previous next contents properties index . ... Inherited? ... inherit . ... yes . aural . ... visual . ... none | ... length> ]{1,2} | ... block-level and replaced elements . ... see individual properties . ... table' and 'inline-table' elements . ... length> <length> ? ... the value of the 'color' property . ... auto | ... positioned elements . ... table-caption' elements . ... yes, the computed value is inherited . ... all elements except non-replaced inline elements and table elements . ...

Your working environment is defined whenever you login or start another shell . This environment is set using the values that the shell finds in initialisation files which it always reads as it starts up. You can change your working environment by editing these files and setting new values for variables. Each shell handles its initialisation files in a different way; select one of the headings below for the shell that you use. ... Changing your environment: Bourne shell . ...

... More on 51 Peg: . The discovery of a Jupiter--mass planet in orbit around the solar--type star 51Peg has been reported by Michel Mayor and Didier Queloz (Geneva Observatory) on October 6th at the 9th Cambridge workshop on "cool stars, stellar systems, and the sun" held at Florence (Italy). ... Recall that the measurements of radial velocity only yield v sin i which in turn gives us M sin i. For most values of i, sin i will be greater than 0.5 and this gives a mass estimate of 0.5 Jupiter masses. ...

... ratios Evolution Equations with · Now write · Evolution equations now · Define trajectories via Cosmic Trajectories Dust =0 de Sitter phase Radiation =1/3 Initial singularity Cosmic Trajectories · For a range of initial conditions, models re-focus around the flat ... case · For decoupled matter and radiation can solve the equations exactly · Solutions governed by two constants: Non-Euclidean Geometry · Axioms of ...

Method of Calculating Cometary Orbits . ... A method of constructing a numerical theory of comet motion covering large intervals of time is presented. ... Very Long Baseline Interferometry (VLBI), Near Earth Objects (NEOs), calculating cometary orbits, numerical theory of comet motion covering large intervals of time , radial component of non-gravitational acceleration , transverse component of non-gravitational acceleration , normal component of non-gravitational ...

... For the past years I have been working on the problem of synthesis of light curves of close binary systems, consisting of a normal star and a compact object (point object with fixed X-ray luminosity). ... Possible existence of a bright spot on the disk's lateral surface is taken into account. ... The last of then will be published in Gordon and Breach Publishers ( Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ... Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ...

... Mars to Appear Normal this August . ... October is the best month to see Mars this year. ... As Earth catches up to Mars in their respective orbits around the Sun, Mars will keep rising earlier in the night. On 2005 October 30, Earth will have caught up to Mars and the planets will be the nearest to each other in their orbits -- this time around. On October 30, Mars will be nearly opposite to the Sun, rise at sunset, set at sunrise, and appear highest and brightest around midnight. ...

Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 29.08 - 04.09.2011, Forecast on 24 - 31.10.2011, Carrington Rotations 2015,2016 (22,71.09; 19,99.10.. 2011) SOLAR SUNSPOT ACTIVITY OF THE LAST PERIOD REMAINED BY 21.09 AT HIGH LEVEL, HAVING REACHED ON OCTOBER, 20-21th THE GREATEST VALUES FOR THE CURRENT SOLAR CYCLE THEN HAS STARTED TO DECREASE GRADUALLY. ... NEXT WEEK THE LEVEL OF SUNSPOT ACTIVITY IS EXPECTED TO BE THE AVERAGE. ...

This is how a typical dispersion modeling result looks when shown as a map. ... Their numerical values are shown at the top. White normally means no data, but high values may be also shown as white if above the fixed high limit (that is, if no automatic normalization is used for colors). Note that calculations were done both for cell positions and for station positions, so both are colored. PO territories are filled by color corresponding to the average value of cells overlaying them. ...

I was wondering what conditions should be met to have the "darkest" sky .. ... Upon the above publication of the Southern Galactic hemisphere, TunГ Tezel started seeking opportunities to create the Northern counterpart image. ... So, the initial quest of having the darkest possible sky have delivered us these two all-sky images of the two galactic hemispheres as seen from Planet Earth. Zoomable and 'full-screenable' fisheye view of the "darkest sky" Southern Galactic Hemisphere image. ...

phpBB2 - attach_mod schema - Postgresql $Id: attach_postgres_schema.sql,v 1.3 2003/03/09 02:21:03 acydburn Exp $ */ /* Create auto_increment values */ CREATE SEQUENCE phpbb_extensions_id_seq start 1 increment 1 maxvalue 2147483647 minvalue 1 cache 1; CREATE SEQUENCE phpbb_forbidden_extensions_id_seq start 1 increment 1 maxvalue 2147483647 minvalue 1 cache 1; CREATE SEQUENCE phpbb_extension_groups_id_seq start 1 increment 1 maxvalue 2147483647 minvalue 1 cache 1; ...

