... Magnetic fields, subatomic particles, etc., traveling in different directions fill the universe. Do they deflect or otherwise affect one another? If so, isnт??t the information we get from them distorted? ... Neutrino astronomy, which is still in its infancy, is attractive because neutrinos interact so weakly with matter that few of these distorting effects occur. Get instant access to subscriber content on Astronomy.com! ...

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... 2004 July 5 . Cassini Images Density Waves in Saturn's Rings . Credit: Cassini Imaging Team , SSI , JPL , ESA , NASA . Explanation: What causes the patterns in Saturn's rings? The Cassini spacecraft just entering orbit around Saturn has started sending back spectacular images of Saturn's immense ring system in unprecedented detail . ... The cause for the beautifully geometric type of ring structure shown above in Saturn's A ring , however, is hypothesized to be a spiral density wave . ...

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• APOD: 2015 October 9 - The Moon Entering Earth's Shadow
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What's new at the DOP? ... What is in the database? ... i) original codes realizing different methods to calculate the optical properties of non-spherical (inhomogeneous) particles; . ii) reviews of exact and approximate methods of light scattering theory ; . iii) a database of several tausends references to papers on various aspects of light-scattering theory and its applications; . ... vi) a self-training algorithm of determination of the optical properties of fractal-like clusters; . ...

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... Cassini Images Density Waves in Saturns Rings . ... Credit: Cassini Imaging Team , SSI , JPL , ESA , NASA Explanation: What causes the patterns in Saturn's rings? The Cassini spacecraft just entering orbit around Saturn has started sending back spectacular images of Saturn's immense ring system in unprecedented detail . ... The cause for the beautifully geometric type of ring structure shown above in Saturn's A ring , however, is hypothesized to be a spiral density wave . ... Crescent Saturn . ...

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Program: REGRID Purpose: Create an output map with different grid along one axis. Category: COORDINATES, MANIPULATION, UTILITY File: regrid.c Author: M.G.R. Vogelaar Keywords: INSET= Give NAME of set: There is no need to specify subsets. ... OUTSET= Give output set: This will be the name of the regridded INSET= It has sizes as defined by BOX= The size of the regridded axis is also defined by CDELT= IPOL= Enter interpolation method: [1=linear] See also 'description'. ...

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. To send a file to a different printer use the command: lpr -P name_of_printer filename . To find out the names of the printers that you can use enter the command: lpstat -p . There may be a local command that gives you this information. Example . Changing to use another printer by default .

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On this page you can compute thermodynamics, opacity and nuclear reaction rates for conditions which exist inside the Sun. ... Logarithmic partial derivative dlogP/dlogT (hi_t) . Logarithmic partial derivative dlogP/dlogRHO (hi_rho) . Logarithmic partial derivative dlogP/dlogX (hi_x) . Logarithmic partial derivative dlogU/dlogT (ksi_t) . ... Input field size does not limit the amount of data entered; you can type or paste thousands of lines (10,000 lines tested with output size over 5MB). ...

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... In today's case, a slightly off-nominal solar array slew caused the safing. ... Hubble's spacecraft computer recognized that this was not normal, and onboard safing procedures were executed as expected. ... Our STScI and GSFC teams are working on full recovery of Hubble this weekend. ... Onboard health and safety procedures will ready Hubble for science, and the science instruments (all of which are safe and in their expected states) will be brought back online accordingly. ... Hubble cheers, Ken ...

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Next: Context Levels Up: MIDAS Command Language Previous: Interrupting Procedures . ... In MIDAS, the ENTRY command defines entry points for different procedures in the same file. These individual procedures are executed by specifying also their entry point besides the file name in the `@@' command. ... DEFINE/PARAM P1 11 NUMBER "Enter input number: " . DEFINE/MAXPAR 1 ! only one parameter expected . ... DEFINE/PARAM P1 spiral IMA "Enter input image: " . ... DEFINE/LOCAL LOOP/I/1/1 0 . ...

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ENERGETIC PARTICLE EXPERIMENT DOK-2 . ... Due to much higher energy, angular and time resolution, better separation of electrons and ions it is expected that DOK-2 experiment will allow to re-examine in more details energetic particle population and related processes in magnetosphere regions covered by the spacecraft orbit. ... Thin foil in front of detector absorbes protons with energies E<400 keV so this detector measures electron spectrum in 20 - 420 keV range. ... Energy values, keV . ...

