... 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. ...

Еще в разделе: (Показать все результаты (>403) - www.izmiran.rssi.ru/ )

• http://www.izmiran.rssi.ru/~obridko/papers/171.pdf
• Magnetic Flux of EUV Arcades and Dimmings

... Explanation: Huge clusters of galaxies are surely colliding in Abell 520 but astrophysicists aren't sure why the dark matter is becoming separated from the normal matter. The dark matter in the above multi-wavelength image is shown in false blue, determined by carefully detailing how the cluster distorts light emitted by more distant galaxies. ... Publications with keywords: cluster of galaxies - dark matter . Publications with words: cluster of galaxies - dark matter . ...

Еще в разделе: (Показать все результаты (>16130) - www.astronet.ru/ )

• Journal "Peremennye Zvezdy"
• XWare > APOD
• Two Worlds, One Sun

... 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. ...

Еще в разделе: (Показать все результаты (>18) - www.vista.ac.uk/ )

• VISTA - Visible and Infrared Survey Telescope for Astronomy
• Use of the (UK) VISTA Data Flow System

Next: NICMOS Science Up: NICMOS Data Calibration and Previous: NICMOS Software at the . ... Reference File Tools . Image Analysis and Reduction . ... These include the tasks used in the STScI pipeline, tools to generate the reference files used by the calibration pipeline tasks, and general image analysis, manipulation, and arithmetic tasks. ... Calnica is used to apply instrumental calibrations to individual datasets, while calnicb is used to process associated sets of NICMOS images. ...

Еще в разделе: (Показать все результаты (>220) - www.stecf.org/ )

• ST-ECF Grism Spectrum Software for NICMOS Grism Data
• ASNCOMBINE (Nov98) --- nictools --- ASNCOMBINE (Nov98)
• The Photometric Performance of the NICMOS Grisms

... Product details: . ... 2 Composition/Data on components: . ... Information pertaining to particular dangers for man and environment . ... 4 First aid measures . ... Use fire fighting measures that suit the surrounding fire. ... Measures for environmental protection: . ... This information is furnished without warranty, and any use of the product not in conformance with this Material Safety Data Sheet, or in combination with any other product or process, is the responsibility of the user. ...

Еще в разделе: (Показать все результаты (>773) - www.issp.ac.ru/ )

• The XI Asian-Pacific Astronomy Olympiad: 1st announcement
• GaS Safety Data Sheet
• CdWO4 Safety Data Sheet

.

Еще в разделе: (Показать все результаты (>7) - www.schools.keldysh.ru/ )

... aiscam@finesse . ... Install Appropriate Filters and Edit filters.txt file . Edit filters.txt file on aiscam@finesse in /home/aiscam/config . ... aiscam: filter -ini ; initializes filter information . aiscam: filter -r ; lists filters installed . aiscam: filter 4 ; moves filter wheel . ... aiscam: fpzero -w 4044.4 -1591.47 ;set fpzero with wavelength and central z . ... aiscam: file dark ;set filename for dark exposures . ... aiscam: file bias ;set filename for biases, no time needed . ...

Еще в разделе: (Показать все результаты (>479) - www.apo.nmsu.edu/ )

• APOzeropts.htm APO Zero Points
• Astigmatism II
• ARC 3.5m | GFP

Orbit . ... The orbit of the RadioAstron provides four types of study: . rough images of radio sources with ultra-high angular resolution, using all baselines up to the radius of the apogee, that is much larger than Earth diameter; . ... high quality imaging of radio sources, with moderate resolution, by observing either with small projected base lines Earth-spacecraft, i.e. close to the orbital plane, or near the perigee. ... high accuracy orbit determination. ... Space Radio Telescope . ...

Еще в разделе: (Показать все результаты (>130) - www.asc.rssi.ru/ )

• P R O T O C O L
• Contingency Plans

Next: Extinction efficiencies: general behaviour Up: Optical properties of cosmic Previous: Optical properties of cosmic . It is now evident that observed interstellar extinction cannot be explain using particles of only one kind. ... The intensity of radiation after passing a dust cloud is equal to . ... The interstellar extinction is . ... Next: Extinction efficiencies: general behaviour Up: Optical properties of cosmic Previous: Optical properties of cosmic root 2003-04-09 ...

