. September 20, 2002___ SOHO/EIT, 195 (running difference) . Frame: Speed: (frames/sec) . Range Start: Range Stop:

. Weekly OPM report . Summary of the baselined LRP . Differences between current baselined LRP and previous baseline . Visits with dated PWs . Scheduling efficiency chart . Cycle Completion Reports. Long Range Planning Team, Denise Taylor ( dctaylor@stsci.edu , x4824), William Workman ( workman@stsci.edu , x4495), Ian Jordan ( jordan@stsci.edu , x5037), Patricia Royle ( royle@stsci.edu , x5071). 19 September 2000 .

Next: Release of 02 July Up: Old Releases Previous: Version 6.0 - Released Contents . Add output of velocities for sources in the summary file. 2002aug29 RCW. ... RCW 24 Jan 2003. Adding Mark5 for VLBA RCW Jan 2003. Removed Mark2 RCW 6 Feb 2003. ... Put it back 14 Feb 2003. ... Also a messages.txt file has been added to the catalog with text messages that can be sent to the runlog by routine WRTMSG. ... 26 Feb 2003 RCW . ... Add more information about frequencies etc to the OMS file. ...

... 2012 September 11 . Milky Way Over the Bungle Bungles . ... Explanation: Which part of this picture do you find more interesting -- the land or the sky? Advocates for the land might cite the beauty of the ancient domes of the Bungle Bungle Range in Western Australia . ... The photogenic Milky Way band formed over 10 billion years ago and now includes many well-known nebulae and bright stars. ... About APOD | ... NASA Official: Phillip Newman Specific rights apply . ...

... OF NICS . ... NICS FIRST LIGHT . ... The Near Infrared Camera Spectrometer ( NICS ) has been installed in the week 11-17 September 2000 at the TNG Nasmyth A focus. ... NICS is a DRO camera for infrared imaging and spectroscopy operating in wavelength range between 0.9 and 2.6 microns and is equipped with an Hawaii 1024x1024 detector. In imaging mode the platescale can range from 0.25"/pixel to 0.04"/pixel (with Adopt@TNG) correspondig to a field of view ranging from 4.2'x4.2' to 0.7'x0.7'. ...

... St Petersburg 23, September 2014 1 Motivation · Origin of Martian moons? ... Considered error sources: ­ Phobos a priori ephemerides; ­ Phobos a priori GM value; ­ measurements noise; ­ different strategies; · Methods: ­ real data analysis; ­ simulations. ... St Petersburg 23, September 2014 8 Simulations: sensitivity of the measurements to the a priori GM value Simulations: zero noise+ IMCCE a priori ephemerides +GMPH = 7.16 * 105 m3/sec2. ... St Petersburg 23, September 2014 14 Thank you! ...

Tuesday, September 28th, 2010 . 14-17 сентября 2010 года прошла международная конференция WEGENER (http://www NULL .koeri NULL .boun NULL .edu NULL .tr/jeodezi/wegener2010/) (Bogazici University, Istanbul / TURKEY), в которой мы приняли участие и сделали два доклада: . ... You are currently browsing the Лаборатория лазерной интерферометрии blog archives for September, 2010. ... Публикации за 2011 . Публикации за 2012 . ... Лаборатория лазерной интерферометрии is proudly powered by WordPress . ...

... To derive the motion of a penny dropped inside an airliner moving at 600 miles/hr (about 1000 km/hr)--should we calculate it with respect to the interior of the airliner, or with respect to the ground? ... And if a similar penny is let go inside an orbiting spaceship--should its motion be calculated relative to the interior of the spaceship, or relative to the Earth outside? ... Each such choice is known as a frame of reference . Some possible frames are -- the interior of the airliner, . ...

The ETG Mass - Size relation in different environment from z~1.6 to present Simona Mei - GEPI - Observatory of Paris - University of Paris D. Diderot Marc Huertas-Company , Francesco Shankar , Lauriane Delaye, Rossella Licitra, Anand Raichoor, Mariangela Bernardi, Chris Lidman + ACS GTO, COSMOS collaborators Wednesday , September 4, 13 Anand Raichoor Marc Huertas-Company Lauriane Delaye Rossella Licitra Francesco Shankar Wednesday , ... 2013 HAWKI Cluster survey (Lidman et al. ...

Median Twilight Image . all frames normalized by their median before averaging and corrected for 4-port structure) . Median of Normalized Twilight Images at Rotator Angle 0 . Median of Normalized Twilight Images at Random Rotator Angle . Time Frame and Rotator Angle Distribution . B_UT2_2CCD: 134 frames . ... distribution of rotator angles) . U_UT2_2CCD: 106 frames . ... uncorrected median twilight image) . B_UT2: 298 frames . ... U_UT2: 246 frames . ... B_UT3: 266 frames . ...

