The Astrophysical Research Consortium Small Aperture Telescope (ARCSAT) is a 0.5-m (or 20") Classical Cassegrain telescope, formerly known as the SDSS Photometric Telescope (PT). ... Chief Telescope Engineer : Bill Ketzeback (bketzeba/apo.nmsu.edu) . Remote Operations Upgrade Project Manager : Joe Huehnerhoff (jwhueh/apo.nmsu.edu) . ... SurveyCam PI : Dmitry Bizyaev (dmbiz/apo.nmsu.edu) . FlareCam PI : Joe Huehnerhoff ( jwhueh/apo.nmsu.edu ) . ...

Еще в разделе: (Показать все результаты (>636) - www.apo.nmsu.edu/ )

• APO Home Page
• Untitled Document
• Astrophysical Research Consortium - Apache Point Observatory

Next: C.S. Jeffery, Research Astronomer Up: Research Previous: J.E. Chambers, Research Astronomer Contents . ... We examine spectral time-series of two lower-chromospheric lines observed with SUMER/SOHO (N I and C II ). ... Two examples of explosive events observed with SUMER/SOHO in transition region spectral lines are reported here; one detected in C IV 1548?, in a region within the northern polar coronal hole, and the other in O VI 1032?, in an active region. ...

Еще в разделе: (Показать все результаты (>2862) - star.arm.ac.uk/ )

• M.D. Smith, Research Astronomer
• C.J. Butler, Research Astronomer
• Armagh Observatory

... Change to COS FUV Pulse Height Filtering to Lower the Observed Dark Rate . ... Changing Programs & Resolving Problems . ... FUV HV History . ... 99% of source counts while removing approximately 20% of the observed dark counts. The actual amount of the dark rate reduction depends on the PHD of the dark counts in each observation, which varies between observations and with solar cycle activity. Because of the incredibly low dark rate on COS, the effect on most observations is very small. ...

Еще в разделе: (Показать все результаты (>18216) - www.stsci.edu/ )

• NICMOS Observing Strategies
• What effect does the color index of the target have on the observed Transfer
• Proposing Overview

... About ATNF overview . ... Australia Telescope Steering Committee . ... LMC H II Region Luminosities versus . Observed Ionizing Stars . ... These values are compared to the observed H II region luminosities, yielding an estimate for the mean fraction of H-ionizing photons that escape the local nebulae in this sample. We formally estimate that, overall, 0-51% of the ionizing radiation escapes the local H II regions and is available to ionize the warm, ionized medium in the LMC. ...

Еще в разделе: (Показать все результаты (>27496) - www.atnf.csiro.au/ )

• Source size measurement from observed quasar microlensing
• Photo Gallery - Astronomical Images
• Website of Tobias Westmeier - Tools - Data: NGC 300

Sternberg Astronomical Institute, Moscow University, . Moscow, Russia . Supernovae make us brighter .. Search russian astronomical resources . Mirror of International Supernovae Network ( Original site ) . Catalogue of Supernovae Stars . HTTP access to SAI Catalogue of Supernovae Stars . SAI SN Light Curves Online . ... Sternberg Astronomical Institute ( in Russian ) . ... Astronet - Russian Astronomical Network . ... Russian Foundation for Basic Research . ...

Еще в разделе: (Показать все результаты (>1852) - www.sai.msu.su/ )

... The TRACE images may be used without restrictions in publications of any kind. ... These two images, taken on 18 November 2000 at 15:54UT and 16:11UT, respectively, show such an event: the red circle in the image to the left shows a region where many loops are cooling, with bright loop tops (the intensity scales with the square root of the image to reduce the dynamic range). ... See also a collection of images related to the Sun, other cool stars, and solar-terrestrial effects . ... Images | ...