Еще в разделе: (Показать все результаты (>247) - www.astro.spbu.ru/ )

• Linear polarization: wavelength dependence
• Polarization properties (transmitted radiation)
• Optical constant database - Level: measurement/paper

COSMOLOGY ACROSS CULTURES ASP Conference Series, Vol. 409, c 2009 J. A. Rubino-Martґ J. A. Belmonte, F. Prada and A. Alberdi, eds. ~ in, A New Test of Einstein's Theory of Relativity by Ancient Solar Eclipses GЁ oran Henriksson Department of Astronomy and Space Physics, Uppsala University, Box 515, SE-751 20 Uppsala Abstract. ... The Lunar Laser Ranging (LLR) of the distance to the Moon makes it possible to check if there is any significant deviation from Kepler's third law of motion. ... 2002). ...

Еще в разделе: (Показать все результаты (>287) - astro.uni-altai.ru/ )

• http://astro.uni-altai.ru/files/weintraub2000_v531.pdf
• Stellarium: SolarSystem Class Reference

Determination of short-term proper motions of fast stars with Pulkovo Normal Astrograph. ... Khovritchev Laboratory of Astrometry and Stellar Astronomy of the Pulkovo Observatory, RAS, Saint-Petersburg Observations Normal Astrograph (D/F=33 cm/3.5m), CCD camera: S2C, FOV = 18x16 arcmin, Pixel size 900x900 mas Determination of the new proper motions of 413 LSPM stars 1 epoch : CCD-surveys and catalogs -- M2000, CMC14, 2MASS, SDSS DR7 2 epoch : CCD-observations with the ...

Еще в разделе: (Показать все результаты (>26) - www.puldb.ru/ )

• http://www.puldb.ru/nikolaev_2011/PUB_NIKOLAEV_2011/damian.pdf
• http://www.puldb.ru/laza_gao/PUB/asrph_1.pdf
• http://www.puldb.ru/laza_gao/PUB/av_3.pdf

... 53, Moscow, 119991 Russia 2 Moscow Physicotechnical Institute, Dolgoprudnyi, Moscow oblast, 141700 Russia Received May 26, 2008 ° Abstract--The relative intensities of Fe XI­Fe XIII lines in the range 176­207 A have been measured for various plasma structures of the solar corona using data from the XUV spectroheliograph of the SPIRIT instrumentation onboard the CORONAS-F satellite with an improved spectral sensitivity calibration. ... 2005, 2007). ... Density measurement based on Fe XIII lines. ...

Еще в разделе: (Показать все результаты (>33) - www.tesis.lebedev.ru/ )

• http://www.tesis.lebedev.ru/en/docs/1571.pdf
• http://www.tesis.lebedev.ru/en/docs/1525.pdf
• http://www.tesis.lebedev.ru/en/docs/1373.pdf

INDOOR LOCATION USING ULTAWIDEBAND CHAOTIC RADIO PULSES Andrey A. Dmitriev Institute of RadioEngineering and Electronics, Russian Academy of Sciences, Mokhovaya St. 11-7, K-9, GSP-9, 125009, Moscow, Russia, E-mail: chaos@cplire.ru Abstract ­ The report is devoted to the problem of indoor location using ultrawideband chaotic signals. ... In the receiver the moment of pulse (pack of radio pulses) emission and the duration of chaotic radio pulse are supposed known. The duration of CRP is fixed. ...

