PLASMA-F solar wind experiment for Spectr-R mission . ... Measurements of interplanetary magnetic field, solar wind ions, energetic electrons and ions in the interplanetary medium. ... solar wind monitoring for space weather forecast; . ... PLASMA-F experiment, developed for the Russian Spectr-R mission (to be launched in 2007), includes: . ... fast solar wind monitor BMSW with six Faraday cup sensors, providing instantaneous determination of solar wind direction, speed, ion density and temperature; . ...

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• Arcad Instruments
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Photon/Particle Counting Image Measurement System : PIAS-TI . The PIAS-TI is an extremely sensitive image measurement device developed for imaging and quantification in ultimate levels with an extremely small number of photons, electrons and charged particles. ... The PIAS-TI is a measuring system that makes use of the technology of the photon counter to detect the input positions of individual photons or particles, and accumulate them to create an image. ...

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• Photek UV-X-gamma-Beta and Particle Imaging Systems
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• Fast Scan Multi Format Cooled CCD Camera: C4880-81

... Meta Index / Home Page / Description / Soft flare rejection for . The EPIC-pn fast timing mode was designed so that a time resolution of 0.029 milliseconds can be achieved. ... Below this energy the data is affected by so-called soft flares which are caused by stack overflows generated by high energy particles. These so-called soft flares have sharp rise (from 0 counts/sec to several thousand counts/sec in 0.10-0.15 sec) then decaying back 0 counts/sec slightly slower in about 0.3-0.4 sec). ...

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• Cross References to In-Flight Calibration Targets
• Developer's notes

The ALFA Pulsar Survey has discovered and confirmed 38 new pulsars to date. ... This program, developed by Duncan Lorimer and David Champion, searches for new pulsars in real time. ... The P-ALFA consortium plans to reduce all the data using its full frequency and time resolution, a far more computer-intensive job. ... From the confirmation and timing observations made to date, it is clear that this millisecond pulsar (MSP) is in a binary system with an orbital period of several hundred days. ...

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• lbw_crosshead_rfi_may09

ENERGETIC PARTICLE EXPERIMENT DOK-2 . ... Due to much higher energy, angular and time resolution, better separation of electrons and ions it is expected that DOK-2 experiment will allow to re-examine in more details energetic particle population and related processes in magnetosphere regions covered by the spacecraft orbit. ... Thin foil in front of detector absorbes protons with energies E<400 keV so this detector measures electron spectrum in 20 - 420 keV range. ... Energy values, keV . ...

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• The Motion of Magnetically Trapped Particles -- History
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ION AND ELECTRON ENERGY DETECTOR PAN-2 . ... The energy and angular distributions of charged particles can bring further information on the nature and spatial scales of magnetospheres processes. ... It permits the fast measurements of energy and angular parameters of charged particles in the range 40eV-40keV. ... The sensor unit is an electron electrostatic, axially symmetrical, toroidal analyzer. ... The energy range for both types of charged particles must stepped according to the logarithmic scale. ...

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• HIGH RESOLUTION IONOSPHERIC MASS SPECTROMETER P-11

... About ISSP . RAS members working in ISSP . ... A set of technological processes is developed in the Institute of Solid State Physics RAS for manufacturing of scintillation elements for radiation detectors with high space resolution. ... тАв?а a technology of direct forming of scintillation elements with necessary profiles and dimensions by means of external pressure in pressing tools with corresponding geometry. ... Scientific Secretary WWW: www.issp.ac.ru . ...

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• Laboratory of spectroscopy of defect structures ISSP RAS
• Institutes of Chernogolovka
• Astronomy: Olympiad of Scientific Centres: Institutes of Chernogolovka

Full-Simulation Calorimeter Study For Energy Flow Jet reconstruction Jan. ... Good Jet reconstruction is essential Jet Reconstruction .. Energy Flow method We use Tracker for charged particles Calorimeters neutral particles For example, in e+e- !tt (6jets,4jets) events, Charged particles carry ~60% of event energy ! ... I'll report Clustering algorithm GISMO vs GEANT4 Photon reconstruction study In this study, we use e+e- ! ... 0.9) Average # of clusters in a particle .. ...

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• http://zebu.uoregon.edu/~uochep/talks/talks01/Root2001.pdf
• http://zebu.uoregon.edu/~uochep/talks/talks02/Brau05-02.pdf
• http://zebu.uoregon.edu/~uochep/talks/talks00/brau_plenary.pdf

... About ATNF overview . ... Governance overview . Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Our people overview . ... ATCA . ... Images . ... ATNF researchers have used the Australia Telescope Compact Array near Narrabri to image the radio remnant of SN 1987A at 12 mm wavelength (18.5 GHz) using all six antennas of the Compact Array to give a maximum baseline of 6km. This image is the highest resolution image ever obtained with the Compact Array. ...

