... 84, No. 4, pp. 380­384. i A Generalized Polarity Rule for Solar Magnetic Fields V. N. Obridko and B. D. Shel'ting Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences ... 142190 Russia Received August 23, 2006; in final form, October 12, 2006 Abstract--It is shown that, when all components of the large-scale solar magnetic field are longitudinally averaged, the N ... The large-scale fields spread all over the solar surface. ...

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• Oct-Nov 2003: CORONAS-F/SPIRIT and SOHO/EIT Data
• Eric R. Priest

Proposal Identi cation No.: A1583 Date Received: 2001-Oct-01 21:43:17 Technical Page Proposal Type: Large General Category: Astronomy Observation Category: Galactic Total Time Requested: 210 Hours Proposal Title: Statistically sampling HI and OH Zeeman Splitting with Absorption Lines ABSTRACT: We request 210 additional hours to compete the original objectives of our large project (01-JUN-99 deadline). ... We have met the second goal of this project, and initial results are already published. ...

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• Public data products
• The Evolution of Galaxies Seen Through The Neutral Hydrogen Line The Evolution
• AGES - the Arecibo Galaxy Environment Survey

PUBLICATION AGREEMENT AND COPYRIGHT ASSIGNMENT Astronomical Society of the Pacific Conference Series (ASPCS) RETURN TO EDITOR Date: _________________ With regard to the original and previously unpublished paper entitled ___________________________________ ____________________________________________________________________________ ... To protect the copyright of this book, the original copyright notice as it appears in the ASP Conference Series should be included in the credit. ...

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• http://www.astrosociety.org/events/2009mtg/copyright2009.doc
• http://www.astrosociety.org/events/2008mtg/copyright2008.doc
• ASP's 119th Annual Meeting - Conference Proceedings

... Files in red?history) . ... The Sun . ... Large sunspots may be occasionally seen by the unaided eye, with the sun near the horizon and dimmed by thick haze. ... Year after year, beginning in 1826, on every clear day, Schwabe would scan the sun and record its spots, until 17 years later he began to suspect a regular variation . ... Some, led by Rudolf Wolf, examined old records to reconstruct earlier sunspot cycles, while Edward Sabine in England in 1852 found a similar periodicity in magnetic...

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• The INTERBALL Tail PROBE orbital elements
• About modification of the INTERBALL orbital elements
• Two points (INTERBALL-1 and MAGION-4) observations of magnetopause motion

Term mixture regarding solar chemical composition refers to relative abundances of heavy elements. Abundances of hydrogen and helium cannot be determined reliably from observations, therefore concentration of these elements are not taken from observational data. ... Table contains only elements which are abundant enough to be included into opacity and equation of state computations. ... First "low-Z abundances" to be published were AGS05. ... 5.5 . ... 6.22 AG89 : Anders E., Grevesse N. 1989. ...

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• Publications

... Recent Topics . ... MAO main . ... Fw: [eas-aff] Exploring the road to Open Access Publishing . ... To: "EAS Office" . ... Subject: [eas-aff] Exploring the road to Open Access Publishing . ... wishes to bring to your attention the EAS report "Exploring the road to Open . ... on Open Access Publishing, which you will also find on the EAS website at: . ... test.mao.kiev.ua/images/postbyemail/open_access_publishing.pdf . ... test.mao.kiev.ua/images/postbyemail/open_access_publishing1.pdf . ... MAO NASU...

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• MAO NASU :: Topic: Fw: PHD offer (1/1)
• Observations - Page 2
• MAO NASU :: Topic: Fw: e-EPS | Facts and Info from the European Physical

... Watchouts . ... Any XMM-Newton users, who need to convert OM count rates in the optical and UV filters into fluxes (expressed, e.g. , in erg/cm/cm/s/A), can do it by following any of the methods we outline below. OM count rates can be obtained with SAS. ... UVW1 . ... UVM2 . ... convert from count rate, obtained with SAS (files *SWSRLI*, corrected count rate in CORR_RATE column), to flux, selecting the most appropriate factor for the chosen spectral type and filter from the following Tables: . ...

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• Description
• Proposal change classes
• Comments

National Aeronautics and Space Administration . ... Gregory Errol Chamitoff (Ph.D.) . NASA Astronaut (Former) . ... NASA EXPERIENCE: In 1995, Dr. Chamitoff joined Mission Operations at the Johnson Space Center, where worked as a Guidance and Control Flight Controller. ... SPACE FLIGHT EXPERIENCE: Expedition 17/18 - In 2008, Dr. Chamitoff served as the flight engineer and science officer for a 6-month mission aboard the International Space Station during Expeditions 17 and 18. ... OCTOBER 2013 . ...

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• JSC History Collection

Observational data on solar activity is a basement for investigation of processes that take place on the Sun and interplanetary space, with data of long-term observations being of special importance. ... Subsection "Sunspot groups" is the catalogue of all sunspot groups that were observed in the given year. ... For every day of observation of the group the area of the group, the area of the largest spot (both areas - in millionths of solar hemisphere) and number of spots in the group are presented. ...