Еще в разделе: (Показать все результаты (>409) - www.cplire.ru/ )

• http://www.cplire.ru/html/lab234/pubs/apl99xx01.pdf
• http://www.cplire.ru/html/oxide233/publication06/gao06phc.pdf
• http://www.cplire.ru/html/oxide233/publication06/nurg06eucas05.pdf

sw@newmail.ru THE PROBE LAYER METHOD IN THE CALCULATIONS OF CONTRIBUTION AND RESPONSE FUNCTIONS S.G.Mozharovsky Ussuriysk Astrophysical Observatory of FEB RAS, Ussuriysk, Russia sw@newmail.ru The method of probe layer for the calculation of response and contribution functions is discussed. ... This allows us to turn from the response functions to the contribution functions calculated with help of the probe layer (CFPL). ... V- VMAX . ... Solar Phys., v.136, p.239-250. ... Solar Phys., v.35, p.11-29. ...

Еще в разделе: (Показать все результаты (>12) - www.uafo.ru/ )

• SunWorld for Stokes profiles calculations
• Algorithm for calculations of the Voigt function

RELATIVE SUNSPOT NUMBERS Description of Data from SGD Explanation of Data Reports: Relative Sunspot Numbers -- The relative sunspot number is an index of the activity of the entire visible disk of the Sun. ... The provisional daily Zurich relative sunspot numbers, Rz, were based upon observations made at Zurich and its two branch stations in Arosa and Locarno and communicated by M. Waldmeier of the Swiss Federal Observatory. ... This indicates the uncertainty above and below the predicted number. ...

Еще в разделе: (Показать все результаты (>53) - www.wdcb.ru/ )

• http://www.wdcb.ru/stp/data/geomagni.ind/aa/aa_IMF/AAIMF.fmt
• http://www.wdcb.ru/stp/data/mod_I_P/DRAFT.TXT

... 2 Measurement of PMTs counting characteristics and selection of op erating p oint To select the operating point of the PMT, that is the optimal values of the high voltage supply and pulse discrimination threshold, the command run counting=hv value is provided in the program mass. ... Starting with the minimum voltage (say 550 V) run command run counting=550 for the measurement execution. ... It is recommended to take measurements for the set of values of 0.4, 0.6, 0.8, 1.0. ...

Еще в разделе: (Показать все результаты (>21) - curl.sai.msu.ru/ )

... Because you are a newly created organization, we are not now making a final determination of your foundation status under section 509(a) of the Code. However, we have determined that you can reason-ably be expectqd, to- be a pubricly supported organization described sectiongn in )WCl), t futCl lr[1o U-10 Accordingly, you will be treated as a publicly supported organization, and not as a private foundation, during an advance ruling period. ...

Еще в разделе: (Показать все результаты (>10) - www.winer.org/ )

• http://www.winer.org/Downloads/Martini-KOSMOS-arXiv.pdf

... The described algorithm is suitable for measurements of complex images of stars. ... a) the zero-based number of stars in the complex (multicentric) image, . b) set of preliminary coordinates - x i , y i , for all stars, index i is number of a star, . ... i - index of a star in the complex image; . ... These parameters are calculated by a nonlinear method of a least squares.The main output parameters of this algorithm are x i , y i ; where the index i is number of a star in the multicentric image. ...

Еще в разделе: (Показать все результаты (>9) - www.izmccd.puldb.ru/ )

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Flights Chronology . ... Project History . ISS Russian Segment . Steps of ISS Assembly . Spaceflights Chronology . Chronology of Extravehicular Activity . ISS 45/46 . ... Rocket Space Complexes . ... Launches Chronology . ... Support of the Space Station functionality; . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

Еще в разделе: (Показать все результаты (>465) - www.energia.ru/ )

• INTERNATIONAL SPACE STATION

... For today there are two main groups of methods of knowledge acquiring: direct (interviews, literature study and others) and indirect (analysis of a training set of examples, observation of an expert and others). ... 2.1 KNOWLEDGE BASE In this paper we initially assume that the fuzzy­"IF ­ THEN"­ rules specified by the experts are already represented in the linguistic form or in the form of a clear clustering correct input-output data sets. ... For this problem, in both networks 0.45 step is optimal....

Еще в разделе: (Показать все результаты (>309) - www.ssau.ru/ )

• http://www.ssau.ru/files/education/metod_1/Kozlov_Conceptual_Aircraft_Term_Project.pdf