... NICMOS data are represented by five arrays for each readout. ... Samples array. ... Each downlinked readout is always represented by these five arrays ( Figure 13.4 ). Multiple readouts in the same dataset (e.g., MULTIACCUM data) are represented by repeated sets of these five arrays ( Figure 13.5 ). ... For data where multiple samples of the array were obtained during the integration, the samples array denotes the number of samples for each pixel in the corresponding science image. ...

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• Star formation rates from young-star counts and the structure of the ISM across
• WFC3 Data Handbook
• Webcast

... On-board Integrated submm spectrometer for atmosphere monitoring and radio astronomy V.P. Koshelets, P.N. Dmitriev, A.B. Ermakov, L.V. Filippenko, A.V. Khudchenko, N.V. Kinev, O.S. Kiselev, A.S. Sobolev, M.Yu. ... In particular we have developed integrated receiver for novel balloon borne instrument TELIS (Terahertz Limb Sounder) [5]. ... TELIS is designed to be a compact, lightweight instrument capable of providing broad spectral coverage, high spectral resolution and long flight duration. ...

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• http://www.cplire.ru/html/lab234/pubs/2013_18.pdf
• http://www.cplire.ru/html/lab234/pubs/2013_24.pdf
• http://www.cplire.ru/html/lab234/pubs/2010-13.pdf

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Structure of the Orrery . ... The Human Orrery is the latest addition to the grounds of Armagh Observatory and provides a unique investigation of planetary motion. ... The first orrery was conceived by English clockmaker and inventor George Graham (c.1674-1751) around 300 years ago. This initial model only showed the earth-moon system which orbits our Sun. ... Structure of the Human Orrery . ... The First Point of Aries . ...

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... Files with sunspot magnetic fields data ============================================== Column Format Description ______________________________________________ 1-2 I2 Day of month 3-4 I2 Month (numerical) 5-8 I4 Year 9 A1 Blank 10-13 I4 UT in hhmm 14 A1 Blank 15-19 A5 Sc - atmospheric flutter in arc sec 20 A1 Blank 21-25 A5 S - quality of the Sun image 26-27 A2 Blank 28-31 A4 Spot number (everyday new) 32 A1 Blank 33-36 I4 Magnetic field strength in G 37 A1 Blank 38 A1 Polarity (N or S) 2. ...

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• Structure of the database files

... Suspected G36.6-0.7 has the spectral index -0.8, it seems to be a background extragalactic source because the spectral index is too steep for SNR. ... During the last years the RATAN-600 has been used to carry out a new survey of the Galactic plane at 960 and 3900 MHz from l=342^o to l=19^o, |b| < 5.5^o, to search for new SNRs and to study the SNRs that have just been detected. Column (1) lists Galactic notation names of the new and well--known SNRs from Green's catalog; . ...

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• Data Structures
• Optical data
• HyperLEDA documentation: parameter: vdis

ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Information & tools for observers . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ... The Australia Telescope National Facility Colloquium . ...

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• Polarization/Stokes Handling (stokes and select)
• New Structure In The Shapley Supercluster
• Pulsar Group TapeBackup/Method

... Studies of the pathlength fluctuations through the troposphere using geostationary satellite. ... Relationships that connect the temporal structure function of fluctuations measured with the temporal spatial structure functions of pathlength through the troposphere were obtained. ... On the base of experimental data there were determined the parameters of temporal structure function of pathlength through the troposphere (exponent, structure coefficient). ...

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This home page belongs to small group of scientists working at . Sternberg Astronomical Institute which is a part of Moscow State University . ... Электронная библиотека научно-технической и художественной литературы (доступна только из ГАИШ) . ... Local staff . Dr. Edward Kononovich (konon -at- sai.msu.ru), Associate Professor . ... Dr. Sergey Ayukov (asv -at- sai.msu.ru), Research Fellow, Webmaster of the group . ... Joint seminar of Solar Studies Structure Group and Solar Photometry Group . ...

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• Wavelets and equations
• Dynamic HTML in Communicator
• Notation

.

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• Digital Stellar Spectra
• U of O High Energy Physics Seminars

... AAS link ] . ... Our internal perspective makes it difficult to determine the spiral structure of our own galaxy. ... H I absorption, on the other hand, traces colder, denser gas that should be more confined in discrete clouds and perhaps discrete spiral arms. In addition, H I self-absorption (HISA) requires background H I emission at the same velocity as the foreground absorbing gas, thus introducing a much-needed constraint on the large-scale sightline geometry and kinematics. ...

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• Multiscale Structure in Dust Reflection and Cold HI
• Spectral-Line Observing
• Colloquium Schedule

We present the results of our observations of the white-light corona in polarized light performed at Criciuma eclipse, Brazil. During the observation of 3.11.94 we have made five couple of pictures of the solar corona in polarization light. ... Koutchmy S., Molodensky M., Starkova L., Ershov A., Matsuura O .: ... Molodensky M., Starkova L., Koutchmy S., Ershov A .: ... Koutchmy S., Molodensky M.M., Starkova L.I . ... Koutchmy S., Molodensky M.M., Starkova L.I. Koutvitsky V. and Ershov A . ...

