... Generating and compiling the SPIKE grid data. ... Plotting up the data. Generating the sky-mesh/grid data. 1 A) Generating the sky-grid data: o Procedure for making skymesh dat and overplotting available-format files onto contour plots . ... plot-skymesh-avfile.py -spike /data/lrp/sky_grid/mesh-08280-10179/saaorbit_reports/spike_collated_dec_ra_orbs_total_c17_eff30.dat.data -overplot newc.rpt -start=2009.001 -end=2010.179 -intervals=365 . Here is another example using 2-gyro data: . ...

... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Programs . Available Languages: en | ... httxt2dbm is used to generate dbm files from text input, for use in RewriteMap with the dbm map type. ... f DBM_TYPE . ... Available types are: GDBM for GDBM files, SDBM for SDBM files, DB for berkeley DB files, NDBM for NDBM files, default for the default DBM type. -i SOURCE_TXT . ... Name of the output dbm files. httxt2dbm -i rewritemap.txt -o rewritemap.dbm . ...

... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Programs . Available Languages: en . httxt2dbm is used to generate dbm files from text input, for use in RewriteMap with the dbm map type. ... httxt2dbm [ - v ] [ - f DBM_TYPE ] - i SOURCE_TXT - o OUTPUT_DBM . ... Specify the DBM type to be used for the output. ... Name of the output dbm files. httxt2dbm -i rewritemap.txt -o rewritemap.dbm . httxt2dbm -f SDBM -i rewritemap.txt -o rewritemap.dbm . ...

... Table 1: Acceptable temperature difference Invar36 0 .0 5 C А (the CTE was selected as 0.7 for the FEA) Stainless Steel 304 0.002 CА(the CTE was selected as 17.2 for the FEA) Aluminium6061 0.0015 CА(the CTE was selected as 23 for the FEA) (2) Analysis of the temperature gradients of the mount generated by an ambient temperature difference of 0.5 CА on both sides of the mount Invar , S.S. or Al ... Stainless steel material is added to Table 4 and 5 for comparison with Invar. ...

... section 7.4 ) . If the detector map (a grid of positions used to calculate and flux weight the ARF: section 7.3 ) is either psf or flat , the map bounds and pixel size may be specified. ... The user can supply an external detector map instead (section 7.3.2 ), but the bounds must cover the regions. ... The following sub-sections show examples of usage. ... Example 4: Specifying an external detector map for an extended source . Example 5: Using an RMF dataset to specify the energy grid . ...

A spherical meteorite of radius 3m enters the Earth's atmosphere at an altitude of 100km and a speed (relative to the Earth) of 30 km/s. The atmosphere slows it down, so when it hits the Earth's surface it is travelling at only 1 km/s. If half of the heat generated as it passes through the atmosphere is absorbed by the meteorite, how hot will it be when it is about to land? ... However, the number I calculated (500,000 K) is correct, as is the discussion that follows it. ...

... This thread uses PINTofALE to generate a simulated Chandra spectrum. ... define a DEM . ... pset marx .par ExposureTime=50000 OutputDir='sim_ marx ' \ ; GratingType='NONE' DetectorType=' ACIS-I ' SourceFlux=-1 \ ; SpectrumType='FILE' SpectrumFile='spec_ marx .dat' \ ; SourceType='POINT' DitherModel='INTERNAL' ; marx TSTART=2006.46 ; marx2fits sim_ marx / spec_ marx .evt ; dmextract infile= spec_ marx .evt[EVENTS][(x,y)=circle(4018,4141,10)] ; [bin pi=1:1024:1] outfile= spec_ ...

This document describes how number input can be given to tasks which request numbers from Hermes. ... list selection The following constants are implemented: pi 3.14159.... c speed of light (SI) h Planck (SI) k Boltzmann (SI) g gravitation (SI) s Stefan-Boltzman (SI) m mass of sun (SI) p parsec (SI) BLANK Universal undefined value The following mathematical functions are implemented: abs(x) absolute value of x sqrt(x) square root of x sin(x) sine of x asin(x) inverse sine ...

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... We are developing the following problems: a) combine optical and microwave technic to the indication of non-linear surface waves and wave breaking field; b) modelling of microwave propagation in a multiphase air-water interface; c) obtain quantitative dependencies of microwave radiation on geometry and statistics of wave breaking field in ocean surface; d) monitoring of ocean surface states using optical amd microwave airspace data sets. ... Important issue is spray and underwater bubbles. ...

