Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 15 - 21.04.2013 , Forecast on 22 - 29.04.2013, Carrington Rotations 2135, 2136 (21,5.03; 17,78.04.2013) SUNSPOT-FORMING ACTIVITY OF THE SUN REMAINED ON THE AVERAGE LEVEL. ... NEXT WEEK THE LEVEL OF SUNSPOT ACTIVITY IS EXPECTED TO BE THE AVERAGE. ... BY BY SOHO AND STEREO CORONOGRAPHS DATA THERE WERE OBSERVED SOHO 54 CME FROM WHICH ONE WAS THE TYPE OF "PARTIAL GALO III", AND SIX WERE THE TYPE OF "PARTIAL GALO II". ...

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• http://www.izmiran.rssi.ru/services/saf/archive/en/2012/obzor20120820.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2013/obzor20130909.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2013/obzor20130916.en.txt

Some peculiarities of orbits of observed comets. ... Icarus, 2005 Simulation and reality Distribution of anti-perihelia of short-period comets with e 0.9 ( ecliptic coordinates ) Distribution of anti-perihelia of short-period comets with e 0.9 ( ecliptic coordinates ) Distribution of anti-perihelia of long-period comets with 0.9 e 1 ( ecliptic coordinates ) ­ ...

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• http://www.gao.spb.ru/english/personal/malkin/publ/zm08g.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm135.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm12b.pdf

PROJECT SUMMARY (max 3000 characters) The principal goals of the project are the observational and theoretical investigation of complex cosmic objects where the processes of dust scattering, absorption and emission play significant roles. ... Development of light scattering theory and computer codes to calculate the optical properties of non-spherical inhomogeneous particles and laboratory measurements of light scattering characteristics of irregularly shaped particles. ...

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• Polarization properties (transmitted radiation)

If you can see this, it means that the installation of the Russian Apache web server software on this system was successful. ... This page is here because the site administrator has changed the configuration of this web server. ... The Apache Software Foundation, which wrote the web server software this site administrator is using, has nothing to do with maintaining this site and cannot help resolve configuration issues. ... You are free to use the image below on an Apache-powered web server. ...

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Trail encounter . ... Expected meteor rates . ... The Leonids are the debris of Comet 55P/Tempel-Tuttle. ... The Earth's passage right through the centre of trails is associated with the most spectacular meteor displays (studies show that, as well as how close to the centre of the trail you are, the strength of the display also depends on how far along a trail's length you are). ... The encounter with the 1932 trail will lead to enhanced meteor activity: a nice outburst, but below storm level. ...

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• Armagh Observatory
• Leonid Meteors by Moonlight
• M.E. Bailey, Director

The course will start on Tuesday 29th April 2008 and end on Friday 6th June 2008. Lectures" will be held on Tuesdays 2-3pm and Fridays on Fridays, 9.30-10.30 and 11.00 - 12.00. ... This will not be a conventional lecture course: it is intended to be far more hands-on and practical. Notes will be posted ahead of each lecture and everyone will be expected to have read and digested them ahead of each lecture. ... Statistics Notes: Part 1 . ... Radio Astronomy Notes: Part 1 , Part 1 . ...

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• Lecture 19: Probability Distribution Functions
• Lesson 1: Using Uncertainties
• Raquel Salmeron - Research Interests and Experience

... One of the most widely used tools of Fourier analysis is the Parseval theorem. It enables the experimentalist to view how the `energy' in the signal is distributed among frequencies. The Fast Fourier Transform (FFT) algorithms have made power spectra one of the obvious diagnostics tools during data acquisition, and energy maps are a versatile alternative. ... The result is an energy map (Fig. 9), showing the distribution of energy corresponding to the wavelet map (Fig. ...