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• SINGULAR POINTS IN THE SOLAR CHROMOSPHERE
• CMEs and Space Weather

Introduction This catalogue contains mainly the atomic data needed in the astrophysical investigations of low-density plasma. It is a revised and extended version of the "Catalogue of Atomic Data for the Rarefied Astrophysical Plasma" (Golovatyj et al. ... Low-density plasma. ... In the present study we represent only the atomic data for computation of sp ectra of low-density astrophysical plasma (most known kinds of it are gaseous nebulae), their thermal and ionization structure. ...

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• Introduction
• Kholtygin et al., Astron. Astroph. Trans., (2003)
• Course of Non-numerical Programming

THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE BY MEANS OF DIGITAL MODELS. ... The surface brightness of Mercury was measured Danjon (1933, 1949, 1953) and Harris (1961) in phase angle 3o-123o. The analysis of the various data of the integral photometric gives the results of determination of the main photometric constants for Mercury. ... THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE: S.G. Pugacheva The surface brightness of the Mercurian images was established on the geologic map Mercury. ...

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• http://selena.sai.msu.ru/Shev/Publications/ms38/ms082.pdf
• http://selena.sai.msu.ru/Chik/Publications/ms40/17_Chikmachev_etal.pdf
• http://selena.sai.msu.ru/Pug/Publications/ms38/ms080.pdf

... Laboratory for Spectroscopy of Molecular Structures . ... Optics and spectroscopy of molecular and liquid crystals, fullerenes, superthin molecular films. Optical studies of structure, phase transitions, pretransitional phenomena, structural modifications in external field and under high pressure. ... Methods developed in the laboratory enable to determine in free standing films of different types liquid crystals values of polarization, two-dimensional constants of orientational elasticity. ...

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• PLDS-3, Chernogolovka, Russia, 2001 - Program, abstracts and proceedings
• Laboratory of spectroscopy of defect structures ISSP RAS
• LSR ISSP RAS

. The UNIX file system is organised as a hierarchy of directories starting from a single directory called root which is represented by a / (slash). Imagine it as being similar to the root system of a plant or as an inverted tree structure. Immediately below the root directory are several system directories that contain information required by the operating system. The file holding the UNIX kernel is also here. UNIX system directories . Home directory . Pathnames .

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• About the Concepts menu

The subdirectory steppe contains the time series recorded at Zymlyanskaya steppe in Rostov-na-Donu region. The data recorded in Moscow are placed at subdirectory moscow . ... The first one is the horizontal wind velocity, the second one is vertical velocity. ... The first two digits of filename is an identification of recording, and the third digit (1-6) is the number of time series. The first number N in any file is the total number of the points, followed by the N data values. ...

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• Zen: Tsearch V2 Readme
• Astronet
• SAI Supernova catalog

... The file names' construction . The flight (m) stage's file set . ... the orbital data used for the flight operation monthly (m) long-term planning, . ... The orbital calculations are based on the initial orbital data determined by KIAM RAN using the orbital radio- measurement treatment. The determined initial orbital data are presented as a state vector (satellite position and velocity) in the J2000 reference. ... Accept the file with extension '.bgr', where the Moscow time (MT=UT+3h) is used. ...

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• Space Research Institute (IKI) Seminar
• ASCII files description
• The INTERBALL Tail PROBE orbital elements

The preferred way to document an SAS package is via LaTeX. If you created the package directory structure with the SAS package maker pkgmaker , a subdirectory called doc will have been created with partially filled out LaTeX templates. ... Also, the new structure is seamlessly integrated in the overall SAS make file mechanism so that it becomes possible to generate HTML or PostScript documentation for the whole SAS. ... The BibTeX file is called sas.bib and is pat of the package sas . ...

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• Input Files
• Routines which act on DSS RangeT vectors

... As a result of BTA observations of 23 chemically peculiar stars with strong magnetic fields, it was found that in 22 of them the longitudinal magnetic field, measured from the hydrogen line cores are considerably lower (by about 1/3) than the value measured from metal lines in the same spectra. ... New approaches need to be developed in order to interpret the data. ... The Zeeman spectrum of a star with a strong magnetic field, 53 Cam. ...

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• A unique isolated dwarf spheroidal galaxy KKR25
• Solar system sector, archive 1993
• Origin of the internal structures in HL Tauri jet (HH 151)

... A comparison of the computed and experimental relations F max ( H), as well as comparison of drift scans of point sources across different horizontal cross-sections of the BP with the corresponding computed cross-sections were made. ... The drift scans of the point source 3С84 (H=87 o ) at the wavelength 7.6 cm across the horizontal cross-sections of the BP (black lines) and the computed horizontal cross-sections of the BP corresponding to them (red lines). ...

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• Results scientific researchs 22
• Fabry-Perot Interferometer: Gallery Old
• Structure and properties of IRC+10216