... Aims: Today, large ground-based instruments, like VISIR on the VLT, providing diffraction-limited (about 0.3 arcsec) images in the mid-infrared where strong PAH features appear enable us to see the flaring structure of the disks around Herbig Ae stars. Although great progress has been made in modelling the disk with radiative transfer models able to reproduce the spectral energy distribution (SED) of Herbig Ae stars, the constraints brought by images have not been yet fully exploited. ...

... In the median ; function of IDL, the higher of the two values is returned. ... Felix Stoehr, [ST-ECF] xxx = xx(sort(xx)) n = n_elements(xxx) if ((n mod 2) eq 0) then begin return , 0.5 * (max([0,xxx(n/2-1)])+xxx(n/2)) endif else begin return , xxx((n-1)/2) endelse end ;----------------------------------------------------------------------------------------- ; ;***************************************************************************************** function DER_SNR , ...

... 2 Measurement of PMTs counting characteristics and selection of op erating p oint To select the operating point of the PMT, that is the optimal values of the high voltage supply and pulse discrimination threshold, the command run counting=hv value is provided in the program mass. ... Starting with the minimum voltage (say 550 V) run command run counting=550 for the measurement execution. ... It is recommended to take measurements for the set of values of 0.4, 0.6, 0.8, 1.0. ...

... We present a new method for visualizing flux variations in X-ray images. ... The time variability image so constructed visually shows area where strong time variation occurred. ... Figure 1. shows the intensity (left) and time variability (right) image of the ROSAT field centered on the X-ray source MKW 3. ... The corresponding time variability image is shown to the right. ... These examples clearly show the power of the method described in evidencing variable sources in crowded X-ray images. ...

Download Izmccd (~2.7 MB). Installation and adjustment of program. ... Read the license agreement . If you not accept the license agreement, you must press the button " I not accept ", to delete files of the distributive version izmccd and to stop any use izmccd; otherwise, press the button " I accept ". ... Fill in areas . ... Size of pixel" in millimeters X and Y. Characteristic values are from 0.005 up to 0.040. ... Do not change other values during initial adjustment of the program. ...

... St Petersburg 23, September 2014 1 Motivation · Origin of Martian moons? ... Considered error sources: ­ Phobos a priori ephemerides; ­ Phobos a priori GM value; ­ measurements noise; ­ different strategies; · Methods: ­ real data analysis; ­ simulations. ... St Petersburg 23, September 2014 8 Simulations: sensitivity of the measurements to the a priori GM value Simulations: zero noise+ IMCCE a priori ephemerides +GMPH = 7.16 * 105 m3/sec2. ... St Petersburg 23, September 2014 14 Thank you! ...

... ON THE ROLE OF LARGE-SCALE PLASMA IRREGULARITIES AT THE FINAL STAGE OF ANOMALOUS ABSOPTION DEVELOPING UNDER HF HEATING OF THE IONOSPHERE . ... Fig. ... With the aid of numerical statistical modeling based on multiple ray tracing it is shown that in presence of large-scale irregularities the reflected signal amplitude mean value is increased significantly. ... Dependence of the mean amplitude of the reflected from the ionosphere signal on the large-scale (10-50 km) electron density irregularity level...

... Bit . ... Status . Event Time . ... Bits . closed . ... Roof Position . ... automatic . ... 0D:18H:51M:32S . swmode=AUTOMATIC . Roof System . ... 18D:16H:51M:51S . OK SunAltOpen: -1.000000, SunAltClose: -1.000000, SunNow(Alt,Az): +65.769951,-168.421600 . Time of Last Reboot: 29 Days, 21h:28m:00s . Time of ObsDaemon Reboot: +2457458.4259953703731298 (uptime: 29 days, 21h:26m:24s) . ...

... News . ... Research areas . ... English News . ... In the spring of this year the scientists of Samara State Aerospace University (SSAU) will proceed to integrated exploration environment in the near-Earth space and its impact on the engineered materials of spacecraft. ... This spring it will be launched into space by the first carrier rocket from the new Russian space launcher complex Vostochniy. ... The equipment set is designed and manufactured in SSAU Institute of Space Device Engineering (ISDE)...