Blackholes2 Forum Message . Forums: . ... Posted by Richard Ruquist on October 21, 2004 18:26:22 UTC . ... A charge is a standing wave. It is moving at the speed of light as made evident by the propagation of any variation in its field strength. ***ha ha. ... Charges that accelerate propagate EM waves or light, same thing. ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

... 2004 November 2 . Storm Alley on Saturn . Credit: Cassini Imaging Team , SSI , JPL , ESA , NASA . Explanation: What causes storms on Saturn? To help find out, scientists commanded the robot Cassini spacecraft now orbiting Saturn to inspect a circulating band of clouds nicknamed "Storm Alley." ... Although the above image provides data and clues, the power behind Saturn 's storms still remains a mystery. ... About APOD | ... NASA Web Site Statements, Warnings, and Disclaimers . ...

. Comedi Documentation . Prev . Next . comedi_maxdata_is_chan_specific -- maximum sample depends on channel . #include <comedilib.h> . int comedi_maxdata_is_chan_specific (comedi_t * device, unsigned int subdevice); . If each channel of the specified subdevice has different maximum sample values, this function returns 1. Otherwise, this function returns 0. On error, this function returns -1. Prev . Home . Next . comedi_range_is_chan_specific . Up . comedi_get_maxdata

... This section gives a brief description of each of the parameters available to SCHED that are specifically for VLA observations or are especially useful for VLA observations. ... Should be provided for non-VLBI observations. ... This used to be required in order to obtain calibration data for the VLBI observations. ... FREQ: and DOPPLER Warning -- these parameters cannot be used for non-VLBI observations at the VLA since they are only used to adjust the baseband converter frequencies. ...

... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Programs . ... htcacheclean is used to keep the size of mod_cache_disk 's storage within a given size limit, or limit on inodes in use. ... If one or more URLs are specified, each URL will be deleted from the cache, if present. ... Specify limit as the total disk cache size limit. ... By passing the -a or -A options to htcacheclean , the URLs within the cache will be listed as they are found, one URL per line. ...

XPA supports host-based access control for each XPA access point. You can enable/disable access control using the XPA_ACL environment variable. ... See XPA Access Points and Templates for more information about xpa templates. ... For example: xpaset -p xpa1 -acl "somehost -" will turn off all access control for somehost to the xpa1 access point, while: xpaset -p XPA:xpa1 -acl "beberly gs" will give beberly xpaget and xpaset access to the access point whose class is XPA and whose name is xpa1. ...

... This is done by taking in all input files the extension whose name is specified by the maintable parameter (called 'merged extension' in what follows) and merging the columns into a single output extension of the same name. ... Its contents is taken from the CCDID keyword (and QUADRANT for EPIC PN). ... To propagate other column specific keywords, they must be specified manually via the extensionchecks , mainattributes , maxattributes and minattributes parameters (see above). ...

... The following procedures are specific to the reduction of point astrometry data. dispinit ,[ stars _char ],[ class=class ] Initialize the dispersion corrections. ... Initialize (zero) the dispersion corrections for the specified stars. ... For scan data, initialization means setting the dispersion corrected delays equal to the averaged FDL data. dispflag , channels ,[ beams ] Flag the visibility phase for the specified channels and beams. ... Interpolate to the epochs of the point data. ...

... I am still trying to determine the cause of a difference between the results for the new and old code with the other kernels. ... I then returned to trying to figure out the difference between the old and new drizzlepac coordinate mapping. It turns out the old drizzlepac was using its internal mapping code, so I forced it to use the wcs mapping code instead.But that did .. ... I did some more testing and code reading in drizzlepac in search of the discrepancy between the old an new version. ...

... Our Solar System is a stellar-planetary unit consisting of the Sun ; the nine planets and their satellites; the asteroids, comets, and meteoroids; and interplanetary dust and gas. The dimensions of this system are specified in terms of the mean distance from the Earth to the Sun, called the astronomical unit (AU). ... The boundary between the solar system and interstellar space - called the heliopause - is estimated to occur somewhere beyond 120 AU. ... Earth . ...