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Many entry fields permit sexagesimal entry (h:m:s.s or :':"). ... Sexagesimal entry is flexible in that you can specify one to three fields, as you desire. ... Offset and duration entry widgets assume that a single field is decimal arc-seconds or seconds ('.' or s.s) and two fields are (arc) minutes and seconds (':"." or m:s.s). ... You may specify one to three fields. ... Note: sexagesimal positions are entered in the same fashion, but a single field is decimal hours or degrees (h.h or . ...

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... The best way to illustrate the problem is with a few different examples. C example --------- The most well-known example exploits a common implementation of the UNIX popen() call, and affects primarily C programs. popen() allows the programmer to start up a command, and read from or write to it as if it were a file. ... Now imagine a CGI that uses popen to process user input. ... Perl Script example ------------------- Perl has the same problem with it's open command the C has with popen. ...

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... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. July 16, 1999 . Solar Surfin' . Image Credit: High Altitude Observatory , NCAR . Explanation: The sun's corona is a tenuous outer atmosphere composed of streams of energetic charged particles, but it is only easily seen from Earth during a total solar eclipse . ... About APOD > . ...

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• APOD: April 2, 1999 - Stars of NGC 206
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• APOD: May 5, 1998 - Aurora at Midnight

OptInt PmWiki : Pm Wiki / Access Keys . ... On Windows with Internet Explorer, press ALT + the access key. With Firefox, press SHIFT + ALT + the access key. ... Example: <a href="http://example.com" accesskey="x">Example</a> would create a link to example.com that could be triggered by clicking on the linked word "example" or using the access key Akey+x. That same action key link could be created in PmWiki markup by typing %accesskey="x"%[[http://example.com|Example]]%% , like this: Example . ...

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... Science . ... Science Users Information > Data Handling and Products > Data Reduction FAQ > What do I need to enter for the RETARDER_WAVEPLATE_CHROMATISM table when running the pmos_science_recipe? ... Observing Facilities . ... Observing with ESO Telescopes . ... Science Data Products Forum . ... ESO Data . ... After running the fors_pmos_calib recipe, the resulting RETARDER_WAVEPLATE_CHROMATISM file should be specified as an input file for the fors_pmos_science recipe to process the science data. ...

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To construct two-dimension distribution of minor planets user should specify elements/ parameters/ function that will be plotted as abscissas and ordinates. In three-dimension case one should add to them the element plotted on Z axis. ... Though you may choose elements plotted along different axes at will, often there is good reason to plot such elements as a, n, or n" along X axis (two-dimension distributions) and to plot them along Y axis in three-dimension case. ...

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. vw% ifsetup sbh 3500 . vw% set sigphdeg 90 . vw% set if1setup "if1_hybrid true if1_phdsig $sigphdeg" . vw% if1 $if1setup . 3.2 GHz . 130 deg . 3.5 GHz . 110 deg . 3.8 GHz . 90 deg . The above commands should be entered to the VX_works system either on the online computer or using a widget via "user preferences" . from CIMA .

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XMM-Newton Science Analysis System . ... Meta Index / Home Page / Description / Input There are three possible ways of entering the background. ... From a background region within the source image via the backexp parameter. In this case the task normalises for the different source and background region areas. ... From a background image in which case the background is taken from the source region within the image specified in the bkgimageset parameter. ... XMM-Newton SOC/SSC -- 2005-08-16 ...

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P.O. Box 797 Sonoita, AZ 85637-0797 June 19, 2000 Prof. David Chalmers Philosophy Department Room 213, Social Sciences Building University of Arizona Tucson, AZ 85721-0027 Dear Prof. Chalmers: Well, here's another one from Mr. At-Least-I-Thought-Of-It-Independently. ... So as a thought experiment, let's imagine that instead of having our matter transporter actually move matter, what it moves is information. ... That will make it necessary to move the matter to move consciousness. ...

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Astronotes Armagh Planetarium's Stellar Blog! ... Armagh Planetarium . ... Space Flight . ... By admin August 17, 2015 Posted in: Armagh Planetarium . ... If you are not a regular pinner, Pinterest is a website where users can share images and media. Inside of just liking and sharing content, users can pin media onto different pin boards, arranged perhaps by theme or content. ... Here you will find the latest news and views from the fascinating worlds of astronomy and space exploration. ...

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