... Recent Topics . ... MAO main . ... Call for applications to the PhD program of the API/GRAPPA, Amsterdam . ... Тема: Call for applications to the PhD program of the API/GRAPPA, Amsterdam . ... We are now advertising the Call for Applications to the PhD Program of the Anton Pannekoek Institute for Astronomy (API) and the Gravitation and Astroparticle Physics Amsterdam (GRAPPA) Centre, at the University of Amsterdam. ... Applications need to be submitted on or before December 11th, 2014. ...

... One of them is band-limited power spectrum. ... Now, there is a large variety of chaotic oscillators which differ from each other by both the structure and element set and which are capable to generate chaotic oscillations from lowest frequencies up to optical bands [1-5]. ... A typical power spectrum of the output chaotic signal realized for VE= -0.85 V and VC= 5.3 V is shown in Fig. 5a. The spectrum measured in 0-1500 MHz band demonstrates the absence of oscillations outside the generation band. ...

... Kepler's 3rd Law . 21a.Applying 3rd Law . 21b. Fly to Mars! (1) . 21c. Fly to Mars! (2) . ... For circular orbits around Earth, we found . ... The distance of a satellite from the center of Earth in meters is an inconveniently big number, even before we raise it to the 3rd power. ... The ratio r' = (r / R E ) is the orbital distance measured in units of the Earth's radius. ... 25 638 838) = 5063.5 From this . ... This is the practical form of Kepler's 3rd law for Earth satellites. ...

The total radiative power output from the hot outer layers of six late-type stars (of different spectral types and luminosity class) is derived via an emission measure technique. This analysis was based on observational data from the spectral range 100A to 3000A obtained as a result of three separate satellite missions, i.e. Hubble Space Telescope, International Ultraviolet Explorer and the Extreme Ultraviolet Explorer. ...

ASTRONOMICAL SOCIET Y OF THE PACIFIC Science Education and Outreach: Forging a Path to the Future SEPTEMBER 12­16, 2009 · MILLBRAE, CALIFORNIA Applying for Scholarships Sponsored by The Spitzer Science Center UP TO $750 PER PERSON AVAILABLE FOR QUALIFIED MEETING PARTICIPANTS Who is Eligible for a Scholarship? ... Scholarship money will be distributed after the meeting as reimbursement for documented expenses incurred. How Do I Apply for a Scholarship? ... What Will Scholarships Pay For? ...

... 18.2 User preferences for colors . ... 18.4 Dynamic outlines: the 'outline' property . ... w-resize| text | ... all elements . ... For example, the 'se-resize' cursor is used when the movement starts from the south-east corner of the box. text . ... For example, if the element is broken across several lines, the outline is the minimum outline that encloses all the element's boxes. ... Graphical user interfaces may use outlines around elements to tell the user which element on the page has the focus ...

... Bad Astronomy . ... Bitesize Astronomy . ... Have you ever looked at pictures of Saturn's rings and noticed what look like gaps in the rings? ... Gian Domenico Cassini discovered a large gap in Saturn's rings in 1675. Later, an astronomer named Encke discovered a smaller gap near the edge of the rings. ... It was found long ago that an orbit in the Cassini Division, as the large gap is named, has a period almost exactly one-half that of one of Saturn's moons named Mimas. ... 2008 Phil Plait. ...

... The Large Telescopes Program Committee of Russian AS . ... Executive Secretary, e-mail: request@sao.ru . Telescope RATAN-600 Time Request deadline: I half-year (Jan. ... Program title .. ... Principal investigator .. ... Request status .. ... Retarded applications and ones not conforming to form will not be accepted by the Committee. ... In some exceptional cases the Program Committee Secretary can accept a request after deadline with permission of the Chairman of Committee or director of SAO RAS. ...

... Osaka Univ., and SLAC Calibration of HXD (GSO) Well-type phoswich of Gd2SiO5:Ce (GSO) + BGO Large stopping power (Z=64), Fast timing ( =60ns) Energy range : 30-700 keV, FOV=4.5deg(FWHM) Geometrical Area : 370cm2 , E = 10%@662keV BGO active shield also acts as the Wideband All-sky Monitor (WAM) 2 ICWG 2006.June.14 Energy Scale 511 keV 152Gd For the gain correction of each unit, prominent lines caused by the in-orbit activation seen in the background spectra are used. ... 14 ICWG 2006.June.14 ...