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• http://www.gao.spb.ru/english/personal/malkin/publ/zm06h.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm11c.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm134.pdf

... Astrometric Observations of the Second, Third, and Fourth Satellites of Uranus I. S. Izmailova, S. A. Korotkiib, M. V. Ereshkob, and A. V. Stepurab a Pulkovo Observatory of the Russian Academy of Sciences, Pulkovskoe shosse 65­1, St. Petersburg, 196140 Russia b Ka-Dar Observatory, 1-i Neopalimovskii per., ... ASTROMETRIC OBSERVATIONS 43 To determine the center coordinates and other parameters of a satellite or a star image, we solved a redundant system with the nonlinear least-squares method. ...

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• Pulkovo Databases

... Contact A Problem of an estimation of accuracy of the asteroid CCD observations . The Minor Planet Center supported by the Interntional Astronomical Union is the main office for keeping observational data of the small Solar System bodies and their investigations. ... At Pulkovo Observatory we are estimating an accuracy of the CCD asteroid observations obtained by amateurs and professional astronomers all over the World using the MPC database. ...

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Databases (NSDC) of the Natural Planetary Satellites. Sources and references of the data . NSDC: Database of astrometric observations of Natural Planetary Satellites . ... The observational data are taken from various sources: . ... The catalogue of observations of the Martian satellites published by Morley T.A. A catalogue of ground-based astrometric observations of the Martian satellites, 1877-1982, Astronomy and Astrophysics Supplement Series. 1989. vol. 77. n. 2. p. 209-226. ...

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• IMCCE-SAI: Natural Satellites Data Center. Observations
• Technical Details
• Data bases of Natural Satellites. Documentation. Structure

... Up: Data Analysis and Processing Techniques . ... Also, a method for quality control of CCD observations is suggested. ... Everyone who observes a celestial object using a CCD detects moving celestial objects as a ``by product''. ... We hope that our investigations may be useful for near-Earth space control and also for searches of the moving celestial objects through analysis of old and new CCD frames obtained at any amateur or professional astronomical observatory. ...

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• Restoration of HST WFPC2 Images in Gyro-Hold Mode
• The Status of the Second Generation Digitized Sky Survey and Guide Star Catalog
• Observation Interval Determination for the Chandra X-ray Observatory

... I determine th as a time period (from some moment in the past till the present moment) during which papers responsible for 1/2 of the total citation index were published. Parameter Nt represents averaging of the citation index over this period: Nt = C.I./2th 1 Intro duction The problem of estimation of an impact of a scientist (or a group of them) is an actual one (see, for example, [1] and references therein). ... One published in 1965 a paper with C.I.=5000, and nothing after that. ...

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• Introduction
• Determination of the 'diffusion coefficient'.
• Initial Distributions of Binary Parameters

... Determining the nominal roll angle for stable intervals . ... We found the necessary information in a file 'rh*.ao', which has a binary extension table for each obi. ... Unlike the question of determining the nominal roll angle, we know of no a priori indication of this problem (although the guide star configuration may be the cause, or at least associated with this condition): it is necessary to examine the source position for each obi. ... The guide star record is at the end of the 'anc file'. ...

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• *wcscoord* -- all purpose coordinate conversion
• *fixsaoreg* -- restore SAOimage region to original image (physical) coordinates
• False Alarms and Aliasing

... A recent study found that a type Ia supernova's original star could be anywhere from 0.9 to 1.4 times our Sun's mass. Astronomers use these blasts' brightnesses to estimate distances, so are those measurements now incorrect? ... Get instant access to subscriber content on Astronomy.com! ... If you are already registered on Astronomy.com, please log in below. ...

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• Do astronomers know of or suspect any stars that were original members of the
• If a supernovaт??s original star is massive enough to form a black hole, why is
• Chandra captures X-ray echoes pinpointing distant neutron star | Astronomy.com

... Russian . The Astronomical Circular (Astronomicheskii Tsirkulyar) is published online by the Eurasian Astronomical Society and Sternberg Astronomical Institute, Moscow State University. ... All papers are refereed. All published papers are indexed in the SAO/NASA Astrophysics Data System . ... See this directory for sample files (template for a paper in English and in Russian , style file , sample figure and sample PDF file for a paper in English and in Russian ). ...

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.

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• Physics 410/510 Observational Cosmology
• Inflationary Epoch
• Formation of the Earth's Moon

... Shortly after its discovery it was determined to be in a highly elliptical path near Jupiter and on a collision course. ... The size and mass of the original body and the individual fragments is as of this writing still highly uncertain. ... Between 16 July 1994 and 22 July 1994 the fragments impacted the upper atmosphere of Jupiter. ... The pictures were posted to the Net within hours of the impacts and caused severe overloading on some ftp and WWW sites. ... JPL's SL9 page . ... Small Bodies .. ...

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• Bilbio
• SAI SN RESEARCH GROUP
• A little Notes on Web techniques by Oleg Bartunov

To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) METEOR OBSERVATIONS WITH MINI-MEGATORTORA WIDE-FIELD MONITORING SYSTEM S. Karpov, 1, 3 N. Orekhova2 G. Beskin, 1, 3 A. Biryukov3,4 S. Bondar,2 E. Ivanov,2 E. Katkova,2 A. Perkov, and V. Sasyuk3 RESUMEN 2 Favor de prop orcionar un resumen en espanol. ... The faintest detected meteors has the peak brightness about 10 mag, while the ma jority - from 4 to 8 mag. ... 2010; Karpov et al. 2013; Beskin et al. ...

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• astro-ph