Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

Еще в разделе: (Показать все результаты (>534) - xray.sai.msu.ru/ )

• Initial binary parameters
• Initial parameters of compact stars
• Restrictions on the Scenario Parameters

... Meta Index / Home Page This section documents the parameters recognized by this task (if any). ... string . ... yes|no . Yes' forces overwrite of colimchain output. astest . ... Yes' invokes asmooth to smooth the input images before they are supplied to colimplot . ... The maximum allowed value of the width of the smoothing gaussian is specified via this parameter. desiredsnr . ... The maximum desired signal-to-noise ratio of the output image can be specified via this parameter. nconvolvers . ...

Еще в разделе: (Показать все результаты (>14636) - xmm.vilspa.esa.es/ )

Next: HST Paper Products: A New Way to Look at HST Data . ... After providing on-the-fly re-calibration of HST data to archive users, ST-ECF has embarked on a new project aiming at grouping, cosmic ray cleaning and drizzling images taken by most HST instruments. ... The production of the missing jitter files combined with the extraction of additional engineering parameters will greatly enhance the homogeneity and the scientific value of the entire archive. ... 1995, HST Data Handbook, STScI, 107 . ...

Еще в разделе: (Показать все результаты (>1604) - www.adass.org/ )

• ETCs and Observations Simulation at the VLT
• Modern CCD Observations of Moving Celestial Objects: Algorithms and Software
• VLT Data Quality Control

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 . ...

Еще в разделе: (Показать все результаты (>8317) - www.arcetri.astro.it/ )

• Determination of the Detector Parameters
• Program use
• Where are the tunable parameters of the kernel?

... Correcting ETC Calculations of CCD Spectral Observations for CTE Effects . ... HST Overview . Overview . ... Post-Observation . ... ETC . ... ID: CL Script for Applying CTE Loss to Output of Spectroscopic ETC . ... However, the STIS ETC calculations do not incorporate these CTE effects as yet. ... The output from this script should then be used to calculate the appropriate input flux level for a second run of the ETC, which will then yield output which is corrected for the CTE effect. ...

Еще в разделе: (Показать все результаты (>18215) - www.stsci.edu/ )

• Obsolescent Acquisition Parameters
• FOCSIM Parameters Fill-out Form
• STIS PSF Library Input Tool...Help

... Other Characteristics of the Sun: Variability of Rotation, Magnetism, Chemical Structure, Planetary System. ... Methods of Solar Magnetic Fields Measuring: Visual, Photografic, Photoelectric. ... Empiric Datas of Magnetic Fields in Photosphere, Chromosphere and Corona. ... Characteristics of Magnetic Field in Balanced Force Tubes by Potential and Forceless Field. ... Phenomenons in Active Region (Magnetic Field, Spots, Torches, Solar Prominences, Flares, Discharges. ... Magnetic Fields in Flares. ...

Еще в разделе: (Показать все результаты (>122) - space.univ.kiev.ua/ )

• Theoretical Astrophysics
• Optical static Fourier spectrometer
• Sun orbital parameters for Computer Ephemeris for 2014 (DE200/LE200).

Geomagnetic storms and substorms are a natural hazard similar to hurricanes, floods etc. ... Solar and geomagnetic activity also probably influences the Earth's climate and human health. ... Under southward directed IMF the Earth's magnetosphere is open to input from the solar wind flow. ... Since practical importance of solar wind measurements was recognized, a number of approaches was developed for prediction of the geomagnetic activity basing on the solar wind data. ...

Еще в разделе: (Показать все результаты (>1759) - www.cosmos.ru/ )

• Multipoint correlations of the solar wind parameters observed by several
• Space Research Institute (IKI) Seminar
• Magnetic mapping

... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...

Еще в разделе: (Показать все результаты (>373) - www.gao.spb.ru/ )

• http://www.gao.spb.ru/english/as/j2014/presentations/tsyba.pdf
• Pulkovo NEO Page: Ephemeris Support
• Pulkovo NEO Page: Observations

... CentralProcessor 0.11 documentation . ... These parameters govern all processing used for the calibrator observation. ... The dynamic flagging step can also optionally include antenna or baseline flagging. Then the bandpass table is calculated with cbpcalibrator , which requires MSs for all beams to be given. ... Second amplitude threshold applied when flagging 1934 data [hardware units - before calibration] . ... Name of the CASA table used for the bandpass calibration parameters. ...

Еще в разделе: (Показать все результаты (>13520) - www.atnf.csiro.au/ )

• User Parameters - Preparation of the Science field data CentralProcessor 0.11
• Parameters Specific to the VLA
• User Parameters - Pipeline & job control CentralProcessor 0.11 documentation

... 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 . ...

Еще в разделе: (Показать все результаты (>582) - www.ssau.ru/ )

... Column 1 gives the object name from the Case or Markarian catalogs. ... For Markarian galaxies the errors of coordinates usually lie inside 2'' (Lipovetsky [ 1983 ]). Column 4 gives the eye-estimated apparent blue magnitudes according to the same sources. ... Other names of a galaxy we give in column 7. ... In column 3 we cite the original emission-line code of the galaxy for the strength of [O III ] doublet according to the Case catalog (s - strong, m - medium, w - weak). ...

