The Sun 59 Acceleration of electrons in a large-scale electric eld of coronal magnetic loops V.V. Zaitsev Institute of Applied Physics, Nizhny Novgorod, Russia Introduction The main part of the energy, released during solar and stellar ares, goes on the acceleration of energetic particles. ... By this, in the case of a presence of a magnetic eld B j B j j E j in a plasma particles will be accelerated bya The Sun 61 pro jection of electric eld onto a magnetic one Ek = jEBj . ...

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• RADIOSUN Workshop 2014
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... part 1 | ... The Basic Stages in Earth's Pre-geological Development . ... After fragments of the Vortex sleeves separated, whirlwinds of second and third orders ("NC" - new micro-vortex) were generated- future planet cores and their satellites - all of them developing independently, governed by the common laws of development of cosmogenic vortexes. ... Our planet's core today is comprised of considerably deteriorated cosmogenic vortex; consequently, the Earth has a moderated magnetic field. ...

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• The new concept of formation and development of the Solar system

An expanding plasmon model for the radio outbursts of Cir X­1 By J o a n G a r c i a Departament d'Astronomia i Meteorologia, Universitat de Barcelona, Av. Diagonal 647, E­08028 Barcelona, Spain The group of radio emitting X­ray binaries (XRB's), such as SS433, Cyg X­3, LSI+61 ffi 303, Cir X­1, etc., exhibit highly variable bursting radio emission interpreted as synchrotron radiation from relativistic electrons. ... Before modelling the data points, the quiescent spectrum of Cir X­1 (Haynes et al. ...

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Next: CCD Scientific Performance Up: CCD Operation Previous: CCD Operation . A visible light photon releases only one electron-hole pair, and consequently many photons must be collected in each pixel for a measurable signal to be produced. ... This use as an imaging X-ray spectrometer requires that no more than one photon is incident on each pixel in any image frame, which imposes a requirement that image collection times be limited to ~seconds for typical astronomical applications. ...

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. Name of process . Radiative Transitions . Phoionization . Photorecombination . Dielectronic Recombination . Autoionization . Electron Impact Excitation . Electron Impact Ionization . Charge Transfer . Proton Impact Excitation and Ionization . Collisions with heavy particles . Auger Processes .

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ON THE CORRELATION BETWEEN SPECTRA OF SOLAR MICROWAVE BURSTS . AND SPECTRA OF PROTON FLUXES NEAR EARTH . ... which is equivalent to the power-law index of the integral energy spectrum of protons registered near the Earth orbit in a range of 10-100 MeV , on the one hand, and parameters of microwave bursts such as a ratio of peak fluxes at two frequencies (e.g., 9 and 15 GHz) and a microwave peak frequency f m as well. ...

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MATHEMATICAL MODELING: . ... This model is developed on the base of the probabilistic description of the collisional aeronomical processes and is realized on a computer as the numerical system (stochastic model). ... Shematovich, V.I., Bisikalo , D.V.             Nonequilibrium processes in the planetary and cometary atmospheres. ... In Russian) . ... Piarnpuu , A. A.; and Shematovich, V. I.       Construction of structural stochastic models of collision processes in rarefied gas media (abstract) . ...

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Next: Three-dimensional Data Analysis in IRAF and ZODIAC+ . ... A data analysis system has been developed at SRON, which has been designed to allow rigorous control of the quality of its processed data products. ... This means recording all parameters of all steps which lead to the establishment of the final data products (Figure 1 ). ... Figure: A processing pipeline is a sequence of tasks with several input/output files and parameters, which pass data from one task to the next. ...

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PLASMA PROCESSING REACTOR ON A BASE OF BEAM PLASMA DISCHARGE . ... At IRE RAS the effect of ion beam emission from the region of beam-plasma discharge (BPD) with energy best suited to the tasks of etching and deposition of materials for microelectronics has been discovered. ... Our studies [ 1 - 7 ] showed that the source of a flow of ions with controllable energy and geometry could be created on a base of beam-plasma discharge (BPD). ... Beam plasma reactor schematic . IRE RAS 1996-20 10 ...

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... GCR and SCR are primary cosmic rays. 10-15 years after the discovery of cosmic radiation (1919) there emerged two main avenues of investigation in the physics of cosmic rays (CR): 1) nuclear - elucidation of the origin of elementary particles and nuclear interactions; and 2) astrophysical (space physics) - solution of the problem related to the origin and variations (changes in intensity) of CR. ... Besides, the CR flux in interplanetary space is, strictly speaking, not isotropic. ...

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BNO is in Baksan Gorge at the Northern Caucasus . ... The Baksan Underground Scintillation Telescope (BUST) of volume 3000 cubic centimeters at a depth of more 300 m. The mountainous plant ANDYRCHI to register wide air showers located over BUST on the area 5*10 4 square metres. The complex of surface plants KOVER including a large muon detector, a scintillation telescope and a neutrino monitor meant for studying the hard component of cosmic rays and wide air showers. ...

