... 1s2 . ... 1.04e-03 . ... 1s.3p . ... 1.00e+00 . ... 31142150 . ...

. Cosmology . Very Early Universe . Cosmic Microwave Background Anisotropy . Dark Matter Models . Large Scale Structure . High Energy Astrophysics . Active Galactic Nuclei . Astrophysics of Compact Objects . Accretion Disks . Scientific Staff:

... ТЕОРЕТИЧЕСКИЙ ОТДЕЛ . Заведующий отделом . ... Ахметьев П. М. Белый В. В. Волокитин А. С. Дворников М. С. Кутвицкий В. А. Леинсон Л. Б. Маслов Е. М. Молотков И. А. Рашба Т. И. Тарбеева С. М. ТЕОРЕТИЧЕСКИЙ ОТДЕЛ . Физика нейтрино и нейтринная томография внутренних областей Солнца . ... Физика нейтрино в компактных астрофизических объектах . Нелинейные процессы в темной материи . ... Нелинейные волновые процессы и нелинейные структуры . ...

... 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. ...

... ОБ ОТДЕЛЕ . ... Cеминар теоретического отдела АКЦ ФИАН . ... Новости со школы 'Струны и дуальность' . ... Председатель д.ф.-м.н. В.Н.Лукаш. Секретарь к.ф.-м.н. Е.В.Михеева ( helen@lukash.asc.rssi.ru ), . ... Пропуска заказывать у секретаря АКЦ Страут Людмилы Георгиевны по телефону 333-25-12 до 12 часов предыдущего дня, для прохода в ИКИ при себе иметь паспорт. Новости . ...

Calibration of the GHRS . The GHRS has a spectrum calibration lamp which is used by specifying SC2 as the aperture with WAVE as the target. ... The lines are bright enough so that a 30 to 60 second exposure will yield a good comparison spectrum at almost any wavelength, although longer times are needed at some echelle settings. ... Also, wavelength calibration exposures are generally used to just confirm the zero-point of the spectrum and not to obtain a full wavelength solution. ...

Multi-Wavelength investigations of the Sun and modern problems of solar activity . SAO RAS . ... The conference goal is to present and discuss achievements in the field of experimental and theoretical investigations of a solar activity. Analysis of the 23d solar activity cycle and connections with the Space Weather. ... Solar activity and disturbances of the solar wind and cosmic rays. Modern observational methods for solar investigations. ... Copyright ? 2006 SAO RAS . ... RAS | ...

Next: Wavelength calibration Up: Getting Started Previous: Detecting lines in . ... and the Calibration Starting Row will be used for the lines identifications. ... After setting these parameters, click the button. to pop up the Identify window. ... The identification starts by clicking on , which plots one row of the spectrum in the graphic window, indicates the position of the detected arc lines with blue vertical traces and gives a cursor. ... Figure: Lines Identification Window . ...

Multi-Wavelength investigations of the Sun and modern problems of solar activity . SAO RAS . ... Representation of the last findings in the field of experimental and theoretical investigations of solar activity. The analysis of the maximum of the 23d cycle of solar activity and connection with Space Weather. ... Solar corona study. ... Solar activity and disturbances of the solar wind and cosmic rays. Modern observational methods for solar investigations. ... Copyright ? 2006 SAO RAS . ...

... The calibration of astrophysical spectra in wavelength based on calibration lamp data suffers from different kinds of uncertainties. Besides inaccuracies in the observational phase, common data reduction practice adds ``pixelation'' errors, due to the fact that the centering method does not use the correct PSF. These model mismatch errors depend, for a given feature, on the sub-pixel location of the line center (David & Verschueren, private communication). ...