Astronomy Picture of the Day . ... Explanation: Star clusters, planets, and a red giant posed for this portrait of the night sky from rural Jasper County, Iowa, USA. ... The Pleiades and Hyades , the closest open or galactic star clusters to the Sun, should be recognizable to beginning stargazers . Of course gas giant Jupiter rules as the brightest object in the picture and the largest planet in the Solar System, but second largest planet Saturn is also visible nearby. ... September . ...

Astronotes Armagh Planetarium's Stellar Blog! ... Moon . ... Earth Satellites . ... By admin October 4, 2012 Posted in: Moon . A tiny second moon.This is Phobos (27 km across) seen over Mars by ESA's Mars Express (Image credit:ESA) . ... They concluded that at any given time Earth probably has a second moon. ... But, just perhaps, briefly the Earth had a second natural satellite seen by thousands of people.Remember the spectacular fireball witnessed over the UK and Ireland on 21 September 2012 ? ...

... Magnetic Fields in the Sun and stars: Measurements . Chair: Eric Priest . ... 10:00 The dynamic nature of the solar magnetic field . ... 10:40 Coffee break/Posters . ... 11:50 Magnetic Activity and Variability in Stellar Coronae (EUV) . ... 12:30 Magnetic Activity and Variability in Stellar Coronae (X-rays) . ... Magnetic Fields in the Sun and stars: Evolution . ... 14:30 Evolution of chromospheric activity in low mass stars, . ... 16:30 Activity in the Sun and late-type stars . ...

SCORPIO long-slit gallery. Here some spectra obtained on the 6m telescope with SCORPIO in long-slit mode. ... The object 0204+06 (R=19.5 mag) was observed in September, 23 2001. ... Texp=2x300 sec . Setting slit on the object . ... Subtraction of night-sky lines . Spectra energy distribution in the central object . The object Z2210+06 (R=19.7 mag) was observed in September, 24 2001. ... Spectra energy distribution in the object . ...

... The ARC echelle spectrograph records the entire visible and near-IR spectrum in one exposure on a 2048 x 2048 SITe CCD chip with 24 micron pixels, with a resolution of 30,000. (2.5 pixels) . ... CCD is a SITe TK2048E back illuminated CCD . CCD is a 2048 x 2048 pixel array . ... Field of View: Available slits (Observing Specialist installable): 1.6" x 1.6" , 1.6" x 3.2" (default), 1.6" x 4.7", 0.9" x 0.9" (pinhole) . ... 31.6 grooves/mm, blaze angle b = 63.5 deg (nominal), or tan b = 2 . ...

... Sun images . ... September : 2008 . ... Image of Sun's photosphere obtained 15.09.2008 at 22:47 UT with MDI instrument on board SOHO spacecraft . ... Image of Sun's magnetic field obtained 15.09.2008 at 22:29 UT with MDI instrument on board SOHO spacecraft . ... Image of Sun's transition region obtained 15.09.2008 at 19:55 UT with MDI instrument on board SOHO spacecraft . ... Image of Sun's corona obtained 15.09.2008 at 13:00 UT with MDI instrument on board SOHO spacecraft . Image of solar wind . ...

... 13th European VLBI Network Symposium . and Users Meeting . on September 20-23, 2016. ... 13th European VLBI Network Symposium and Users Meeting on September 20-23, 2016. ... Year book "Ephemerides of Minor Planets for 2016" on-line . ...

September 24, 2010 (Friday) Bob Hirosky, University of Virginia . ... This talk summarizes some of our latest results from the summer 2010 conferences and discusses future prospects with a substantial increase of available data. 2:00pm, 472 Willamette Hall . ... CMS has found a ridge in the two-prticle correlation of hadrons produced in pp collisions at 7 TeV at LHC. ... Interpretation of the phenomenon will be given. 4:00pm, 472 Willamette Hall . ...

Below we have listed the most convenient train connections between Zurich airport and Sonthofen on Sunday, September 14, 1997. ... The prices range from around DEM 125 (USD 72) for a single ticket in second class to around DEM 370 (USD 215) for a return ticket in first class. ... Arrival station . ... Arrival time . Zurich airport . Lindau Hbf . Immenstadt . ... Sonthofen . ... Last update: 5 June 1997 bsjoeber@eso.org . ...

Crater Gassendi . ... I made this drawing was made on the 26th of november 2001. If you compare this one with the previous drawing of Gassendi (below) the differences are clear. ... This drawing was made on the 28th of september 2001. After nearly a full month without observations I had a one hour gap between the thicker clouds. ... This drawing was made on the 29th of august 2001. ... This drawing was made on the 27th of august 2001. ... This drawing was made on the 25th of august 2001. ...