temperature to low luminosity, low temperature . c) high luminosity, low temperature to low luminosity, high temperature . d) high luminosity, high temperature to low luminosity high temperature. ... Back to Paul Green's Peer Instruction page. ...

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• Model Spectra for Spectral-Fitting Program
• Cosmological parameters constraints
• The AstroStat Slog Blog Archive Quintessential Contributions

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
• BTA meteo parameters: temperature for the last day
• BTA meteo parameters: temperature for the last week

... 172 ] Briefly, the count rate at the detector from a source at a redshift z is . ... Figure 55 shows the ``Green functions'' for the double compact binary merging rate   evolution assuming no collapse anisotropy. ... Another way that diverse peculiarities in the - distribution induced by the sources evolution could arise is connected with a possible non-monotonic character of the star formation rate in galaxies. ... 22 ] Figure  56 shows two-dimensional cuts through the parameter space. ...

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• The Effect of Relativistic Wind on Accretion Flow Parameters
• The Gravimagnetic Parameter
• Initial Distributions of Binary Parameters

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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• POLIMPLOT (V1.00) --- April99 --- POLIMPLOT (V1.00)
• Space Telescope-European Coordinating Facility

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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• Colours and magnitudes
• IAU Symp317 Scientific Program
• Preparation of parameter file

... astro-ph . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . ... Quasar Variability in the Framework of Poissonian Models . ... It is shown that in this very general framework the well established anti-correlation between variability amplitude and wavelength can only be understood as an effect of an underlying spectral component which remains stable on long time-scales, and is redder than the variable component. ...

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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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... 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
• Parameters of lightcurves of minor planets
• Table of Minor planet lightcurve parameters

Gravitational wave contribution to CMBR anisotropy V.N. Lukash 1 and E.V. Mikheeva 2 Astro Space Center of P.N.Lebedev Physical Institute 3 , Profsoyuznaya 84/32, Moscow 117810, Russia We argue that the contribution of cosmic gravitational waves into the large­scale CMBR anisotropy can exceed 50% for a broad class of the inflationary models with effective \Lambda­term producing the standard local spectrum of primordial cosmological perturbations. ... 10 7 k hor (Figure 2). ...

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• Detailed Schedule of IAU 201
• XXVIIth YERAC Contributions
• Astrophysics Group STFC announces бе119 million contribution to The Square

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

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?

Visual Discovery of SN 1996X in NGC 5061. ... It was not until the IAU Circular was issued that we found out there had been an independent amateur photographic discovery of this supernova by Kesao Takamizawa of Japan. ... Earlier in the week, 660 galaxies had been observed during two nights we had use of the 40 inch telescope at Siding Spring. ... The supernova in NGC 5061 was first seen with the smaller telescope about 10pm local time on Friday, April 12 (April 12.5 UT). ...

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• Contributions
• Contributions by amateurs: SN1996bk.
• Contributions by amateurs: SN1995V.

... Agababaev V. СПбГУ . ... Altaisky M.V. ИКИ & ОИЯИ . ... Dark matter and generation of galactic magnetic fields . Borisevich T.P. ГАО РАН . ... Gladyshev A.V. ОИЯИ . ... Gnedin Yu.N. ГАО РАН . ... Ikhsanov N.R. ГАО РАН . ... Ivanchik A.V. ФТИ им. А.Ф. Иоффе . ... Jordan J.E. Max Planck Institut for nuclear physics (Heidelberg, Germany) . ... Karshenboim S.G. ГАО РАН & MPQ (Garching, Germany) . ... Koriukin V.M. Марийский ГУ . ... Mostepanenko V.M. ГАО РАН . ... Stepanov A.V. ГАО РАН . ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/heinkelmann_swg3.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm03d.pdf

Ionospheric Data 2. Ionospheric Digital Database - 2 discs. The Ionospheric Digital Database compact discs contain approximately 40,000 station years (1.35 gigabytes) of scaled digital vertical incidence parameters from about 130 sites around the world for the period from 1957 through 1990.These data have been contributed through a major cooperative effort among the World Data Centers and many ionosonde network organizations. ...

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• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/f min
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/M3000
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fo Es