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• Bugs found so far in XFree86/OS2 3.3
• Bugs found so far in XFree86/OS2 3.3.1
• Bugs found so far in XFree86/OS2 3.3.3

... CYGAM FLIGHT IN THE HIGH APOGEE ORBIT? Distribution of the Galaxy diffuse emission with high angular resolution allowing to refine the spatial distribution of the cosmic-ray protons in the Galaxy. More than 1000 compact sources with the fraction of degree location accuracy and continuouse monitoring of their flux time variation. Up to 10 new gamma-ray pulsars emitting in the very high energy range. Several high energy gamma-ray bursts with the fraction of degree localization accuracy. ...

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• INTERBALL TAIL PROBE Long-term Situation Analysis for the 1998
• The summary plot of time distribution of the multisatellites magnetic
• Main results of the experimental and theoretical research completed in 2010

... This year SSAU provides 1429 state-funded places for admission in all kinds and directions of educational programs. ... In addition, SSAU Admission Committee notes the substantial increase in interest from the foreign applicants this year. The number of applications from foreign countries has already surpassed last year's totals - 76 applications. Based on the experience of admission campaigns of previous years, SSAU expects summer 2014 to enrol about 150 foreign students in the university. ...

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Pulverizarea termic, ISIM, Timioara, Romania (2000) FINITE ELEMENT ANALYSIS OF THE BONDCOAT INFLUENCE ON RESIDUAL STRESS DURING THE PLASMA THERMAL SPRAYING OF PARTIALLY STABILISED ZIRCONIA P. Fogarassy(1,2), F. Rotaru(1), N. Markocsan(1), B.B. Straumal(3) (1) Institutul Naional de C&D Нn Sudare i нncercri de Materiale (ISIM) Timioara, ROMANIA, (2) Universitatea "Politehnica" Timioara, ROMANIA (3) I.V.T. Ltd. ... Figure 4.7 present a detail of the normal X stress distribution. ...

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• http://www.issp.ac.ru/lnep/pdf/tartakovskii2000c.pdf
• http://www.issp.ac.ru/lek/shovkun/art18.pdf
• PLDS-3, Chernogolovka, Russia, 2001 - Attendance of the Conference

PHOTOMETRIC SEARCH FOR BLACK HOLES IN DORMANT X-RAY TRANSIENTS ґ ґ Aleksander Sadowski1 , Janusz Ziolkowski2 , and Krzysztof Belczynski3 ё Astronomical Observatory of Warsaw University, Al. ... Such definition means that our statistics for the number of expected BH X-ray binaries include both transient and persistent systems. ... If this value is 2 M , then, according to our calculations, Galaxy contains some 15 000 to 40 000 of BH X-ray binaries (and some 30 000 to 250 000 of NS X-ray binaries). ...

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• http://hea.iki.rssi.ru/integral06/papers/E36_Stephen01-07May07_17:57:56.pdf
• http://hea.iki.rssi.ru/conf/hea2007/presentations/26.12.2007/09-popov.pdf
• http://hea.iki.rssi.ru/integral06/papers/I32_Kalemci01-13Feb07_15:37:29_bandw.pdf

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

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• Index of /lk/source
• The NMW survey homepage

XmCCD ----- The programs provided here offer a Linux graphical user interface to astronomical and scientific CCD cameras. ... It is the latest one they offer and the files included allow support for Android and Mac OS X. This distribution of XmCCD includes source code to utilize the SBIG shared library libsbigudrv.so with a Motif-based graphical user interface. ... The XmCCD source package includes and will install: SAOimage ds9 xpa cfitsio SAOimage is the primary image display for XmCCD. ...

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• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.2.2/README
• http://www.astro.louisville.edu/software/sbig/xmccd-5.1/README
• Distribution (ImageJ API)

... For this purpose, catalog entries for stars within 12њx6њ region centered at 12h 20m right ascension and 33њ declination were examined. ... In Figure 1, the distribution in Johnson V magnitude of all Tycho catalog entries for stars within 12њx6њ region centered at 12h 20m right ascension and 33њ declination is plotted . ... Figure 1 : Distribution of magnitude in Johnson V. This is for the 510 stars from the Tycho catalog in a 12њx6њ area in the center of the northern survey region. ...

