... Credit Copyright: Jose Antonio Hervюs Explanation: What's more rare than a supermoon total lunar eclipse? How about a supermoon total lunar eclipse over a lightning storm. ... The full moon is seen setting as it faded to red in Earth's shadow and then returned to normal. ... Although the next total eclipse of a large and bright supermoon will occur in 2033, the next total eclipse of any full moon will occur in January 2018 and be best visible from eastern Asia and Australia. ... Spot the Moon . ...

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• Moon Shadow Sequence
• Journal "Peremennye Zvezdy"
• Астронет > Supermoon Total Lunar Eclipse and Lightning Storm

... 2015 September 29 . Supermoon Total Lunar Eclipse and Lightning Storm . ... Explanation: What's more rare than a supermoon total lunar eclipse? How about a supermoon total lunar eclipse over a lightning storm. ... Although the next total eclipse of a large and bright supermoon will occur in 2033, the next total eclipse of any full moon will occur in January 2018 and be best visible from eastern Asia and Australia. Follow APOD on: Facebook , Google Plus , or Twitter . ... About APOD | ...

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• APOD: 2012 November 16 - Moon Shadow Sequence

T he Siding Spring Survey (SSS) is a Near-Earth Object search program that utilises the 0.5-m Uppsala Schmidt Telescope at Siding Spring Observatory, N.S.W., Australia. ... The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. ... Based on the CSS Mission page . ... Siding Spring Survey Main Page . ...

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... About ATNF overview . ... Governance overview . Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Our people overview . ... Australian Square Kilometre Array Pathfinder . ... Parkes radio telescope . Australia Telescope Compact Array . ... Very Long Baseline Interferometry . ... Parkes | ... VLBI . ... Square Kilometre Array overview . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ...

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• VLBI antenna locations and baselines
• ATNF/AAO Postdoc Symposium 2011
• Australia Telescope National Facility

... Tonight's Sky . ... Sky this Month . ... The Sky This Week: April 1 - 10 . ... Sky this Week . ... Astronomy for Kids . ... Sky Events . Get to Know the Night Sky . Tour the Deep Sky . Sky Guide . ... Observing springtime deep-sky objects with a large telescope . ... Astronomy 101 . ... Gift Center . ... International Center for Radio Astronomy Research, Perth, Western Australia . ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...

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• CSIRO, Sydney, Australia | Astronomy.com
• Caastro, Australia | Astronomy.com
• Capturing the night's "flying flames" | Astronomy.com

... ESO is building what will be the World's largest optical telescope array, The Very Large Telescope (VLT). The VLT Project organisation is responsible for the design and construction of the Unit Telescopes, including enclosures, optics, adapter-rotators and coating unit. ... Unit Telescopes Overview - This page is outdated, an update is in process. ... Secondary mirror (M2 Unit) - This page is outdated, an update is in process. ... Coating Unit - This page is outdated, an update is in process. ...

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• Geographical Map with VLT and ALMA Locations | ESO Australia
• Location of ESO HQ Relative to Munich | ESO Australia
• Location of the Compact Configuration of ALMA | ESO Australia

... In FOS polarimetry mode the incoming beam was split into orthogonal polarization components by a Wollaston prism behind the entrance aperture. ... As with non-polarimetric observations, no concurrent WAVECAL exposure was routinely taken with polarimetry data, so the limiting accuracies of the default pipeline polarimetry wavelength calibration are the same as for the non-polarimetry case described earlier ( See "Wavelength Calibration" on page 32-49. ...

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• Index GPI Data Pipeline 1.0 documentation
• Combined IRAC2 vs HST Color-Magnitude Diagrams of Bulge Globular Clusters.
• Note on FORTRAN and C Versions

The sections <Directory> , <Location> and <Files> can contain directives which only apply to specified directories, URLs or files respectively. Also htaccess files can be used inside a directory to apply directives to that directory. ... The order of merging is: . ... If multiple <Directory> sections apply to the same directory they are processed in the configuration file order. ... Using the options in question is only possible inside a <Directory> section (or a .htaccess file). ...

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• Server-Wide Configuration

All stars derive their energy through the thermonuclear fusion of light elements in to heavy elements. High temperatures are required so that the mutual electrostatic repulsion of the protons in each fusing atomic nucleus is overcome. ... Elements with more protons in their nuclei require higher temperatures. ... This sequence is now shown in the animation below. ... First Step of the Proton-Proton Chain Narration . Second Step of the Proton-Proton Chain Narration . ...

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• Solar Collection and Energy Transport.

... 430 plots . ... 430 dome . 430 rcvr dome and carriage house centered at 430 MHz. interim correlator: . ... the old optical lab (or photometer lab) is on 110V Power from Building 1. several incandescent lights . ... seq: off, off . ... seq: on . ... A dotted purple line was made where it looked like rfi was coming from this location. spectral results 430 dome, all locations vertical scale .04Tsys (.ps) ( .pdf ) . spectral results 430 dome, all locations vertical scale .2 Tsys (.ps) ( .pdf ) . ...