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• ATNF Daily Astronomy Picture
• SKAreport
• difx:highspecres [ATNF VLBI Wiki]

The classic solution for homogeneous sphere was suggested in 1899 by A.E.N. Love [ 330 ], in 1908 by G. Mie [ 342 ] and in 1909 by P. Debye [ 199 ]. ... Traditionally the theory of light scattering by a sphere is called the Mie theory. ... The exact solutions of the Mie problem for an optically active sphere (i.e. a sphere of optically active material [ 7 ]) and for a sphere with an optically active mantle were first obtained in 1974-5 by S. Bohren [ 158 , 159 ]. ...

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• Anomalous diffraction approximation (AD)
• Extinction properties (transmitted radiation)
• Polarization properties (transmitted radiation)

To main of Laboratory . The research work and design of optical and optical-electronic devices are carries out by laboratory staff: . ... Lens: . ... In the layout 1 prism systems perform functions of dispersive element, corrector of aberrations, optical reducer. ... Spectral range 200 - 400 nm; . ... Back Forward . ... The main corrector's function are compensation of field aberrations of the main spherical mirror of a telescope (diameter of 600 mm, f'=1200 mm) and increase aperture ratio. ...

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... Science . ... Science Users Information > Science Publications > Science Announcements > HIRES 2014: Astronomy at High Angular Resolution - A Cross-disciplinary Approach . ... Science Users Information . ... Observing with ESO Telescopes . ... ESO Science Newsletter . ... Recent years have seen a huge development in high-resolution techniques, which are critical to progress in many different areas of astronomy. ... Current and future instrumentation for high angular resolution will also be featured....

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• ESO - Science Announcements
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... Posts tagged ?particle filter? ... Astronomers have developed their ways of processing signals almost independent to but sometimes collaboratively with engineers, although the fundamental of signal processing is same: extracting information. ... This particular issue of IEEE signal processing magazine may shed lights for astronomers interested in signal processing and statistics outside the astronomical society. IEEE Signal Processing Magazine Jul. ... ArXiv] 3rd week, Dec. ... Entries RSS . ...

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• The AstroStat Slog Blog Archive Signal Processing and Bootstrap

.

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... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...

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• Hardware sector, archive 2014

A Wide Energy Band Compound Pixelated Photon Detector A Wide Energy Band Compound Pixelated Photon Detector Upendra Desai, Larry Orwig Code 682, NASA/GSFC We present a new concept of a stacked detector that provides high spectral resolution over a wide energy band (keV-MeV). ... For the energy range from sub keV to 20 keV we use silicon PIN detectors. To cover energies from 20 keV to 60 keV we use a 2-mm-thick CZT detector beneath the "Si" PIN detector. ...

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• Fabrication Technology for Single Electron Transistors and Submillimeter
• Conclusions
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... Torgashina, Gert de Lange, Leo de Jongb, Pavel A Yagoubovb a The Kotel'nikov Institute of Radio Engineering and Electronics, Moscow, Russia b SRON Netherlands Institute for Space Research, Groningen, the Netherlands Abstract--A Superconducting Integrated Receiver (SIR) developed for balloon borne instrument TELIS covers frequency range 450-650 GHz. The DSB noise temperature was measured as low as 120 K. The SIR application for high resolution spectroscopy of breathed out air has been proven. ...

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• http://www.cplire.ru/html/lab234/pubs/2009-14a.pdf
• http://www.cplire.ru/html/lab234/pubs/2005-23.pdf
• http://www.cplire.ru/html/lab234/pubs/2010-03b.pdf

... Earth at Night . ... The date was July 4th and the fiery streaks were part of the traditional annual celebration of independence day in the United States. ... Rays from an Unexpected Aurora . ... Spiral Galaxy NGC 2997 from VLT . ... The Galactic Center A Radio Mystery . ... Comet 57P Falls to Pieces . ... Orbiting the Sun every 5.9 years or so this faint comet - also christened Comet 57P/du Toit-Neujmin-Delporte for its three 1941 co-discoverers - is simply.. Sunspots and Solar Active Regions . ...

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... The following results were achieved in the course of S.P.Korolev RSC Energia's launch vehicle development efforts: . ... Two-stage intercontinental ballistic missiles R-7 and R-9, three-stage Vostok launch vehicle (consisting of R-7 and upper stage Block E as a third stage) for missions to the Moon, and four-stage Molniya launch vehicle for launching payloads to Venus and Mars (consisting of R-7 and upper stages Block I and Block L) were developed; . ... Official WEB-site of S.P.Korolev RSC Energia ...

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• RSC "Energia" - History
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• S.P.Korolev RSC Energia - MIR ORBITAL COMPLEX

This instrument is a spectometer with . ... maximum resolution of 40 Hz (8.4 m/s at 1.4 GHz) . ... The control software has been developed using Object Oriented analysis and modelling techniques ( Arcetri report 3/98 ). ... n. 3/93: ARCOS - Arcetri Correlation Spectrometer: Clock Generation module . n. 13/93: ARCOS - Arcetri Correlation Spectrometer: Project status report . ... n. 3/98: Software Analysis for the Arcetri COrrelation Spectrometer . ...

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• Arcetri Solar Physics Group: High Resolution Studies
• research field
• Adaptively smoothing astronomical images with adaptsmooth