Date: Thu, 12 Apr 2007 18:15:45 +0200 (MEST) From: Alessandro Marconi <marconi@arcetri.astro.it> To: boch@sai.msu.ru Subject: Summer school on AGNs and VLTI Dear Colleague, here is the first announcement and call for applications for a VLTI summer school on "Active Galactic Nuclei at the highest angular resolution: theory and   observations". ... It is supported by 15 EU member states, including new member states, and thus integrates the entire European optical interferometry community. ...

... Most Important Journals . Less Popular Astronomical Journals . Physics . Space, Selectial mechanics, .. Russian Journals . ... Astrophysics & Astronomy . ... Astronomical Journal . ... New Astronomy . ... Publications of the Astronomical Society of the Pacific . ... STScI News . Space Telescope Insitute Newsletter . ... Journal of Astronomical Data . ... Journal of High-Energy Physics (mirror in CERN ) [astro, grav, hi-energy .. ... Journal of Experimental and Theoretical Physics . ...

... In the western literature this method is now called ``coupled dipole method" (CDM). ... Thus, a system of equations relative to the fields scattered by the elementary domains can be obtained, and summation of these fields gives the total scattering field. ... A subtle difference between both methods is in the fact that in the first method one works with the fields which excite a dipole (without the field of the dipole), whereas in the second method one uses the real fields in a given domain. ...

CCD output for full detector simulation in JAS Nick Sinev , University of Oregon April 22, 2004 Nick Sinev , LCWS2004 , Paris , 19-23 April , 2004 1 Outline · · · · · · · · · Brief overview of Oregon R D in CCD vertex detector Justification for need of full CCD output simulation What CCD features have been simulated CCD signal processing ... April 22, 2004 Nick Sinev, LCWS2004, Paris, 19-23 April, 2004 16 ...

Lutsenko Olena L. (PhD, Psychology, Associate Professor) Filonenko Anna (Master, Psychology, Lecturer) School of Psychology V. N.Karazin Kharkiv National University COURSE DESCRIPTIONS ­ PSYCHOLOGY OF LEADERSHIP Title and N of module 1­ Leadership Theories Themes 1. ... Ethical leadership. ... Organizational Behavior and Human Decision Processes, 95 , 140-155. ... Socializing the newcomer: The mediating role of leader-member exchange.Organizational Behavior and Human Decision Processes, 119, 114-125. ...

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Flexible frame grabbing to PC over PCI bus from area & line scan cameras . ... Analog input up to 20 MHz and digital input up to 32 Mbytes/Sec. ... The LPG-132 will easily interface to virtually any analog or digital camera and provides lightning fast PCI transfers at an amazingly attractive price. The LPG-132 will interface with any camera or sensor at data rates up to 32 Mbytes/Sec. ... The LPG-132 comes in two configurations - one for analog input and the other for digital inputs. ...

National Aeronautics and Space Administration . Lyndon B. Johnson Space Center . ... Paul Desmond Scully-Power . Payload Specialist . ... SPECIAL HONORS/AWARDS: Royal Australian Navy Exchange Scientist to U.S. Navy, 1972-1974; Order of the Decibel, 1974; U.S. Citizenship, September 17, 1982; recipient of 18 U.S. Navy Special Achievement Awards. ... Mr. Scully-Power is also a qualified Navy diver. ... July 1972 to March 1974: Australian Navy Exchange Scientist, U.S. Navy. ...

Figure 10. The circles show the thermal defocus corrections that were observed on August 15, 2000. These data were derived by combining the defocus measurements seen in Figure 6 with the thermal measurements of the truss seen in Figure 7. ... I then fit the thermal defocus data given by the circles above using only the thermal time constant and an arbitrary "zero-point" constant as fit parameters. ... M1 corresponds to a thermal time constant of 0.37 hours (22 minutes) for the rods. ...

OptInt PmWiki : Pm Wiki / Wiki Styles . ... Wiki styles allow authors to modify the color and other styling attributes of a page's contents. ... The most basic use of wiki styles is to change text attributes such as color, background color, and font. ... table class="green" style="font-style:italic; border:1px solid blue; background-color:#ffffcc":) (:cellnr:) Everything after the above line is styled with green italic text, This includes preformatted text * lists -> indented items (:tableend:) . ...

... 9) Oknyanskij V.L. 1994, "Optical-radio time delays in Q0957+561", Odessa Astronomical Publ., ... 11) Oknyanskij V.L. 1994, "Connection between X-ray and optical variability in NGC4151", in Proceedings of Int. Conf. ... 1994. 12) Oknyanskij V.L. 1994, "Connection between X-ray and optical variability in NGC4151", Astrophys. and Space Science, 222, p.157. ... 14) Oknyanskij V.L., van Groningen E., 1997, "Optical spectral variability of NGC4151 in 1990", Astronomical and Astrophys. ...