Еще в разделе: (Показать все результаты (>8708) - www.arcetri.astro.it/ )

• A Hubble diagram for Quasars
• CHIANTI atomic database
• Dust grains from the heart of supernovae

... This is the truly fun part, observing molecular and atomic gas in star-forming regions with a variety of telescopes. Depending on the temperature and density of the gas, different observations are necessary to study the components of star-forming regions. Because stars form in cool gaseous regions, I most often use radio and sub-mm observations, but I also look for opportunities to make complementary observations using infrared and optical telescopes. ... Copyright 2015 Adele Plunkett. ...

Еще в разделе: (Показать все результаты (>48282) - www.eso.org/ )

• ESO - The Seventh NEON Observing School
• ESO - Santiago Research Groups
• ESO - Garching Research Projects

... Future seminars . ... Relativistic magneto-active laser plasmas " . ... Generation of super-strong magnetic fields. ... This method is based on the observation of resonance interaction between the Landau levels in magnetic field and energy levels of plasma ions. ... The important peculiarity of the energy distribution of fast ions is their slow decreasing up to the energy of 1.4 MeV at the laser intensity of 2 10 18 W/cm 2 ; the effective temperature of fast ions is of the order of 350 keV. ...

Еще в разделе: (Показать все результаты (>1729) - www.cosmos.ru/ )

• Институт космических исследований РАН (ИКИ РАН)
• Multipoint correlations of the solar wind parameters observed by several
• Main research and development work completed in 2010 and ready for

RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . Research results on fast active processes General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Principle of generation of radio images Radio telescope's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases ... Distribution of the recorded spikes in duration . ...

Еще в разделе: (Показать все результаты (>37) - ssrt.iszf.irk.ru/ )

The neutral hydrogen in dust cloud . ... The intensity of line emission of neutral hydrogen (HI) is proportional to concentration of gas and is inverse proportional its temperature.Therefore the reduction of intensity emission of HI in dust clouds could not be interpeted simple. It has been observed the decreasing of HI line absorption at radiation frequencies and coordinates of the dense dust cloud which covered the most part of NGC 6618 nebula (figures 1 and 2). ...

Еще в разделе: (Показать все результаты (>844) - jet.sao.ru/ )

• Results scientific researchs 3
• V.Shergin's Home Page
• Results scientific researchs 21

Investigation of grain boundary faceting phase transitions in aluminium . Project 01-02-16473 funded by . ... Head of the project . ... The twins appear instead of {111}1/{115}2 or (110)S9CSL facet. ... Parallel elongated sides of the twin plate are formed by the coherent symmetric twin (1,–1,0,–2)1||(1,–1,0,–2)2 grain boundary (STGB) facets. ... Grain boundary faceting phase transitions in zinc (in Russian) . ... Faceting and roughening of the asymmetric twin grain boundaries in zinc . ...

Еще в разделе: (Показать все результаты (>1368) - www.issp.ac.ru/ )

• Laboratory of spectroscopy of defect structures ISSP RAS
• LHPP ISSP RAS
• XI International Astronomy Olympiad

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... One of the rarest but most interesting effects which can be observed with the Irkutsk IS radar is anomal high power signal registraion(coherent echo) due to strong magnetic storms. ... These signals are formed at E-layer heights in the presence of a strong electric field which causes particles to drift. ...

Еще в разделе: (Показать все результаты (>42) - rp.iszf.irk.ru/ )

• East Siberian Center for the Earth's Ionosphere Research. Ionospheric parameter
• East Siberian Center for the Earth's Ionosphere Research. Capabilities and
• East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary

Marc White . ... Turbulent entrainment processes may play an important role in the outflows from young stellar objects at all stages of their evolution. In particular, lateral entrainment of ambient material by high-velocity, well-collimated protostellar jets may be the cause of the multiple emission-line velocity components observed in the microjet-scale outflows driven by classical T Tauri stars. ... University of Amsterdam; STARPLAN, Copenhagen, Jul 2013 . ... E marc.white@anu.edu.au . ...

Еще в разделе: (Показать все результаты (>690) - www.mso.anu.edu.au/ )

• Dougal Mackey - CV
• Research Interests
• CHIAKI's Research

... 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. ...

