The present paper considers resonant slow waves in 1D non-uniform magnetic flux tubes in dissipative MHD. ... From these analytical solutions we obtain the fundamental conservation law and the jump conditions for resonant slow waves in dissipative MHD. The validity of the ideal conservation law and jump conditions obtained by Sakurai et al. (1991) for static equilibria and Goossens et al. (1992) for stationary equilibria is justified in dissipative MHD. ...

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• A Blinker Model
• Armagh Observatory
• Observations and Data Reduction

... Tpram - time of the PRAM instrument (aquisition computer) . ... Bx - DC magnetic field with a fixed amplitude calibration; X component . ... The color lines present FFT from the AC magnetic field (Waveform); Bwx, Bwy, Bwz - from the bottom. ...

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• Magnetic field restoring
• Space Weather Dials Interpretation Guide
• Current Solar Wind Conditions

... Tpram - time of the PRAM instrument (aquisition computer) . ... Bx - DC magnetic field with a fixed amplitude calibration; X component . ... The color lines present FFT from the AC magnetic field (Waveform); Bwx, Bwy, Bwz - from the bottom. ...

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• Space Research Institute (IKI) Seminar

Due to technical issues, on September 11, 1998 the radiolink was switched to 465 MHz channel. Data acquisition is presently performed only by SRC "PLANETA", Data Receiving Center in Obninsk and Western Siberia Data Receiving Center in Nobosibirsk . For conditions of obtaining data from RESURS-01 N3 please contact SRC "PLANETA". ... Registration of full data stream (61.44 Mbit/s) is performed only by Data Receiving Center, SRC "PLANETA", Obninsk. ...

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Next: Data reduction Up: Spectral observations and data Previous: Observations with the KPNO . Follow-up spectroscopy with this telescope was conducted as a back-up for a main program which needed photometric conditions. So, the observations presented here were obtained in non-photometric conditions and the absolute flux calibration of the data is unreliable. The Cassegrain focal reducer CAFOS of the 2.2m telescope was used with a long slit of 300 3 and a grism of 187 ? ...

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• Equations of condition
• Up-date RC-sources Spectra
• The main observational parameters

... Aromatic dust emission features and emission lines from molecular and atomic hydrogen are detected but they are not particularly strong. The dominant spectral features are emission lines from moderately ionized species of argon, neon, and sulfur, which are used to determine the physical conditions in the ionized gas. The ionized gas excitation shows strong variations on parsec scales, some of which can plausibly be associated with individual hot stars. ... ADS Citation Query . ...

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• Iterative Image Restoration
• Cool dust heating and temperature mixing in nearby star-forming galaxies
• Example of Deconvolution: The HST Image of SN1987A

. I will briefly summarise the methods to estimate the magnetic field strengths of different types of neutron stars and the caveats associated with them. In this context I will present some recent results we have obtained in finding the limits to the field strengths of accreting millisecond X-ray pulsars from the interaction between the accretion disk and neutron star magnetosphere.

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• Some Black Holes are Pink
• Raquel Salmeron - Research Interests and Experience
• Penny Sackett presents a copy of the book, signed by the authors, to John

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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• The Effect of Relativistic Wind on Accretion Flow Parameters
• The equilibrium period
• Binary NS Merging Rate Estimates

Abstract -- The strengths of magnetic fields in interstellar gas clouds are obtained through observations of the circular polarization of spectral line radiation. ... To infer information about these irregularities from the observational data, we develop statistical relationships between the rms values of the irregular component of the magnetic field and spatial variations in the circular polarization of the spectral line radiation. ...

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• Project: PAHs

Magnetic Stars, 2011, pp. ... 2008). ... The origin of magnetic fields of hot massive stars is explained by the fossil field theory, MAGNETISM OF STARS 451 1-5 Be measurements -> 1278 stars 100 N stars 6-10 Be measurements -> 80 stars 50 11-15 Be measurements -> 47 stars 0 20 40 60 80 100 120 140 160 180 The namber of individual measurements The number of individual measurements Figure 1: The number of stars in a single bin versus the number of individual Be determinations for a single star. ...

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• Sun image
• Galaxy sector, archive 2012
• The Present and Future of Small and Medium Size Telescopes

... Unsafe act - a behavioral departure from an accepted, normal, or correct procedure or practice which, in the past, has produced injury or property damage or which has potential for doing so in the future; an unnecessary exposure to a hazard; conduct reducing the degree or safety normally present in an activity. ... Any hazardous unsafe condition, or act that presents a situation of imminent danger to life and/or property requires urgent action. ...

