... 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. ...

Еще в разделе: (Показать все результаты (>452) - www.cplire.ru/ )

• http://www.cplire.ru/html/lab234/pubs/2009-12a.pdf
• http://www.cplire.ru/html/lab234/pubs/2012_08.pdf
• http://www.cplire.ru/html/lab234/pubs/2004-15.pdf

Astronomy Discussion Forums . Forums: . ... Discussion Forums . ... If You Sent Mail, I Never Received It . Forum List | ... Post Message | ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

Еще в разделе: (Показать все результаты (>106) - www.astronomy.net/ )

• Communications For Your Astronomy Event - an Astronomy Net Article

... Director of the RAS ISR . RAS Academician . ... Astrophysics module Kvant of the orbital complex Mir launched in 1987 contains the largest on the station complex of the scientific equipment named the orbital observatory Roentgen. Observatory Roentgen consists of 4 X-ray telescopes, jointly exceeding the range of energies from 2 to 800 keV. ... Among the most significant results that were received in the observatory Roentgen are: . ... measurement of the periods of 9 X-ray pulsars; . ...

Еще в разделе: (Показать все результаты (>415) - www.cosmoworld.ru/ )

• News of Cosmonautics - October, 2002 | Russian Space News | CosmoWorld.ru
• Letter to the Deputy Head of the Administration of Russian Federation President

... SMIS ] . noise temperature of the low noise amplifier less than 100 K . automatic frequency and polarization adjustment of the received signal . double transform of frequency . power supply: single phase, 220 V, 50 Hz . power consumption: less than 30 Wt . the unit measures: 470 x 300 x 130 mm . weight: less than 10 kg . ... Back to SMIS Home Page . ...

Еще в разделе: (Показать все результаты (>42) - smis.iki.rssi.ru/ )

• SMIS IKI RAN (Equipmaent)
• SMIS IKI RAN (Satellite data)

... files referenced by the PNMs are FTPed to PASSOPS: . ... one of the standard PASS calibration files or the . ... Modules . ... Data . ADD_PASS_ARCHIVE_DIR = '/data/scheduling/spss_flight_data/pass/archive/add' . CALIBRATION_DIR = '/data/scheduling/spss_flight_data/pass/calib' . ... CCSXFER = '/data/scheduling/spss_flight_data/pass/ccsxfer' . ... PASS_ARCHIVE_DIR = '/data/scheduling/spss_flight_data/pass/archive' . PASS_TO_SPUNIX_DIR = '/data/scheduling/spss_flight_data/pass/tospunix' . ...

Еще в разделе: (Показать все результаты (>3586) - www.stsci.edu/ )

• Python: module receive_dan
• New Page 1

Radio Interferometry Principles . Radio Interferometry Signal Processing . ... A radio interferometer consists of a pair of directional antennas that are tuned to receive radio emissions from a source in a desired RF band. ... The antennas are pointed at the radio source of interest and are set up to receive the signal and process it into a form suitable for transmission to the correlator. ... In connected element interferometry, the digital signal goes directly to the correlator. ...

Еще в разделе: (Показать все результаты (>107) - www.gao.spb.ru/ )

• PULK GNSS station

... After passing degree work in MAO of NAS of of USSR Sosonkin has received the recommendation for receipt in post-graduate course of M??. ... Subjects of his scientific work were use of new receivers of radiation, in particular of electron-optical converters at observant astronomy. ... On industrial base FTI Sosonkin has created installation on base EOC UM - 92 for Cassegrain focus of a telescope ?ZT-2 and similar to it and installation with the same type EOC for focus of Newton. ...

Еще в разделе: (Показать все результаты (>313) - www.mao.kiev.ua/ )

• MAO NASU :: Topic: Vhena rada ?1_2014 (1/1)

... As part of my PhD I worked on various submillimetre instrumentation projects for the JCMT . As part of my PhD , I worked on commissioning HARP (Heterodyne Array Receiver Project), a new array spectrograph for the JCMT . ... As part of my PhD I helped to re-design the JCMT's high-frequency receiver (RxW) to operate as part of the eSMA, using HARP-design mixers and a new optics arrangement. ... Facilities that constitute the eSMA, from left to right the CSO, JCMT and SMA. ... 2010 Emily Curtis | ...

Еще в разделе: (Показать все результаты (>568) - www.mrao.cam.ac.uk/ )

• Astrophysics Group VSA
• The HARP-B Home Page
• IAU 201 Abstracts

It could be that SETI signals have arrived at the Earth, but are lower then the noise level, and our receivers cannot detect them. ... Fig. ... It follows that two zones form around the star with civilization X: "Zone Yes", where its SETI signal can be detected, and "Zone No", where its signals are hidden by noise (Fig. ... In practice, it is more efficient to use a time factor, since the problem of SETI contact does not limit the duration of the signal element and semantic text. ...

Еще в разделе: (Показать все результаты (>157) - lnfm1.sai.msu.ru/ )

• http://lnfm1.sai.msu.ru/SETI/koi/articles/abstr2.html
• http://lnfm1.sai.msu.ru/SETI/koi/bulletin/12/petrovic.html

From LISTSERV@AUVM.BITNET Sun Dec 16 00:04:45 1990 Received: from corton.inria.fr by nadia.ircam.fr, Sun, 16 Dec 90 00:04:32 +0100 Received: from resin.cicb.fr by corton.inria.fr (5.65+/90.0.9) via Fnet-EUnet id AA22555; Sun, 16 Dec 90 00:04:48 +0100 (MET) Message -Id: Received: by FRCICB62.bitnet; 15 Dec 90 23:49:56 +0100: Received: from AUVM.BITNET by FRMOP11.BITNET (Mailer R2.03B) with BSMTP id 8583; Sun, 16 ... This message is sent when the channel pressure changes. ...

Еще в разделе: (Показать все результаты (>1097) - crydee.sai.msu.ru/ )

• http://crydee.sai.msu.ru/ftproot/pub/misc/doc/MIDI/SDSFMT
• http://crydee.sai.msu.ru/ftproot/pub/misc/doc/MIDI/MIDIBNF
• http://crydee.sai.msu.ru/ftproot/pub/comp/hardware/U.S.Robotics/unofficial/Disconnect-reason.FAQ

RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . ... SSRT - Receiving systems . The SSRT has two independent receiving systems for recording solar observational data, and several ancillary receivers for checking, setting up and adjusting the instrument. The base receiving systen is a multichannel filter receiver for a simultaneous recording in 180 channels with the 500 kHz band each, adjusted at steps of about 600 kHz. ... Channel's band . ...

Еще в разделе: (Показать все результаты (>17) - ssrt.iszf.irk.ru/ )

The Agile ICC computer (nimble) contains a high-accuracy GPS-synchronized timer card that emits pulses that trigger readout of the Agile camera when run in external synch mode. ... The recommended configuration for Agile has no GPS receiver (see 1 PPS Vs. The Built-In GPS Receiver below). ... Using external 1 PPS with on a GPS receiver mode is not fully supported, in that the timer card's firmware has been programmed to assume a GPS, but the tech support person claimed it would work. ...

Еще в разделе: (Показать все результаты (>147) - www.apo.nmsu.edu/ )

• RJ11 Serial DBx Adapters
• traininglist.html
• BOurGuest.html