In this method the fields outside and inside a particle are represented by expansions in term of proper basis functions (practically always the vector spherical harmonics). Since the particle surface does not coincide with the coordinate surface, it is impossible to satisfy the boundary conditions exactly, and the expansions are limited by a finite number of terms, and the boundary conditions are considered in a finite set of points (matching points). ...

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• intro3e
• Wavelength dependence
• Polarization properties (transmitted radiation)

... Status of the numerical solutions and validation 2. ... Coupling of "solid" Earth components, e.g. core ­ mantle (Dehant et al.) ... Consistent relativistic formulation of Earth rotation (Gerlach, Klioner, Soffel) Status of the numerical solutions - 2 · The results from numerical solutions suffer from ­ Simplified solid Earth models ­ Incomplete Earth system models or neglecting of certain parts or neglecting of certain coupling mechanisms ­ Methodological limitations of computations...

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• http://www.gao.spb.ru/english/personal/malkin/publ/zm03e.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/vavilov.pdf

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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• VISTA - Visible and Infrared Survey Telescope for Astronomy

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• Trend Extrapolation
• Fabry-Perot Images of Spiral Galaxies
• The Galaxy Gallery: Messier Objects

... Pointers to Pointers . ... Pointers to a Function . ... We have introduced some advanced pointer issues already. This chapter brings together some topics we have briefly mentioned and others to complete our study C pointers. ... main(int argc, char **argv) . ... These are the only arguments main accepts. argc is the number of arguments typed -- including the program name. argv is an array of strings holding each command line argument -- including the program name in the first array element. ...

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• Pointers
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The Olympiad participants are not supposed to study at any institutions of higher education (university or school which can be considered technical colleges). ... Only students did not participated at the IAO or APAO of the current educating year may participate in SiberiaOpen (that is, during an educating year - since autumn till spring - a student may participate in IAO or in APAO or in "Siberia Open", not in any two of these Olympiads). ... m - those who finish school later than in 3 years; . ...

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• III International Astronomy Olympiad, Problems to solve
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... Up: Algorithms . ... The imaging problem can be described as an optimizing problem in mathematics. ... Computer simulations of rotating modulation collimator imaging show that the quality of images from this method is better than that from the traditional cross-correlation method. ... The imaging problem is: . ... The results show that this algorithm can be used in the imaging problem and usually results in a better image than that obtained from a traditional method such as cross-correlation. ...

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• ADASS 2003 Conference Proceedings
• Modelling Spectro-photometric Characteristics of Nonradially Pulsating Stars
• Time Series Analysis of Unequally Spaced Data: Intercomparison Between

ATMoB "Double Star Award " Guidelines Purpose: To promote observing among the membership of the Amateur Telescope Makers of Boston ­ in particular, double, triple, and multiple stars. Introduction: Double, triple, and multiple stars are the "Rodney Dangerfields" of the night sky. ... W hile they can be observed under a variety of sky conditions, double stars ­ especially close ones ­ are best viewed on nights when the seeing is steady. ... The direction from a star to Polaris is north. ...

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• http://www.atmob.org/about/observing/awards/files/open_cluster_instructions_2011-02-01.pdf
• http://www.atmob.org/about/observing/awards/files/globular_cluster_instructions_2011-02-01.pdf
• http://www.atmob.org/library/member/brewster/SolarSystemModel.pdf

... ON THE ROLE OF LARGE-SCALE PLASMA IRREGULARITIES AT THE FINAL STAGE OF ANOMALOUS ABSOPTION DEVELOPING UNDER HF HEATING OF THE IONOSPHERE . ... Fig. ... With the aid of numerical statistical modeling based on multiple ray tracing it is shown that in presence of large-scale irregularities the reflected signal amplitude mean value is increased significantly. ... Dependence of the mean amplitude of the reflected from the ionosphere signal on the large-scale (10-50 km) electron density irregularity level...

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• Vladimir Marsakov Abstracts
• Anomalous Absorption Theory
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These observations are aimed at fully charactering FORS1 photometric system (UBVRI zero-points, color-terms and extinction coefficients) for the Tektronix 2048x2048 pixel CCD (24µm px) . To this aim, the two Landolt/Stetson photometric fields SA95 and SA101 will be observed on a number of epochs and at different airmasses during February and March 2007. ... SA101 . ... OBs for SA101 have to be observed during evenigh twilight (exceptions are expected for the second half of March) . ...

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• Synthetic Star Forming Region HRDs
• The SPHERE instrument attached to the VLT
• Events and rules

Optimal transportation, curvature flows, and related a priori estimates Alexander Kolesnikov Moscow 2010 1 Curvature flow Shrinking family of (convex) surfaces At, where every point x A on the curvature of A at x x = -K (x) · n(x). Here K (x) is the (Gauss) curvature of At at x. Approaches to the curvature flows · 1) Solving a parabolic nonlinear equation with smooth data ( R.S. Hamilton, R. Huisken .. ... curvature flow x = -td where t = (x). ... C1(M ) sup | ... Let F (r, ) be a smooth function. ...