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 . ...

Next: FOURTH Example - a9999d.sls Up: SETUP & PROCEDURE FILES Previous: SECOND Example - a9999b.sls . ... a9999.log srcfile src.list # Source the standard procedure which is invoked as 'dosrc' source /share/obs4/usr/a9999/onoff.tcl # Set correlator board and mean RF center frequencies set sbfr1 1350.0 set sbfr2 1370.0 set sbfr3 1390.0 set sbfr4 1410.0 set rfcfr 1380.0 # Setup Doppler corrections dopsetfrq $rfcfr $sbfr1 $sbfr2 $sbfr3 $sbfr4 dopsetvel 0 hel dopsetrfonly dopsetdoit # ...

Southern Mars . ... Credit Copyright: MOLA Science Team , NASA Explanation: This topographical map of the southern hemisphere of Mars was generated using data from the Mars Orbiter Laser Altimeter (MOLA). Flying on the Mars Global Surveyor spacecraft, MOLA has bounced a laser beam off the Martian surface over 200,000,000 times producing a wealth of detailed elevation measurements. ... In fact, liquid water is not present on Mars' surface today, but may have been in the past . ...

In order to calculate the line profile of a given absorption line for atomic species Z with a wavelength LAMBDA (in Angstroms) and a microturbulent velocity VT (in km/s). ... mode . ... 1) The input model may contain more than one model (i.e. it may be an entire grid of models). Spectrum will cycle through this grid NMOD times, omitting NSKIP-1 models from the . ... However, the input data following MODE must be repeated NMOD times in order to obtain equivalent results for each model in the grid. ...

This module illustrates many of the aspects of the Apache 1.2 API and, when used, demonstrates the manner in which module callbacks are triggered by the server. ... Source File: mod_example.c . ... The files in the src/modules/example directory under the Apache distribution directory tree are provided as an example to those that wish to write modules that use the Apache API. ... Example . ... Uncomment the "AddModule modules/example/mod_example" line near the bottom of the src/Configuration file. ...

Groups, ends and trees: exercises II Michele Triestino 2015-07-22 Exercise 1. ... Show that the function dS : G Ѕ G - G defined by dS (x, y) = x-1 y S is a distance on G and coincides with the graph distance on the Cayley graph of G with respect to generating set S. Exercise 4. ... Let S and S be two different finite generating sets of a group G. Show that the Cayley graphs (G, S) and (G, S) are quasi-isometric. ... Show that the Cayley graph of a finite group is quasi-isometric to a point. ...

. This diagram illustrates the boxes generated by a UL list with two LI list items. There are two parts to the illustration. The first shows the actual rendering of the boxes generated by the list elements. Background colors and border styles vary to delimit the box areas. The second shows the same rendering, but the content, padding, border, and margin edges of each box are shown explicitly. In particular, the illustration shows how vertical margins between the LI boxes collapse. Return to image.

This perspective view of Marcia Crater on the giant asteroid Vesta shows the most spectacularly preserved example of "pitted terrain," an unexpected discovery in data returned by NASA's Dawn mission. ... Scientists think low-speed collisions with carbon-rich meteorites left hydrated minerals on Vesta's surface. Heat generated during later, high-speed collisions with asteroid belt rocks released water that was previously bound within the hydrated minerals. ...

To find out if a command name is located in your command path: which ue /usr/local/bin/ue . This returns the information that the MicroEMACS editor (ue) is available on this system as the file /usr/local/bin/ue . ... To find out which (if any) of several commands are available: which delete talk ps No delete in /usr/local/utils/bin:/bin:/usr/bin: /usr/local/ucb/bin:/usr/local/gnu/bin: /usr/local/public/bin:/usr/bin/X11:. /usr/bin/talk /bin/ps . ...

The following images of the icy surface of Ganymede, the Solar System's largest moon, were made by the Galileo spacecraft during its ongoing mission to explore Jupiter and the Jovian system. ... This image was taken when Galileo was 7,448 kilometers (4,628 miles) away from Ganymede; north is to the top of the picture, and sunlight illuminates the surface from the lower left nearly overhead (77 degrees above the horizon). ... The image was taken June 27 at a range of 7,448 kilometers (4,628 miles). ...