Next: Adding plot classes Up: Plotting Previous: Plotting Contents . Plot variables are identified by a sequence number in , and are defined in terms of data variables in set_plotdata (and the corresponding function set_ploterr . ... The following additional information needs to be entered for each plot variable. Each plot variable's ID is entered in set_plotlabels for the index label it requires so that it is displayed together with the name in the plots. ...

... From the uvby photometry and proper motions for about 5500 nearby F stars we have found the following: (i) F stars , taken in narrow ranges of metallicity , show at [fe/H] 0 rather distinct cut-off in their distribution along the Main Sequence (MS) at the blue side, which is suggested to be an indication for the MS turn-off in stellar groups of fixed metallicity ; (ii) the corresponding turn-off age from theoretical isohrones strongly correlates with the ...

Patterns of calculated concentrations by pollutant for different receptor territories corresponding to stations (furthest down the picture) and POs (the remainder). While all patterns are qualitatively similar, there are marked quantitative differences between territories. The pollutants go along the abscissa in the following sequence from left to right: CO, NO, NO 2 , NOx, O 3 , PM10, SO 2 , benzene, toluene, formaldehyde, xylene, Cd, Ni (the last four are meteoparameters). ...

... MAYER{VIETORIS SEQUENCE TOPOLOGY-2, FALL 2012 The following is for the students who solved Problem 4.2 (the Bockstein's exact sequence) or are ready to believe its statement. ... The corresponding exact sequence of cell homology (see Problem 4.2) is called the Mayer{Vietoris sequence. ... Problem 3*. (a) Prove that the inclusion : C A;B (X ) C (X ) is a morphism of complexes, and is trivial on homology | ... The - corresponding exact sequence of singular homology is called the Mayer{Vietoris...

... The orbits as follows are considered: INTERBALL Tail Probe (IB_TAIL) & Auroral Probe (IB_AUR), GEOTAIL (NASA/ISAS), and POLAR (NASA). ... The situation investigation aim is to select the following favourable spatial positions (FSP) : . ... FSP3 : That part of the FSP1 & FSP2 time intervals, which corresponds to the magnetic conjugations of the any couple of the considered spacecraft. ... The polar diagram plot . ... The geocentric distance (GCD) of the 4 spacecraft as a function of the time. ...

... The keywords EXPRTIME and ZEROMAGN set the zero point for magnitudes. ... The program automatically determines a Point Spread Function when it gets proper initial values from the keywords SPROFIL. Initial values may be wrong by 0.1 each, and the program still can converge to the right Point Spread Function. ... The program looks for an initial point spread function into that descriptor at first and it uses data from the keywords SPROFILx when the descriptor DPROFILE is absent. ...

Suppose measuring system has 16 electrodes. ... If the measuring system doesn't perform redundant measurements, as the current injection through electrodes n and m is equivalent to the injection through electrodes m and n , corresponding redundant values should be set to zeros as in the following example: POLAR 16 0.000 0.908 0.513 0.313 0.202 0.280 0.752 0.000 0.000 0.869 0.351 0.243 0.297 0.311 0.340 0.000 0.000 0.000 1.358 0.484 0.205 0.212 0.355 1.214 0.000 ... EIT Gallery ...

Instructions for using Menu-driven Axis Control Software . ... Altitude and azimuth axes use position feedback and the setting is in counts per second times 10. ... Use b to set the brakes and use c to clear the brakes for the corresponding axis, either azimuth or altitude. ... Use m to move to the previously specified position and velocity for the corresponding axis; either azimuth or altitude. ... Use g to move to the previously specified position and velocity for both the azimuth and altitude axis. ...

... You are here: start €Ё difx €Ё difx_call_sequence . Trace: тАв difx_call_sequence . difx:difx_call_sequence . DIFX Call Sequence . DataStream . ... Main Loop (execute) . ... Core . ... Mode . ... The following are essential тАЬprivateтАЭ notes to sort out the call sequence used as data flows through DataStream processes and Core processes. ... Except where otherwise noted, content on this wiki is licensed under the following license: CC Attribution-Share Alike 3.0 Unported . ...

