... The principle of communication using unstable periodic orbits (UPO) of a chaotic attractor can be represented as follows. ... Lozi attractor with period-16 unstable periodic orbit. ... Processing of the unstable orbits Forming of asynchronous data stream. ... Asynchronous packet data transmission Unstable periodic orbits can be utilized for not only encoding the entire transmitted information, but also for attributing it to this or that group of users, i.e., they play the role of "chaotic markers". ...

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• Basic Principles of Direct Chaotic Communications - NDCS-03
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• Project 5 - State Program "Condenced Matter Physics"

... ATNF Home . About ATNF . ... About ATNF overview . ... Governance overview . Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Our people overview . ... Publications overview . ... Careers overview . ... ATNF facilities . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... Parkes | ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... A project of the ATNF Astrophysics Group . ...

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• The Parkes 21cm Multibeam Receiver
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• ATCA_report

... Up: Data Pipelines . ... The Data Handling System (DHS), developed for the Gemini project by the Canadian Astronomy Data Centre, accepts observational data from multiple sources. There may be data descriptions, image data in chunks (to be composed into a single image), and multiple images for one dataset, all being received at different times. ... DHS is data-driven and is composed of a collection of servers that work together to act on any data it receives from any Gemini principal system. ...

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• ADASS 2003 Conference Proceedings
• Mapping the Jagiellonian Field of Galaxies
• Data Structure and Software of the UCAC-S Project

Note: These models for T-receiver are based on measurements for all of the 14 pipelines. download Trx polynomial fit parameters . ... any additional offset to be addded as a correction not incorporated in the model (e.g. the contribution to receiver temperature from beyond the pre-amplifier stages), . ... No. of coefficient pairs, n_harm, associated with the harmonic (Cos & Sin) part of the fit (where the final fit is a simple sum of the two parts).. ... cos(j*pi*X/2) & sin(j*pi*X/2), . ...

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• RECEIVER CHOICE
• gregorian cals
• rcvr shutters

... Driver ID: GPS-AS2201 . ... This driver supports the Austron 2200A/2201A GPS/LORAN Synchronized Clock and Timing Receiver connected via a serial port. It supports several special features of the clock, including the Input Buffer Module, Output Buffer Module, IRIG-B Interface Module and LORAN Assist Module. ... The specific data collection commands and attributes are embedded in the driver source code; however, the collection process can be enabled or disabled using the flag4 flag. ...

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• Reference Clock Drivers
• Further Information and Bibliography
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... The set of equipment includes 8-mm band transmitting/receiving module (TRM), 1.5-cm band multi-channel receiver, and 2-cm band receiving module. TRM, operating in 8-mm range, assures two-way communication with up to 10 Mbaud rate (33–36 GHz input/output frequency). The 1.5-cm receiver is designed for receiving the service and scientific data from the space radio interferometer in 18–26 GHz frequency range (8 channels) with up to 36 Mbaud data transfer rate. ... 1.5-cm multi-channel receiver . ...

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Next: XMM_MISCDATA Up: CCF Components Previous: Appendix: List of valid Contents . While some relevant RGS calibration data are given in the general-purpose CCF components . ... Some information concerning the maintenance of RGS CCF files is given below, though more details are available in the release notes that accompany new file releases and other technical notes. ... Use of CCF components by RGS SAS tasks . ... Purpose . Functionality . Ground calibration . Maintenance procedures . ...

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• Procedure
• omi_stepbystep

... My research focusses on spectral line and dust continuum observations of star formation in the Galaxy, particularly using the JCMT. My PhD thesis involved using HARP (the Heterodyne Array Receiver Project, see also my technical pages ), an array spectrograph built in the Cavendish Astrophysics Group for the James Clerk Maxwell Telescope ( JCMT ) for a wide-field survey of star formation. ... For an overview of the survey see Curtis, Richer Buckle (2010) . ... 2010) . ... 2010 Emily Curtis | ...

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• Astrophysics Group VSA
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• OptInt PmWiki : Wiki Structure

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... ISS Russian Segment . ... Study of USH-radio signal transmit/receive conditions in the mode of onboard radio beacon in the ISS RS using world-wide ham radio network. ... Determining zones of DP radio shadowing zones by the station structural members depending upon its spatial orientation. ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

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• S.P. Korolev RSC Energia - News

... About Plug-ins page 8 . ... building plug-ins 32 . ... function group (Netscape) 108 . function group (Plug-in) 106 . ... creating a stream 75 . creating an instance of a plug-in 41 . ... function group (Netscape) 107 . function group (Plug-in) 105 . drawing methods, reference 122 . ... receiving data streams 109 . ... Plug-in methods 9 . ... receiving data streams group (Netscape) 109 . receiving data streams group (Plug-in) 106 . ... sending data streams group (Netscape) 109 . ...

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• HyperLEDA: documentation
• Plug-in API Reference
• THE MOLONGLO REFERENCE CATALOGUE/1Jy. II

The information path to prepare, perform and reduce a radioastronomical observation, using the Arcos correlator , is schematized in the figure: . The programs reside part on the computer network of the Arcetri Observatory, and part at the Medicina Radio Telescope . All programs running at Arcetri are written for a Sun workstation, and are public domain software, available upon request. Programs running at the telescope are written for a PC with DOS/Windows (or Linux).