Еще в разделе: (Показать все результаты (>1748) - www.sao.ru/ )

• LEDA documentation: homogenisation
• Parameter estimation
• Results of observations

Next: System configuration Up: How to use CONSTRICTOR Previous: Preparation of parameter file Contents . ... DayNumber: Even though this number is in the data, some packet headers have the wrong number and it makes it a whole lot easier to have the user check and enter this number correctly. ... CONSTRICTOR will add a multiple of 24 hours to the time tag when the day number changes. Remember to set the StopTime to, say, 48 hours if you use a DayNumber of one less than the actual day number. ...

Еще в разделе: (Показать все результаты (>66621) - www.eso.org/ )

• AstroRaikoh
• The Brightness of the Night Sky
• Preparation of parameter file

... Minute Values of Geomagnetic Field Components . ... AA 1868 - Present (3 hourly and daily) (monthly) (yearly) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) KP_AP 1932 - Present (3 hourly and daily) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) AE_HV 1957-75, 78-88 (hourly) AE_MIN 1978-881-6;198903;1990-94 (minute) DST 1957 - Present (hourly) PC 1975 - Present (15-minute) AMANAS 1959 - Present (3 hourly and daily) KMKNKS 1983 - Present (3 hourly) . ...

Еще в разделе: (Показать все результаты (>344) - www.wdcb.ru/ )

• 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
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fo E

... Main page . ... Parameters . ... Modes: . ... Long-slit . ... Back to SAO web page . ... This page is designed by A.V. Moiseev . ... The SCORPIO-2 project: . Spectral Camera with Optical Reducer for Photometric and Interferometric Observations - 2 . The SCORPIO-2 main parameters . ... Spectral range . ... Spectral resolution . R=500-4000 in long-slit mode . R=4000-15000 in scanning FPI mode . The CCD detector . ... The quantum efficiency measurements for CCD detector ...

Еще в разделе: (Показать все результаты (>1051) - jet.sao.ru/ )

• harak_e
• SCORPIO-2 project: filters
• Parameters of the 41 Dra system components

... V.N. Obridko . ... Solar cycle . Coronal holes . ... webmaster@izmiran.ru . ... Solar Physics 124: 73-80, 1989. ... Solar Physics 176: 107-121, 1997. ... I.M. Chertok, Hudson H.S., Mogilevsky E.I., Obridko V.N., Shilova N.S. Solar disappearing filament inside a coronal hole and associated large-scale activity . ... Contrast of coronal holes and parameters of associated solar wind streams . ... Relationship between the Contrast of Coronal Holes and Parameters of the Solar Wind Streams . ...

Еще в разделе: (Показать все результаты (>777) - www.izmiran.rssi.ru/ )

• Magnetic Flux of EUV Arcades and Dimmings
• Ilya M
• Dependence of Forbush-decrease c

EPM-ERA2012 Lunar Ephemeris and selenodynamical parameters from LLR data(1970-2012) M.V. Vasilyev, E.I.Yagudina IAA RAS, St-Petersburg, Russia Reflector at the Moon The reflector 's positions at the Moon surface 3.5 m telescope at Apache station INTRODUCTION MODERN EPHEMERIDES: 1. ... IAA RAS, Russia-EPM-ERA2012 The present analysis of (17580) LLR observations, (time interval 1970, March - 2012, February) Model ( brief description). The dynamical model EPM-ERA has been developed by G.A. Krasinsky. ...

Еще в разделе: (Показать все результаты (>640) - www.ipa.nw.ru/ )

• Intl collabration
• Keywords_174
• Keywords_262

... The Search of a pulsar Once the dedispersed time series is obtained, a Fourier transformation is performed. ... 2 Binary parameters The orbit of a pulsar , as well as any object, in a binary system is determined in its geometrical characteristics, space displacement and syncronised in time by the following parameters : Semimajor axis Eccentricity Longitude of periastron Binary period Time of ascending node a e PB T0 True spin period and observed spin period The ...

Еще в разделе: (Показать все результаты (>5154) - www.naic.edu/ )

• WAPP File Format Page
• The Mock Spectrometer
• Orbits in the period / acceleration plane

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... The interface between the lower solar atmosphere where energy is generated by subsurface convection and the corona comprises the chromosphere, which is dominated by jet-like, dynamic structures, called mottles when found in quiet regions, fibrils when found in active regions and spicules when observed at the solar limb. ... In addition, how they affect the coronal heating and solar wind need to be further explored. ...

Еще в разделе: (Показать все результаты (>2587) - star.arm.ac.uk/ )

• FFIT - Command Syntax
• sfit help file
• Refereed Journal Publications 2004

... Our scientific interest is an accuracy of asteroid CCD observations obtained by amateurs and professional astronomers all over in the World. ... These data help us to analyse an accuracy of real CCD positions in the MPC Database. ... Do you test your observations of the small Solar System bodies permanently before sending them to the International Minor Planets' Center? ... Do you know a real accuracy of your positional CCD-observations in comparison with the other observatories' one ? ...

Еще в разделе: (Показать все результаты (>104) - www.accuracy.puldb.ru/ )

... Bojan Nikolic web pages (r. 329) . ... From astromap version 1.5b3, the OOF software supports deconvolution of an observation of a planet to retrieve the assumed Gaussian parameters of the beam. This deconvolution can be useful for empirical monitoring of telescope beams over time over which the planets used as sources vary significantly in size. ... Bojan Nikolic <b.nikolic@mrao.cam.ac.uk> # Initial version 2005. ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

Еще в разделе: (Показать все результаты (>2359) - www.mrao.cam.ac.uk/ )

• Bojan Nikolic -- Nested sampling modelling of Star-Formation History of the
• DUST: dustiface.h File Reference
• Determination of the relative orientation between radio and dynamical reference