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• Analysis of temperature measurements
• Mirror actuators
• Fiber Positioning System Performance

... Sun images . Magnetic storms online . Sun flares . Geomagnetic activity forecast . ... September : 2009 . ... No magnetic storm is expected . From 1 October 2009 to 27 October 2009 no magnetic storms and disturbances are expected 1 October 2009 - 27 October 2009 . Probability of a magnetic storm . ... Probability of a strong magnetic storm . ... Last updated: October 1, 2009 00:00 UT . ... 7(499)132-65-96, Fax: +7(499)132-65-97 . ...

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• Space weather forecast February 10, 2006
• Space weather forecast February 10, 2009
• Space weather forecast February 01, 2008

FEATURES OF THE HYDROGEN DISTRIBUTION AROUND LUNAR CRATERS PROCLUS AND KEPLER. ... In result of analysis of the data Lawrence and Feldman constructed the hydrogen distribution on the lunar surface [1]. ... However, the authors shown, that EN flux data features may be explained by other element abundance in the lunar soils, namely: Si, Ca, Gadolinium (Gd), Samarium (Sm) and Fe. ... Using of the Feldman's interpretation of the Lunar Prospector data [8], we constructed hydrogen distribution map (Fig.1). ...

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• http://selena.sai.msu.ru/Rod/Publications/ms34/MS060.pdf
• http://selena.sai.msu.ru/Bus/Publications/m44_14_busarev_etal.pdf
• http://selena.sai.msu.ru/Pug/Publications/Pugacheva%20LPS%2041.pdf

... For a semple of red giants comprising about 2000 stars, the distributions of metallicity [Fe/H] are given. ... The center of the distributions of giants in both galactic poles is found to demonstate a statisticaly significant gap similar to the one found earlier for the late main-sequence stars. The implications of the metallicity distribution properties for the problems of the chemical evolution of the galactic disk are discussed. ...

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• Vladimir Marsakov Publication List
• Vertical Structure, figures
• RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, figures

... Planets . ... Earth Satellites . ... The newly discovered ?mega-Earth? ... Its sibling, the lava world Kepler-10b, is in the background (the two planets? proximity is grossly exaggerated) .€а Kepler-10c has a diameter of about 29 000 km, 2.3 times as large as Earth, and weighs 17 times as much. ... The first mega-earth to be discovered is Kepler-10c which orbits a star lying about 560 light years from the Sun in the constellation Draco. ... Astronomers Find a New Type of Planet: The ?Mega-Earth? ...

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• Whatever Happened to the Beagle 2 Mars Lander | Astronotes
• Soyuz 11 and Salyut 1: The Truth About the 1971 Space Disaster | Astronotes
• Ice Worlds at Armagh Planetarium | Astronotes

... The hotter the gas, the faster they move, and the more energy each of them holds. The free ions and electrons in a plasma behave the same way. Knowing the temperature of the high atmosphere of Earth, or that of the Sun, we can calculate energies expected of ions and electrons found there. However, ions and electrons actually observed in space are often much , much more energetic, and may move at a respectable fraction of the velocity of light (300,000 km/sec or 186,000 miles/sec). ...

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• Environmental Health Information Processing System - Executive summary
• Russian HEND for NASA mission 2001 MARS ODYSSEY
• Plasma theories [Oulu]

... Parallel Tree N­body Code: Data Distribution and DLB on the CRAY T3D for Large Simulations U. Becciani, V. Antonuccio­Delogu, M. Gambera and A. Pagliaro Osservatorio Astrofisico di Catania, Citt‘a Universitaria, Viale A. Doria, 6 -- I­95125 Catania ­ Italy R. Ansaloni Silicon Graphics S.p.A. St.6 Pal. ... A bodies data distribution ranging from contiguous blocks (coarse grain: cdir$ shared pos(:block,:)) to a fine grain distribution (tf) (cdir$ shared pos(:block(1),:)) was adopted. ...

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• A Color Analysis of NICMOS Parallel Observations
• Design and Status of the NICMOS Cryocooler
• Introduction