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• pulsars
• OLD ANALYZ instruction sequences HI in galaxies
• location and travel for workshop at AO

Although both Joe and Sarah are registered as users on their local UNIX system, they belong to different departments; Joe is a postgrad student in artificial intelligence while Sarah is Head of the Math Department. Their respective home directories might be: /(root) | tmp /home | ai /biol /math | joe /staff | sarah . The full pathname to Joe's home directory is /home/ai/joe - that to Sarah's is /home/math/staff/sarah . ...

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• Where are commands located?
• Locating a command
• Examples of locating commands with the which command

Next: RSOG Pre-Observation Products . ... Mission Elements . ... The main mission elements (ME) are: . The RSOG, based at ASC, which is responsible for the science operation of the RadioAstron Mission. ... The Main Ballistic(Navigation) Center (MBC) belonging to Lavochkin Association coordinates preparation and exchange of orbit determination and orbit reconstraction ptoducts. ... Experiment codes of five characters are used in naming GRT related files. ... RSOG . ... Corr (GTS?) ... Corr (RSOG?) ...

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• Description of the RadioAstron project, english version

... All previous such superstars have been found along with many companion stars in the centres of crowded star clusters. The star is known as VFTS 682 from the VLT-FLAMES Tarantula Survey catalogue of the European Southern Observatory's Very Large Telescope (VLT) located at Paranal in Chile by means of the attached FLAMES instrument. ... Although VFTS 682 seems to be alone now it is not very far away from a very rich star cluster known as RMC 136 that contains several similar superstars. ...

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• Co-orbital asteroids
• Stars Beyond Maturity
• Observations with the Faulkes Telescopes

Spacecraft ephemeris , or more generally, location of an observer, given as a function of time. ... The ephemeris data for spacecraft and target bodies are normally combined in a single file called the SPICE SPK file. ... Attitude data is contained in the SPICE CK file. ... Several miscellaneous kernel files - spacecraft clock (SPICE SCLK file) and leapseconds (SPICE LSK file) - are also part of SPICE; these are used in converting time tags between various time measurement systems. ...

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• Auroral ovals [Oulu]
• LOC Information (I)
• TNP Mirrors

. INFRARED PROCESSING AND ANALYSIS CENTER

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• The VLT Images a "Rectangular" Planetary Nebula (ESO PR Photo 21/98)
• NEO precovery work on the UK Schmidt archive
• mod_auth_basic - Apache HTTP Server

... Right: The telescope's octagonal "dome" enclosure. ... MT KENT OBSERVATORY (longitude 1510 51' 19.5 E, latitude 270 S 47' 52.3 , elevation 682 m) Louisville Telescope ( Robotic astronomy research) · 50cm f/6.8 astrograph Celestron C-20 (new product) Supplier : www.celestron.com · 3.5m Sirius fibreglass dome Supplier : siriusobservatories.com · SBIG STL-6303 CCD camera + LRGB filters (UBVRI planned) Supplier : www.sbig.com · Vantage Pro weather station ...

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• http://www.astro.louisville.edu/shared_skies/archive/select/stars/ursa_minor/polaris/20111025/README
• Index of /shared_skies/archive/select/planets/uranus/sequence

... The very first thing you should do now is to locate the limits of your slitlets because this information is needed for all further commands. ... LOCATE/MOS . ... Then you should have a look at your flat field and try again with . ... OFFSET/MOS . ... The results are stored in the frame . If you have not written anything to this keyword it will derive the name of the normalized flat field by adding an `n' to the name of the input flat (e.g. nmosff1 ) and write the name to . ... FLAT/MOS . ...

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• Location of slitlets and flat-field correction
• Weather data Location
• Configuration Sections - Apache HTTP Server

... Bojan Nikolic web pages (r. 329) . ... Building CASA . ... /ccm/CCM_Local/CCM_OCL/OclHelpers.h 2009-09-29 14:30:42.000000000 +0100 @@ -123,10 +123,10 @@ OCL_Collection T excluding( const T object ) const { OCL_Collection T result; - const int s = size(); + const int s = vector T ::size(); for( int index=0; index s; index++ ) { - const T element = operator[](index); + ... Building CCMTools as required by CASA . ... Building . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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• Workshop on Simulations for ALMA

... Radiation mechanisms of astrophysical objects: classics today . ... Saint-Petersburg is the 2n d largest city in Russia located on the Neva River at the head of the Gulf of Finland on the Baltic Sea. Founded in 1703 by Tsar Peter the Great Saint Petersburg was the imperial capital of Russia until 1918. The meeting will be held in the Conference Hall of historical building of the Saint-Petersburg State University - Twelve Collegia. ... Conference program . ... Conference location . ...

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• Alexei Kritsuk's Home Page
• INI main page

WPLTN Technical Workshop . ... WPLTN-2012) . ... of the International Scientific Technical Conference WPLTN-2012 . ... Having an opinion that the collocation of various space geodesy measurement technologies has a fundamental role in increasing the accuracy of fundamental and applied positioning, navigation and timing provision, the International Scientific Technical Conference WPLTN-2012 has come to the following conclusions: 2.1. ... Web-page . ... Resolution of the conference WPLTN-2012 . ...

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• Keywords_122
• EVN Symposium 2016