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... Direct data transmission rate (Mbps) . ... the density of electron fluexs with energies in four bands from 0.04 MeV to 1.7 MeV; . ... sensor (TV, IR) data and heliogeophisical information (HGI) transmission to data receiving and processing centers at a rate of up to 2.56 Mbps; . ... 1.76 GHz - TV- and heliogeophysical information and DCLI's data transmission to data receiving and processing centers; . 7.5 GHz - TV- and heliogeophisical data transmission to data receiving and processing centers; . ...

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... 2003). ... RHESSI, (HXR) , HXR- . ... 15) n = n0 1+(bm - b)l2 (15) (1) (14), bl(bm - b) , ME = ME0 1+(bm - b)l2 33 1 2007 (16) 67 ME0 - , : ME0 = np0 Ne0 . ... ME = ME0 1+(bm - b) (18) (17) ME/ME0 6 5 4 a 3 b 2 c 1 1.0 0.8 0.6 I (З) a 60 40 20 0 0.2 b c 0.4 0.6 (b- 1)/(bm - 1) 0.8 1.0 0.4 0.2 0 () 100 80 (17), (18) . ... 33 1 2007 5* 68 , 1.0 () 0.8 шгкгЭ HXR-ЫСЮл~ТЬЫfl, з 10-8 йгкгЬА в-1 ЭЧ-1 0.6 0.4 0.2 0 1.0 8 (З) 6 a b c 0.8 0.6 l 0.4 0.2 0 a 4 2 b c 0 0.2 0.4 0.6 (b - 1)/(bm - 1) 0.8 1.0 . ...

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• http://www.tesis.lebedev.ru/en/docs/126.pdf
• http://www.tesis.lebedev.ru/docs/129.pdf
• http://www.tesis.lebedev.ru/en/docs/124.pdf

The radiation belts around the planets are the interrnal regions of planets' magnetospheres where the own magnetic field of a planet keeps the charged particles (protons and electrons) having the great kinetic energy. ... They usually distinguish the Earth's internal and external radiation belts. the internal radiation belt of the Earth has the maximum particles density (mainly protones) over the equator in the height of 22 thousand km. ... Jupiter and Saturn have the powerful radiation belts. ...

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RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . 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 Publication SSRT - Siberian Solar Radio Telescope . ...

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• Radioastrophysical department ISTP RAS SB

FrancoRussian Workshop « Stochastic Processes in Physics and Biology », August 17 ­ 19, 2009 10.00 ­ 10.15 10.15 ­ 11.00 11.00 ­ 11.45 11.45 ­ 12.30 12.30 ­ 13.15 13.15 ­ 15.00 15.00 ­ 15.45 15.45 ­ 16.30 16.30 ­ 17.15 17.15 ­ 17.30 17.30 ­ 18.15 18.15 ­ 19.00 20.00 Monday, The Ising rain stays mainly in the plain 11.00 ­ 11.45 V.MALYSHEV. ... Mean-field models of queuing networks 13.15 ­ 15.00 Lunch Section chairman: V.HAKIM 15.00 ­ 15.45 S.NECHAEV. ...

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High Energy Astrophysics: Course Outline 1 Some useful information Lecturer Geoff Bicknell, Research School of Astronomy & Astrophysics Contact details: Telephone RSAA: (02) 6125 9088 Email geoff.bicknell@anu.edu.au Course Webpage: http://www.mso.anu.edu.au/~geoff/HEA/HEA.htm 2 What is High Energy Astrophysics? High energy astrophysics (HEA) is the study of astrophysical phenomena that involve particles of "high energy". ... All lecture notes and the problem set will be available via my web page. ...

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• Mike Bessell, MSSSO - Images
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• Marc White - Astrophysicist - The Australian National University

Next: A Universal Diagram for Up: ``Ecology'' of Magnetic Rotators Previous: The Corotation Radius . The interaction of a magnetic rotator with the surrounding plasma to a large extent depends on the relation between the four characteristic radii: the stopping radius, , the gravitational capture radius,   , the light cylinder radius,   , and the corotation radius,   . ... Hence, the classification of the interaction regimes may well mean the classification of magnetic rotators. ...

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... Comet Animation . ... Comet structures are diverse and very dynamic, but they all develop a surrounding cloud of diffuse material, called a coma, that usually grows in size and brightness as the comet approaches the Sun. ... As comets approach the Sun they develop enormous tails of luminous material that extend for millions of kilometers from the head, away from the Sun. ... The evaporated molecules boil off and carry small solid particles with them, forming the comet's coma of gas and dust. ...

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Blackholes2 Forum Message . Forums: . ... Firtual Particles Are Not Only Particle Pairs . ... Posted by Richard Ruquist on October 19, 2004 12:03:20 UTC . ... Vacuum production of virtual particle pairs cannot violate the uncertainty principle. ... This theory is dual to the particle theory of gravitons. ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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