Subject, Problems and Objects of Theoretical Astrophysics. ... Stellar Photospheres, Their Features. ... Physics of Continuous Radiation Absorption in Stellar Photospheres. ... Continuous Radiation Absorption in Stellar Photospheres of Various Spectral Classes. Solar Type Photospheres. ... Characterisics of Absorption Lines. ... Interstellar Absorption Lines, Their Features. ... Physical and Dynamic Features of Interstellar Medium, Which Follows from Observations of Interstellar Absorption Lines. ...

installed at the AXAF X-ray Calibration Facility at Marshall 2. ... On theoretical grounds, we expect this line to be even nar3 0.04 rower than measured, but in any case, it will serve very well for calibrating the MEG resolution. ... Spectrum of the Penning source with 0.02A bins. ... D. S. Finley, S. Bowyer, F. Paresce, and R. F. Malina, "Continuous discharge Penning source with emission lines between 50 A and 300 A", Appl. ...

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In order to calculate the line profile of a given absorption line for atomic species Z with a wavelength LAMBDA (in Angstroms) and a microturbulent velocity VT (in km/s). ... mode . ... 1) The input model may contain more than one model (i.e. it may be an entire grid of models). Spectrum will cycle through this grid NMOD times, omitting NSKIP-1 models from the . ... However, the input data following MODE must be repeated NMOD times in order to obtain equivalent results for each model in the grid. ...

False-color image of the dark cloud Barnard 68, prepared using data from the Herschel Space Telescope at different far-infrared wavelengths. ... This could be a cloud fragment in collision with Barnard 68. The wavelengths for the images are 100, 160, 250, and 350 micrometers, respectively. The image colors show the intensity of the radiation received at that wavelength, from purple and blue at low intensity to high intensities in red and white. ...

... The minimum precision occurs at x = 0.1 and is approximately equal to precision(1d0)-1. subroutine getBBfluxPerMetre(angstromValues, kelvin, powerValues) real(double), intent(in) :: angstromValues(:), kelvin real(double), intent(out) :: powerValues(size(angstromValues)) end subroutine getBBfluxPerMetre function bbFluxPerMetre(angstroms, kelvin) result(power) real(double), intent(in) :: angstroms, kelvin real(double) :: power end function bbFluxPerMetre . ...

... Theoretical department of ISSP RAS . ... Pis'ma v ZhETF, 69 , 543, 1999; V.E.Bisti , Pis'ma v ZhETF, 73 , 25, 2001 ). (ii) Collective intrasubband charge density excitations are investigated in double GaAs/AlGaAs quantum wells in external parallel magnetic field. ... Goldstone mode relaxation in a quantum Hall ferromagnet . ... The considered system is a Quantum Hall Ferromagnet possessing "classical" spin S 0 ~N j /2 (N j being the number of magnetic flux quanta, S 0 || ... Spin biexciton. ...

... This file table3 82 660 Observed wavelengths, laboratory values and identifications -------------------------------------------------------------------------------- Byte-by-byte Description ... Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- SpOrd Spectrum order 5- 12 F8.3 0.1nm SolLam Wavelength determination of all solar and telluric lines measurable on the ... Note (6): J: Junkes et al., ...

... Буклет школы в PDF здесь . ... Материалы к семинарам В.А.Рубакова - Д.Г.Левкова : задачи (PDF) и таблицы (PDF) . ... 14 августа , воскресенье . ... Знакомство. 15 августа , понедельник . 08.00-09.00 Завтрак . ... 10.40-11.00 Кофе-брейк . ... 16.00-17.30 Рубаков В.А. Генерация первичных возмущений во Вселенной I . ... 18.00-19.30 Макаров Д.И. Космология ближней Вселенной I . ... 16 августа , вторник . ... 17 августа , среда . ... Семинар V ( Задачи IV-V (PDF) , контрольная с решениями (PDF) ). ...

... Space Research Institute . Main . ... Main results of the experimental and theoretical research completed in 2010 . ... Moon's topography is shown based on LOLA laser altimeter data, white contour shows a permanently shadowed region and a white rhomb indicates LCROSS spacecraft impact location. ... Ultra deep survey of the sky in hard X-rays, performed by INTEGRAL observatory . INTEGRAL observatory has completed the first and the most sensitive survey of the sky in hard X-ray energy band. ...