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• media

. Present section of the package enables one to perform following actions: . — . To make selection out of the total number of elements in accordance with the conditions imposed on some element or on a variety of elements. — . to sort the set of elements in order of ascending or descending value of any element. — . to draw the histogram of element distribution for obtained selection. — . To construct dotty picture of minor planet distribution in two– or three–dimension space of elements.

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• Keywords_28
• Keywords_312
• Keywords_327

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

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• Introduction
• Point matching method
• intro3e

... The Astronomical Society of the Pacific (ASP), in partnership with the American Astronomical Society (AAS), has presented the annual Priscilla and Bart Bok Awards to two high-school seniors at the Intel International Science and Engineering Fair held May 9 to 14 in San Jose, California. ... The Priscilla and Bart Bok Awards are given jointly by the ASP and the AAS. ... Upon his death in 1983, the ASP established the Bart Bok Memorial Fund to support educational projects. ...

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• ASP: Astronomical Society of the Pacific to Present 2009 Annual Meeting,

Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 05 - 11.03.2012, Forecast on 12 - 19.03.2012, Carrington Rotations 2121 (04,62.03.2012) SOLAR SUNSPOT ACTIVITY OF THE LAST PERIOD WAS ON AVERAGE LEVEL. ... IMPORTANT OF FLARE ACTIVITY STARTED MARCH, 4th AND TO 11.03 IN CAR OCCUREN- CED X-RAY CLASS X - 3, CLASS M - 12 FLARES, 5 OF WHICH ARE LARGE. ... Class E(1-8A) AR RII/IV CME X/opt. ... NEXT WEEK MARCH, 12 IN ENVIRONMENT WILL COME THE DISTURBANCE FROM LARGE SOLAR FLARE OF MARCH 10. ...

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• http://www.izmiran.rssi.ru/services/saf/archive/en/2011/obzor20110711.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2011/obzor20110725.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2012/obzor20120123.en.txt

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

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• GRB follow-up team
• Observational data and reduction
• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Physics and

... NASA U.S. Spacesuit Knowledge Capture . ... During the program?s existence, more than 65 seminars have captured spacesuit history and knowledge; those that are available at this site have been approved for public release. For questions about the program or presentations, please contact: cinda.chullen-1@nasa.gov or vladenka.r.oliva@nasa.gov . The following presentations consist of video recordings (MPEG-4 and Ogg), transcripts (TXT),and accompanying slides and/or information (PDF). ...

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Iron (Fe) i s extremely reactive with oxygen. ... Archean - Find occurrence of minerals that only form in non-oxidizing environments in Archean sediments: Pyrite (Fools gold; FeS 2 ), Uraninite (UO 2 ). ... Chemical building blocks of life could not have formed in the presence of atmospheric oxygen. ... Oxygen prevents growth of the most primitive living bacteria such as photosynthetic bacteria, methane-producing bacteria and bacteria that derive energy from fermentation. ...

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• Fossil Fuel Primer
• Solar Collection and Energy Transport.
• Comparative Review of Alternative Energies

... Because the DMR instrument is differential and every pixel is multiply sampled, sky maps are produced by solving a coupled system of linear equations (the normal equations) to minimize a chi-squared. ... This is reflected in the algebraic form of the normal equations matrix, so that, if one were to diagonalize the matrix, one would find a single eigenvector whose eigenvalue was identically zero, and the associated eigenvector, viewed as a sky map, would have a constant value. ...

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• Identification and Analysis of Binary Star Systems using Probability Theory
• Calibration and Performance Control for the VLT Instrumentation
• ADASS 2003 Conference Proceedings

TOOLS OF TEST GENERATION FOR SATELLITES CONTROL PROGRAMS Andrey Tyugashev, Ekaterina Myasnikova, Elena Sopchenko S.P. Korolyov Samara State Aerospace University (National Reseach University) The paper presents a research in the field of test automation for testing spacecraft control programs. ... Programmers or designers of spacecraft systems write tests manually. ... Tests are carried out by issuing the control actions on the spacecraft and condition monitoring systems parameters of the spacecraft. ...

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• For the first time Russian university presented its achievements in outer space
• SSAU presented its educational programs at the exhibition AULA-2015
• SSAU's nano-sattelite presented in Brussels