Еще в разделе: (Показать все результаты (>6100) - www.astronomy.com/ )

• Southwest Research Institute, San Antonio, Texas | Astronomy.com
• Max Planck Institute for Solar System Research, Gottingen, Germany |
• NASA's Ames Research Center in Moffett Field, California | Astronomy.com

. Language [RU/EN] Search: . Home . UP . Research . Projects . Services . Info . News . Events . Personal . Archive . Ionosphere and radiowave propagation: structure . The main page . Information . Publications: . 2011 - 2015 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2000 - 2004 . 1995 - 1999 . Participation in International symposiums and conferences: . 2013 - 2015 . 2011 - 2012 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2002 - 2004 . N.V. Pushkov . 09/04/2016 23:52 MSK . webmaster@izmiran.ru .

Еще в разделе: (Показать все результаты (>1133) - www.izmiran.rssi.ru/ )

• IZMIRAN - Laboratory for ionosphere discontinuity investigation: The main
• IZMIRAN - Laboratory for Physics and modeling of the ionosphere: The main
• Ilya M

... Search . ... Astrophysics Group . Research . ... Research and Instrumentation . ... While this seems an extraordinary endeavour, in light of what we have learnt about Solar System planets, only a handful of key ingredients are required to start characterising an exoplanet. ... The NGTS project is a partnership between the University of Cambridge, Queen?s University Belfast, University of Warwick, University of Leicester, Observatoire de Geneve, DLR (Berlin) and Universidad Catolica de Chile. ...

Еще в разделе: (Показать все результаты (>1395) - www.mrao.cam.ac.uk/ )

• Research
• Welcome Bojan Nikolic web pages (r. 329)
• ALMA WVR phase correction algorithms and software Bojan Nikolic web pages (r.

XMM-Newton OM Response Files Page . ... Data Analysis SAS News What is SAS? ... The response files have the name om_effarea_<filter>_v2.0.rsp. The response files should be used in conjunction with a spectral data file containing the filter count rate. Such a data file may be created by editing the template filter file om_filter_default.pi with a fits editor such as 'fv' and changing the "RATE" and "STAT_ERR" entries in the SPECTRUM extension to the filter count rate and error. ...

Еще в разделе: (Показать все результаты (>2525) - xmm.vilspa.esa.es/ )

• XMM Science Objectives
• XMM-Newton SAS Download Feedback
• XMM-Newton Trainee Project 2005

... Moore Observatory is a research and advanced teaching facility of the University of Louisville. ... The 24-inch Ritchie Chretien (RC24) telescope is a research instrument used by faculty and graduate students involved in studies of exoplanets, optical properties of the atmosphere, and the development of imaging and spectroscopic technology. ... Kent (CDK20S) are collaboratively operated by the University of Louisville and the University of Southern Queensland for both research and education. ...

Еще в разделе: (Показать все результаты (>290) - www.astro.louisville.edu/ )

• University of Louisville Research Telescope Photo Gallery

... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...

Еще в разделе: (Показать все результаты (>286) - www.gao.spb.ru/ )

• http://www.gao.spb.ru/english/as/j2014/presentations/gross.pdf
• Pulkovo NEO Page: Ephemeris Support
• Model 05_w_03, all curves

... Max-Planck Institute for Solar System Research, Katlenburg-Lindau , Germany ; Институт космических исследований . ... In particular, a systematic and long-term survey of the atmosphere was missing, and most aspects of atmospheric behaviour remained puzzling. After the Magellan radar mapping mission ended in 1994, there followed a hiatus of more than a decade in Venus research, until the European Space Agency (ESA) took up the challenge and sent its own spacecraft to our planetary neighbour . ...

Еще в разделе: (Показать все результаты (>1026) - www.iki.rssi.ru/ )

• Журнал Advances in Space Research (в печати)
• Close-up of the Aurora
• Satellites which look down and observe Earth