DIGITAL WDC EXCHANGE FORMAT . FOR OBSERVATORY 1.0 MINUTE VALUES 1. ... DATA-1 .. DATA-60 are 1-minute values of the given element for that hour. ... Typically, digital 1-minute values received by WDCs from organizations operating automatic magnetic observatory instruments are averages of more frequendy sampled values, e.g. 10-second point samples. ... If the method used to obtain 1-minute average values is important to a user, the WDC will assist in determining the exact procedure applied. ...

Общая Астрономическая Конференция . ... Правила форума . ... Сообщения за день . ... Добро пожаловать на Общая Астрономическая Конференция. ... Форумы общей направленности . Любые вопросы от новичков (просматривают: 17) . ... Общий форум любителей астрономии (просматривают: 7) . ... Новости магазина Starshop.ru . ... Менее астрономические товары (просматривают: 1) . ... Форум исключительно для сообщений об испытаниях астрономической техники. ... Общая Астрономическая Конференция статистика . ...

... Apr 14, 2016 - Monthly Meeting . ... The Amateur Telescope Makers of Boston, Inc. ATMoB) is an astronomy club devoted to telescope making, observing, and studying the heavens. ... CURRENT MOON . ... April Sky . ... Lyrids Meteor Shower . ... Sources: NASA JPL Space Calendar , StarDate Online , Sky Telescope , Harvard-Smithsonian Center for Astrophysics , RASC Observer’s Handbook , Abrams Planetarium Sky Calendar and Astronomy Magazine . ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

... You are here: start €Ё lbaops €Ё rtfcobs . ... VLBI Schedule . ... lbaops:rtfcobs . ... Remote recording . ... At each observatory you need to run the obs.pl program. ... Once you have logged onto the recorder PCs, you need to cd to the directory where the data is being recorded then run obs.pl. ... Note that at the ATNF observatories we also record data onto cave-store-ext and pam-store-ext. In such cases you need to run obs.pl on the machine where the data is being recorded - see the note below. ...

SN 1999aa - A Third Supernova Discovery . Just 9 weeks after the discovery of SN 1998ey a suspect was found 1" east and 28" north from the centre of NGC 2595 on Feb.11.0166 U.T.. ... Further inspection of 6 images of NGC 2595 taken during Feb. and March 1998 showed no object at the position of the suspect. ... Beijing Astronomical Observatory recorded SN 1999aa on Feb. 11.6 and 12.6 UT, the first obervation being only 14 hours after the discovery. ... Back to Supernova 1999aa in NGC 2595 . ...

The Chandra X-ray Observatory is the third of NASA's four " Great Observatories ", and is used by Astronomers to study some of the more extreme objects and events (in terms of temperature and mass) in the Universe. ... This page uses Javascript to show you the timeline for Chandra, NASA's X-ray Observatory. ... If you can not enable Javascript, much of the information is available at the Chandra X-ray Center . Further information on Chandra can be found at: . ... The Chandra X-ray Center . ...

Domes Forum Message . ... Domes and Observatories Discussion | Post . ... Sharing Your Observatory Plans . ... Post Message | ... John . ... Re: Sharing your Observatory Plans - louielouie - November 7, 2000 - 16:10 UTC . Re: Re: Sharing your Observatory Plans - firefighter - January 14, 2001 - 14:22 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" . ...

A great many years ago, one of our members created a type of slide show that took you on a guided tour of Warren Rupp Observatory. Needless to say, that was a great many years ago and things have changed for the better! ... Warren Rupp Observatory is proud to be associated with these fine groups and endorse these resources.. ... The WRO/RAS was designed and donated by Tammy Plotner - Copyright 2008-2015; Original Content - Tammy Plotner - Copyright 2008-2015; All rights reserved. ...

This form calculates which transits of the 1039 known transiting exoplanets are observable from a given location at a given time. Specify a time window, an observing location (either an observatory from the list or choose "Enter latitude/longitude" at the end of the list), and optionally any filters (e.g. minimum transit depth or elevation). The output includes transit time and elevation, and links to further information about each object, including finding charts and airmass plots. ...

... Цвет: PLUSH BLUSH . ... Модель: SHOW ME OFF . Сезон: SS15 . ... Легкий, свободный и невероятно женственный топ Show Me Off с вязанными элементами будет смотреться так же утонченно как и платье. ... Бренд: Novline . ... Применяемость: Renault Logan . ...