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• HwB: EIA-449 (RS-449) Connector (Offline)
• Radioastronomy laboratory
• Arcetri Radioastronomy group

This home page belongs to small group of scientists working at . Sternberg Astronomical Institute which is a part of Moscow State University . ... Электронная библиотека научно-технической и художественной литературы (доступна только из ГАИШ) . ... Local staff . Dr. Edward Kononovich (konon -at- sai.msu.ru), Associate Professor . ... Dr. Sergey Ayukov (asv -at- sai.msu.ru), Research Fellow, Webmaster of the group . ... Joint seminar of Solar Studies Structure Group and Solar Photometry Group . ...

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• Not so well documented Device Helpers in OS/2

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 . ...

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Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Antenna system . ... The Irkutsk incoherent scatter radar is one of the world's nine active radars which give the opportunity to investigate ionosphere by the incoherent scatter method. ... Antenna gain coefficient . ... Antenna . ... Two antennas . ... To get an idea what station "Dnepr" antenna system looks like, let us consider some of the radar views which are given by the photographs General view and Side view . ...

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• East Siberian Center of Earth Ionosphere Research. IS radar Receivers Hall.
• East Siberian Center of Earth Ionosphere Research. Chirp ionosonde.

... NICMOS Data Handbook > Chapter 2: Data Structures > 2.4 From the Phase II Proposal to Your Data . ... The connection between the Exposure Logsheet that each observer fills out during the Phase II proposal process and the datasets and associations that the observer receives once the observations are executed can be better understood through some examples. The first example shows an exposure logsheet entry that will generate only one dataset: . ... Config: NIC2 . Opmode: MULTIACCUM . ...

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• WFC3 Data Handbook
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• ACS Data Handbook

Communications For Your Astronomy Event . Articles | ... Some manufacturers have received approval to market radios that are certified for use in both the Family Radio Service (FRS) and the General Mobile Radio Service (GMRS). ... FRS radios have a maximum power of Ѕ watt (500 milliwatt) effective radiated power and integral (non-detachable) antennas. ... FRS and GMRS Channel 1 . ... The FRS/GMRS radios I have transmit more than 1/2 watt when on channels 1-7 and 15-22. ... www.astronomy.net . ...

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• If You Sent Mail, I Never Received It - an Astronomy Net Exploration Forum

... Several of the tasks in the spectral package share a common set of parameters. ... Each task in the spectral package has a hidden parameter which points to the pkgpars parameter file. The parameters stored here include the observed data sets and the model descriptor, and instrument-specific parameters. ... The observed counts and error data set contained in the table file ( *_obs.tab ) produced by qpspec will be the input data for subsequent spectral tasks. ...

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• Introduction to XPA
• COSPAR Capacity-Building Workshops Fellowship Program
• Doug Burke's Perl/S-Lang pages: Structure examples

... INTERCOSMOS 19 . ... The Intercosmos-19 satellite was designed for investigations of the topside ionosphere structure and electromagnetic processes in it. ... The instruments installed onboard Intercosmos-19 were designed and manufactured by scientists of Bulgaria, Poland, Czechoslovakia and USSR. ... The sounding data could be directly transmitted to a receiving station (direct mode) or be stored in the onboard memory device for a certain period and then sent to the Earth (recording mode). ...

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• Formation, stability and decay of inhomogeneus plasma structures in a hot

... FPV 400mw 5.8GHz AV Powerful Transmitter + Receiver (RC5808) Combo . FPV Equipments : FPV Accessories . ... Package Contents : 1 x Transmitter, 1 x Receiver . ... Цвет: бежевый . ... Артикул: 62759_OAB ВАР.1 Цвет: голубой Состав: ткань верха: текстиль, 40% хлопок, 60% полиэстер Страна дизайна: Россия Страна производства: Китай Товар сертифицирован. ... Цвет: черный . ... Цвет: синий . ... Цвет: серый . ... Платье Topshop - Topshop - Topshop . ...

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• AV Transmitter + Receiver (TS351 + RC305) Combo Набор садовника-яркая клумба
• Кабель удлинительный 3.0м Hama 3.5 Jack (M) - 3.5 Jack (F) черный 122314 - HAMA
• Что? Зачем? Почему? Большая книга вопросов и ответов 12296407 Платье Bestia

Stellarium 0.12.3 . ... Classes . ... ClassљList . ClassљIndex . ... TuiNodeEnum Class Reference . ... setValue (QString s) . TuiNodeEnum (const QString &text, QObject *receiver, const char *method, QStringList items, QString defValue, TuiNode *parent=NULL, TuiNode *prev=NULL) . ... virtual TuiNodeResponse љ . ... virtual QStringљ . ... TuiNodeEditable (const QString &text, TuiNode *parent=NULL, TuiNode *prev=NULL) . ... TuiNode (const QString &text, TuiNode *parent=NULL, TuiNode *prev=NULL) . ...

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• Stellarium: TuiNodeColor Class Reference
• Stellarium: TuiNodeDouble Class Reference
• Stellarium: TuiNodeFloat Class Reference