... Seek help from APO hub specialists before moving to the instrument. the exposure sequence are working is a good sign that everything is talking), but the results are files filled with 0's. Array power needs to be powered in software using: tcamera arrayPower state= on or tspec arrayPower state= on 3) General error guidance: If the errors are coming from tspec or tcamera (not tcam) then there may be troubles in the instrument : --------------------------Guider ( ...

... In spite of the good potential possibilities, some of the station "Dnepr" design characteristics did not allow us to apply the usual special IS radar measurement methods. ... Thus for IS signal measurements at the "Dnepr" station, we have developed special methods for recording and processing IS signals in order to determine plasma ionospheric parameters. ... Equations (4-5) from the basis for data post processing to obtain ionosphere parameters. ...

Astronomy Picture of the Day . ... 1.06.1998 . ... June 1998 . ... 1997 1998 . ... NASA Web Site Statements, Warnings, and Disclaimers . NASA Official: Jay Norris. ... A service of: LHEA at NASA / GSFC . ... U. Based on Astronomy Picture Of the Day . Publications with keywords: Sun - flare . Publications with words: Sun - flare . ... Hole in the Sun . All the Colors of the Sun . Orange Sun Simmering . Station and Shuttle Transit the Sun . ... SDO: The Extreme Ultraviolet Sun . ...

Large-scale activity in solar powerful eruptive events of November 2004 by SOHO/EIT data, . ... Practically in all 9 events of this series, two recurring system of dimmings (regions of a decreased brightening with life-time of the order of 10–15 h ) were observed: (a) trans-equatorial dimmings connecting the north near-equatorial eruptive center with a south active region; (b) north dimmings covering a large sector between two coronal holes. ...

... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 . ... Configuring Apache to listen on specific addresses and ports. ... When Apache starts, it binds to some port and address on the local machine and waits for incoming requests. ... For example, to make the server accept connections on both port 80 and port 8000, use: . ... One complicating factor for Apache administrators is whether or not an IPv6 socket can handle both IPv4 connections and IPv6 connections. ...

... ISC Kosmotras . ... Dnepr Cluster Mission 2013 19 June 2014. ... Mission profile SHM configuration Reliability Dnepr LV Performance Launch Sites . ... Depending on requirements of a specific launch mission, ISC Kosmotras offers several configurations of the Dnepr Space Head Module (SHM), where customer s payload will be accommodated. ... The SHM configuration is selected based on the type of the launch mission: dedicated, cluster (multiple small satellite) or shared (primary payload and a piggyback)...

... This is a preliminary summary of the event on November 24, 1996, considered during the INTERBALL Workshop in Kiljavanranta, Finland, February 1998. ... Pronounced plasma sheet thinning (Bz decrease) . ... Particle burst observed inside the Polar Cap and in tail lobes . A short burst of particles detected by the Auroral Probe particle detectors during the Polar Cap crossing at 21:45 UT, almost simultaneously with the Tail Probe detectors registration of the particle burst inside the North Lobe. ...

October 16, 2006 (Monday) Srikanth Raghavendra, India . November 13, 2006 (Monday) Tuhin Roy, Boston . November 20, 2006 (Monday) Dave Soper, University of Oregon . ... Fall 2005 . Winter 2006 . Spring 2006 . Summer 2006 . Fall 2004 . ... Fall 2000 . ... Winter 2000 . Spring 2000 . Summer 2000 . ... L = 2 terms in the low-energy regime but no ? ... This system is remarkably well-suited to addressing outstanding issues in both cosmology and fundamental physics. ...

MRO Delay Line ICD Delay Line to Beam Relay System ICD INT-406-VEN-0008 The Cambridge Delay Line Team rev 0.1 10 August 2007 Cavendish Laboratory JJ Thomson Avenue Cambridge CB3 0HE UK 1 ICD Description Sub-systems Delay line Beam Relay system Org UoC Owner MF Brief description and preliminary contents Defines the mechanical interface between the delay line pipe and the beam relay pipe. ... An interface `stub' of length [TBD] provides a flange to which the beam relay pipe can be fitted see Figure 1. ...