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• http://www.mccme.ru/~smirnoff/papers/oberwolfach11.pdf
• http://www.mccme.ru/circles/oim/mmks/works2013/zimin2.pdf
• http://www.mccme.ru/circles/oim/mmks/works2013/zimin.pdf

... The INPUT element is used for a wide variety of different kinds of entry fields within HTML fill-out forms. ... These are used for entering short text strings, like peoples names, numbers and dates. ... The NAME attribute is used to identify the field when the form's contents are converted to the name/value list. The VALUE field can be used to initialize the text string. ... The VALUE attribute can be used to initialize the text field for these users. ... It defaults to TEXT. ... NAME . ...

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• rtftohtml Users Guide - 4 Special Processing
• Redirecting standard input and output
• Removing files that have links

... 't impress me I won't feel sorry for you You chose what you wanted to be But I hope I don't live to see that day No, not for me @ SONG : Reality - When You Die 6:33 The final chapter's finished The curtain is about to fall Ending mediocre life Nothing to be proud of at all Thinking back now Despising yourself Feelings oppressed Always ready to bow It wasn't real life In fact ...

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• http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/d/duran.duran/the_promise
• Pointers
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This section of AMPLE enables one to make ephemeris calculations in various coordinate systems (spherical, rectangular) connected with different main planes (equator, ecliptic, horizon) and having origin in different points: geocenter, any point on the Earth surface, the Sun, any major planet, any minor planet. The choice of some minor planet as a center gives possibility to find approaches of the minor planet with any set of major planets and minor planets. ... equinox . 1950 2000 true . ...

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... It is found that the correlation coefficients between these two parameters calculated separately inside and outside the sunspot formation zone ±30 have cyclic variation and occur in anti-phase. This suggests different mechanisms of formation of the corona in the fields of small, medium, and large scales. ... The relationship between the coronal green line brightness (CGLB) and the magnetic field strength (MFS) has been investigated by constructing the corresponding synoptic maps for the 1977-2001. ...

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• IZMIRAN: Laboratory for Physics and modeling of the ionosphere - publications -

... Тhis new concept touches our simple lives, yet for those intrigued by the natural sciences, especially experts deeply engaged in the 'eternal' questions of general geology and astronomy, it is all the more fascinating. The problems to be faced by any theory for the formation of the Solar System . Any theory has to account for certain rather tricky facts about the Solar System. These are in addition to the obvious facts that the Sun is at the centre with the planets in orbit around it. ...

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• Arithmetic excercises in the Solar system
• The basic stages in the Earth's pre-geological development
• The new concept of formation and development of the Solar system

Magnetic Stars, 2011, pp. 153 ­ 156 Ab out the Dep endence of the Rotation Velo city of CP Stars on the Magnetic Field Glagolevskij Yu. ... Based on the observational data of the average magnitudes of the surface magnetic field strength Bs for a number of chemically peculiar stars we investigate the dependence of the rotation period on the magnetic field. ... Now the periods of rotation P and the average values of the surface magnetic field Bs are known for more than 50 magnetic stars. ...

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• http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p470.pdf
• http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p081.pdf
• http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p147.pdf

RTT150 . ... This search system is designed for generating the necessary information on series of pointings (observations of each source consist of sets of exposures with different filters and sometimes with different exposure times) for observed sources. Search results appear at the separate page as a table with the following data: . DATE - real (not evening!) observations date (in YYYY-MM-DD format); . ... Bin - minimal CCD binning mode (may vary during the observations); . ...

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• GRANAT Home Page

This module provides an environment variable with a unique identifier for each request. ... The unique identifier is even unique across multiple machines in a properly configured cluster of machines. ... On Unix machines, Apache creates several children, the children process requests one at a time. ... To distinguish time we will use a Unix timestamp (seconds since January 1, 1970 UTC), and a 16-bit counter. ... The actual ordering of the encoding is: time stamp, IP address, pid, counter. ...

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• Running a High-Performance Web Server for BSD
• Apache suEXEC Support
• The Apache EBCDIC Port

... Michael E. Lopez-Alegria (Captain, USN, RET.) ... After his second mission, he led the International Space Station (ISS) Operations branch of the Astronaut Office. ... In October 2014 Lopez-Alegria became an independent consultant; he is based in Washington, D.C. SPACE FLIGHT EXPERIENCE: Mission Specialist (MS)-2, STS-73 Columbia (October 20 to November 5, 1995). ... The primary mission objective was delivery of the Expedition 6 crew to the ISS and the return of the Expedition 5 crew to Earth. ...

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• Astronaut Bio: Clayton C. Anderson (01/2013)
• Astronaut Bio: Jerry Ross (05/2014)
• Astronaut Bio: Jay Apt 06/1997