The NICFPS:Data Cube script allows you to take a sequence of exposures over a range of wavelengths. ... Exp : the number of exposures per etalon Z spacing. ... Initial Index: specify this to restart a partial data cube ; otherwise leave it blank. Initial Z : the initial etalon Z spacing. Delta Z : the etalon Z spacing interval. ... Then to restart the data cube later, set Initial Index to the recorded Current Index and restore all other input parameters. ...

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• lsst.tcc: tcc.msg.formatObjFields Namespace Reference
• Procedure to Collimate the SDSS 2.5m Secondary Mirror
• TUI:Instruments:Expose Window

... The keywords EXPRTIME and ZEROMAGN set the zero point for magnitudes. ... The program automatically determines a Point Spread Function when it gets proper initial values from the keywords SPROFIL. Initial values may be wrong by 0.1 each, and the program still can converge to the right Point Spread Function. ... The program looks for an initial point spread function into that descriptor at first and it uses data from the keywords SPROFILx when the descriptor DPROFILE is absent. ...

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• Search for High Rotation Measures

... Simulation Images . Simulations of convection in stars . Vertical cross-section of an A9 main sequenceтАж . Sidebar Left . Sidebar Top . ... Title: Vertical cross-section of an A9 main sequence star . Description: This is a vertical cross-section through a snapshot of a simulation of an A9 main sequence star. ... The longest arrows correspond to the highest velocities of about 29 km/s. The up-flow enters from the bottom of the simulation, bringing up hot plasma from the interior. ...

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• Software Maintenance Manual
• Index of /~akarakas/stellar_yields

Radiotekhnika i elektronika, 1998, vol. ... Transmission of Chaotic Sample Sequences Through RF Channel . ... Received January 29, 1998 . ... The following set of operations is proposed for this purpose: transformation of the chaotic sample sequence into a sequence of AM pulses, modulation of high-frequency carrier by this signal, filtering out the high-frequency signal, demodulating it into a sequence of pulses, and retrieving estimates of the sequence of the chaotic samples. ...

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• Magnetic field influence on martesite phase transition in Ni2+УMn1-УGa

... Southern . ... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Discovery and characterisation of Pre Main Sequence stars in southern star forming regions . ... Observing with ESO Telescopes . ... ESO-MIDAS . ... Using a robust method to identify Pre-Main Sequence (PMS) stars through their photometric excess in the Hн± band, we have recently studied the star formation history in several star burst clusters in the Galaxy, Small and Large Magellanic Clouds. ...

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• ESO - Thesis Topic: Star formation: probing magnetic fields and their spheres
• Gaitee Hussain @ ESO
• Rivi: Be Stars

... Parameters of the Moon-perturbed orbit . ... From orbits consistent with this limitation and with the date of the launch October 1, 2000 as an example, an orbit was selected with apogee directed to the North Galactic pole at the begining and rotation of orbit plane was maximized. The initial state vector is given in the inertial coordinate system in epoch J2000.0. ... The orbit has initial perigee radius Rp=7000.0 km, initial apogee radius Ra=343000.0 km and initial period T=8.453 days. ...

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• GOCG Post-Observation Products

Galushina T., Bykova L., Letner O., Baturin A. Tomsk State University Russia 1 Investigation Dynamics Asteroid of of 2 Solving problems construction of numerical model of asteroid motion with account chosen perturbed factors; asteroid orbit improvement according to positional observations; construction of initial probabilistic domain by linear and nonlinear methods; study of evolution of initial probabilistic domain; revealing of ...

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• http://www.gao.spb.ru/personal/ivanov/papers/ivv-mil2002.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/huang.pdf
• http://www.gao.spb.ru/database/csa/protuberances/prt_fmt_e.txt

... Points to note: . ... The function returns a pointer argument. ... andedRanges => andRangesPair(andedRanges, rangesB) . ... Then later, when appropriate, deallocate(andedRanges) for the final time. % function andRangesPair(rangesA, rangesB, doChecks) result(andedRanges) function andRangesPair(rangesA, rangesB) result(andedRanges) type(RangeT), intent(in) :: rangesA(:), rangesB(:) type(RangeT), pointer :: andedRanges(:) % logical(bool), intent(in), optional :: doChecks end function andRangesPair . ...

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• Initial processing
• Description

Next: Polarization efficiency: size/shape/orientation effects Up: Optical properties of cosmic Previous: The 2175? feature . To model the interstellar polarization one needs to calculate the forward-transmitted radiation for an ensemble of non-spherical aligned dust grains. ... Let non-polarized stellar radiation passes through a dusty cloud with a homogeneous magnetic field. ... The angle between the line of sight and the magnetic field is ( ). ... where the angle is connected with and ( ). ...

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• Optical constant database - Level: data

... Shustov B.M., Wiebe D.S. Dust expelling from the Galaxy ( abstract from the journal ). Astronomy Reports , 1995, 39 , 578-586 [AZh, 72 , 650-659]. Wiebe D.S., Shematovich V.I., Shustov B.M. Chemical and dynamical evolution of protostellar clouds: initial stages of collapse ( abstract from the journal ). ... Shustov B.M., Wiebe D.S., Tutukov A.V. Evolution of disk galaxies and loss of heavy elements into the intracluster medium. ... ApJ (Letters), 1998, 503 , L71-L74 ( astro-ph/9806155 ). ...

