... 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 . ...

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. ...

... dataset . ... The input image dataset. outset . ... integer . ... The number of columns of the input image to fit into 1 column of the output image. binysize . ... The number of rows of the input image to fit into 1 row of the output image. offsetx . ... offsetx . The number of the first column of the input image to go into the first column of the output image is given by offsetx . ... The number of the first row of the input image to go into the first row of the output image is given by offsety . ...

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. ...

... 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. ...

This form will calculate the count rates for a simulated direct image of ONE point source in a 512X512 FOC image with an average value for the background. ... Calculate exposure time to reach a S/N of . ... Calculate S/N reached in an exposure time of . ... Choose a spectra . ... or, created by FOCSIM that is either: . ... a Power-law: F_lambda(ergs cm -2 s -1 -1 ) = lambda ** ( ) . ... U magnitudes B magnitudes V magnitudes ergs cm -2 s -1 -1 photons cm -2 s -1 -1 at Angstroms. ...

... 25.01.2001 . OC "MIR") . ... Flight orbit number (day) . ... Orbit period (in min) . ... Mean orbit altitude (km) . ... solar F 10.7 flux . ... Date of the orbit parameters calculations 25.01.2001. ... Cargo ship "Progress M-43" (№243) undocked the station, burn ~ 9.5 m/s was executed to break it out from the Station "Mir" . ... 08.19.23 "Progress" 243 undocked OC "Mir". Progress" 243 breakout from the Station performed ( н V=9,5 m/sec); the Station is switched to the spinning mode. ...

The parameter agnclass describes the nature of the object. The table below gives the list of the notes of agnclass, together with their description. agnclass . Description . ... Quasi-stellar objects (QSO) . ... Hight polarized objects . ... Broad-line Seyfert 1 . ... Narrow-line Seyfert 1 . ... S1 with a broad Paschen Hbeta line . ... Seyfert 2 . ... Possibly Seyfert galaxies . ... S3 with broad Balmer lines . ... S3 with broad Balmer lines seen only in the polarized light . ... HyperLeda . ...

Next: Algorithm Up: Description of program searchdup Previous: Program parameters . Program is started by the command searchdup with no parameters. The graphic user interface appears, with all parameters to their default value. After parameter entry, the button START starts data processing. ... It is possible to stop the program clicking button BREAK! ... It is then possible to change some parameters, or to exit the program, by clicking on the EXIT button. ... 2000-06-30 ...

... 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) . ...

... CentralProcessor 0.11 documentation . ... These parameters govern the pre-processing needed for the science field, to split by beam, flag, apply the bandpass (although none of the parameters listed here relate to that), and average to continuum resolution. ... FIELD_SELECTION_SCIENCE . ... Range of channels in science observation (used in splitting and averaging). ... Dynamic threshold applied to a