Kermit : . It's the Muppet Show with our Very Special Guest Star, _____! ... It's time to play the music . ... It's time to meet the Muppets on the Muppet Show tonight. ... It's time to raise the curtain on the Muppet Show tonight. ... Muppets : . And now let's get things started Audience : . Why don't you get things started Kermit : . It's time to get things started Muppets : . on the most sensational inspirational celebrational Muppetational this is what we call the Muppet Show! ...

... Hartmann Test Using a Screen With Four Holes 2 Hartmann test with four holes screen The theoretical concept of the primary aberrations measurement by four apertures Hartmann test introduced by "Malacara" * and "SalasPeimbert et. al. ... Black curve show the calculated coefficients for phase screens which have 8 modes of Zernike aberrations and red curve show the calculated coefficient for original phase screen. (a) astigmatism 45 (b) astigmatism 090 14 Coma Coma modes of Zernike aberration. ...

... Bad Astronomy . ... Bitesize Astronomy . ... Bad Astro Store . ... Site Info . ... It is from from Voyager 1 and shows a whopping big impact crater dominating the profile of the moon. Note that Mimas is about 400 kilometers across (about 250 miles). ... The wall around the crater is 5 kilometers high, and that central peak rises 6 kilometers above the surface (many impact craters have a large central peak which is caused by a pressure rebound from the impact). ... 2008 Phil Plait. ...

Next: The Sliding-Cell Detection Program for Chandra X-ray Data . ... The Chandra X-ray Observatory uses an optical CCD in its aspect camera. ... This ``on the fly'' determination allows us to adjust for variations in CCD conditions between dark current calibration observations and provides useful information for identifying bad regions on the Aspect camera CCD. ... As the aspect camera CCD is exposed to radiation, warm pixels will develop. ... Chandra's Aspect camera detector is a pixel CCD. ...

. Experimental base . • . Yakutsk Extensive Air Shower (EAS) Array . • . Polar Geocosmophysical Observatory (PGO) . • . Complex Geophysical Station (CGS) . • . Optical Station . • . Radiophysical Station . • . Yakutsk Cosmic Ray Spectrograph . • . Magnetic Observatory . • . Ionospheric Station . • . Station for Receiving of Satellite Information .

... Astronomy news . ... Saturnian Moon Shows Evidence Of Ammonia . Data collected during two close flybys of Saturn's moon Enceladus by NASA's Cassini spacecraft add more fuel to the fire about the Saturnian ice world containing sub-surface liquid water. ... In space, the presence of ammonia provides strong evidence for the existence of at least some liquid water. How could ammonia equate to liquid water inside an ice-covered moon in one of the chillier neighborhoods of our solar system? ...

In the C and TC shell, to show the values of all your environment variables: printenv TERM=vt100 HOME=/home/eucs/helper SHELL=/usr/local/bin/Tcsh USER=helper TZ=GMT0BST UCBPATH=:/usr/ucb:/bin:/usr/bin ATTPATH=:/bin:/usr/bin UCBSHELL=/usr/local/bin/Tcsh ATTSHELL=/bin/sh LOGNAME=helper MAIL=/home/eucs/helper/.mail . ... This shows the value of an assorted range of variables. ...

Photograph quality The photographs must be: I no more than 6-months old 35­40mm in width close up of your head and top of your shoulders so that your face takes up 70­80% of the photograph in sharp focus and clear of high quality with no ink marks or creases too close too far away I I I I blurred ink marked/creased I The photographs must: show you looking directly at the camera ...

Spectropolarimetry and modeling of Galactic Wolf-Rayet star WR156 O LGA M A RY E VA Special Astrophysical Observatory RAS; olga.maryeva@gmail.com For the first time spectropolarimetric observations of Wolf-Rayet star WR156 (WN8h sub-class) were conducted. ... This polarization is, most probably, has an interstellar origin, as its magnitude and orientation are similar to the ones of field stars. ... By its parameters WR156 is similar to other WN8h stars, displaying the line effect. ...

Next: ASSIGN/GRAPHIC and COPY/GRAPHIC Up: General Commands Previous: General Commands . SET/GRAPHIC plays an important role in the plot package. This command gives the user control over the plot size, line types ( LTYPE ) љ , line thickness ( LWIDTH ) љ , symbol type ( STYPE ) љ and size ( SSIZE ) љ , etc. In Table the various options that can be set with the SET/GRAPH command are listed, together with the default settings. ... When STYPE=0 a line will be drawn corresponding to LTYPE . ...