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• Globular Clusters: Self-Enrichment

... The relation between the metallicity of F stars and their loci on the c 1 , diagram is investigated for a semple 2000 galactic-disk F stars having uvby data. ... По данным uvby -фотометрии, для двух тысяч F-звезд диска Галактики изучена связь между их металличностью и положением на диаграмме c 1 , . ... Если считать, что распределение металличности звезд диска в диапазоне lg Z/Z (или [Fe/H]) от -0.5 до +0.3 непрерывно, то Y 0.02. ...

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• Sceintific interests

Magnetic Fields around Radio Galaxies Robert Laing (ESO) Laing et al. ... 2008) Negligible depolarization and 2 rotation Almost all Faraday effects must be due to foreground material How to fit depolarization caused by foreground Faraday rotation Complex polarization Rotation measure Integrate over a beam Observed RM for 0 2 rotation and depolarization Faraday rotation and depolarization 5.5 arcsec FWHM Faraday effects at high resolution FWHM = 1.5 ...

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• http://www.mrao.cam.ac.uk/~mh475/poster.pdf
• http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/ABarker1.pdf
• OptInt PmWiki : Initial Setup Tasks | Attach

... Составленная из нулей и единиц цепочка 100010111011110100000111 выглядит более случайной, чем цепочка 010101010101010101010101. ... Однако можно пытаться решать ее для бесконечных цепочек, т.е. для последовательностей. Иными словами, можно пытаться найти строгое математическое определение для понятия "случайная последовательностей нулей и единиц". ... Вот что это означает для того простейшего случая, когда нули и единицы равновероятны ? ...

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• Spectral sequences of fibrations (Fall 2004)
• Dubna-2006: A.N.Dranishnikov --- Morse-Thue sequence.
• Introduction to dynamical systems (Spring 1999)

Microsymposium 38, MS015, 2003 (letter format) MARS: MOVEMENT OF GEOGRAPHICAL POLES AND DEFORMATION OF ITS SURFACE. ... The global analysis of the Earth linear structure elements has allowed to define the position of geographical poles in the different geochronological periods [3, 4]. ... It is the curves that unite sequences of geographical poles - poles of symmetry of faults in the global stress field fixed by faults on a surface of the mantle during its rotation around of the core. ...

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... part 2 | ... Part 1 . The new concept of formation and development of the Solar system. ... Thus, the initial pulse of the rotation of a protosolar cloud of the solar system was determined as a result of the diversion of a part of the moment of the rotational pulse of the Galaxy. ... Besides this new approach to the pre-solar system as a system of the destroyed vortex structure, we can understand now a number of other peculiarities of the Solar system's structure. ...

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• The basic stages in the Earth's pre-geological development

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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The Earth. ... The middle raiding of the Earth is 6371,032 km, the pole 6356,777 km equatorial - 6378,160 km. The Earth surface area is 510,2 mln km^2, 70,8% of which is the World ocean. ... According to the modern cosmogonical views the Earth was formed 4,6 - 4,7 billions years ago from the protoplanet cloud captured by the Sun. ... The Earth is conditionally divided into 3 parts: a bark a cloak and a core (in the centre). The external layer - the bark is 35 km thick. ... Above the Earth. ...

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• jupitere
• moone
• marse

... New Developments in the FITSIO and Fv Software Packages W. Pence NASA/GSFC, Code 662, Greenbelt, MD 20771, Email: pence@tetra.gsfc.nasa.gov Abstract. This paper describes recent improvements to the FITSIO subroutine library and the fv FITS file viewer and editor, both of which were initially described at previous ADASS conferences. ... Introduction The FITSIO subroutine library for reading and writing FITS format files was last described in the ADASS IV conference proceedings. ...

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• The Formation and Evolution of LMC Rich Star Clusters: NGC 1818
• NICMOS Observes the Galactic Center

This sequence of images, taken over a 13-year span by NASA's Hubble Space Telescope, reveals changes in a black-hole-powered jet of hot gas in the giant elliptical galaxy M87. ... The magnetic field is believed to arise from a spinning accretion disk of material around a black hole. Although the magnetic field cannot be seen, its presence is inferred by the confinement of the jet along a narrow cone emanating from the black hole. The visible portion of the jet extends 5,000 light-years. ...

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• Previously understood that magnetic fields were directly related to rotation,
• Mysterious quasar sequence explained | Astronomy.com

WDC-A Digital Exchange Format for One-Minute Geomagnetic Data (Update August 1993) 1. The logical record length is 400 coded characters containing header information, blank spaces, and data for one element for one hour. ... Each logical record contains header information and data in the following format: North polar distance, longitude, year, month, day, hour, element, observatory code, blank spaces, 60 data values, and an hourly mean. ... ORG is the origin of the data. A = Alaska Chain. ...

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• http://www.wdcb.ru/stp/data/sudden.com/pstorm/pstorm.txt.1
• http://www.wdcb.ru/stp/data/geomagni.ind/kp_ap/apstar/ReadmeAPSTAR
• http://www.wdcb.ru/stp/data/geomagni.ind/kp_ap/11Kp_Ap_fmt.txt