... Let be a random deviate which follows a Poissonian probability distribution about the expectation value . Although the Poisson distribution itself is only defined for integer , one can find the following continuous `envelope function' to the Poisson values: . ... where is the gamma function . ... The expectation value of is . ... Equation 5 is used both in the present program and in boxdetect to estimate the null-hypothesis probability distribution of the weighted sum of Poissonian images. ...

From: "Swain, Scott" Date: September 28, 2011 7:00:16 AM EDT Subject: SCI: *FLASH* NSSC-1 SMS Intercept Complete Following the recovery from the CU/SDF lock-up event of DOY 2011/270, the NSSC-1 intercept of the cold start SMS returning the Payload to nominal science operations has been successfully completed. In preparation for this, the N02 NSSC-1 load and ATP setting were completed at 270/23:38 UTC via OR 19146-3, corresponding to an SMS intercept time of 271/10:10:56 UTC. ...

... Content Model: Optional list header (LH), followed by one or more terms (DT) and definitions (DD). A definition list is a list of terms and corresponding definitions. Definition lists are typically formatted with the term on the left with the definition following on the right or on the next line. ... The definition list element can take the COMPACT attribute, which suggests that a compact rendering be used, and is appropriate if the list elements are small and/or the entire list is large. ...

... 2015 October 7 . La Palma Eclipse Sequence . ... Explanation: At left, a dramatic image sequence follows late September's total lunar eclipse above a rugged landscape and sea of clouds from the Canary island of La Palma . Composited in a circular fisheye projection, the brightness of the Full Perigee Moon changes drastically in transition from outside the total eclipse phase compared to its dim glow during the 72 minute long totality . ... About APOD | ... A service of: ASD at NASA / GSFC . ...

Astronomy Picture of the Day . La Palma Eclipse Sequence . ... Credit Copyright: Miguel Claro ( TWAN ) Explanation: At left, a dramatic image sequence follows late September's total lunar eclipse above a rugged landscape and sea of clouds from the Canary island of La Palma . Composited in a circular fisheye projection, the brightness of the Full Perigee Moon changes drastically in transition from outside the total eclipse phase compared to its dim glow during the 72 minute long totality . ...

Next: e-Science Up: C.S. Jeffery, Research Astronomer Previous: Post-AGB Stars . ... Simon Jeffery and Myron Smith (Space Telescope Science Institute, Baltimore, USA) have continued to study the physics of surface oscillations in the Cepheid star BWVul. They are investigating empirically how a shock wave can affect the temperature and density structure of a stellar atmosphere as it passes through. M.E. Bailey . 2004-05-18 ...

Next: Other parameters of the Up: The Model Previous: Initial binary parameters . As we only deal with initially massive binary systems (their primary's mass is higher than 10 ), which are capable of evolving off the main sequence during less than years, the compact stars left behind stellar evolution are (in the case of the most massive stars) NSs and BHs. ... For a NS belonging to a binary, the evolution complicates as the secondary star evolves: for example, (recycling), etc. ...

... Let us first find out which way -- rise in spectral resolution with some loss in the S/N ratio or increase in the S/N ratio with a fixed spectral resolution -- is better for the purpose of reduction of equivalent width determination errors. ... N -- number of counts for 1 ? ... line equivalent width, . ... Thus if the spectral resolution is managed to be increased (i.e. to decrease )without loss in the number of counts falling at 1 ?, the equivalent width measurement error is then proportional to . ...

... This distance is equivalent to 3.26 light years. ... The Universe was now a large place and the intrinsic energy output of the stars had to be huge in order that their light could reach us. ... Newton implicitly assumes space is flat . ... An Orbit in Curved Space This is a prediction made by General Relativity and confirmed by direct observation of Mercury. The Ant Universe in Flat Space . ... Hubble noticed a correlation between recessional velocity and distance. ...

Astronomy Discussion Forums . ... I Don't Follow You! ... Post Message | ... Posted by Richard D. Stafford, Ph.D. on September 16, 2002 14:59:47 UTC . ... Let me explain - harvey1 - September 16, 2002 - 18:31 UTC . Once again, we are askew of the issue. - doctordick - September 17, 2002 - 18:15 UTC . ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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