Download Izmccd (~2.7 MB). ... a) a choice of the best mode of measurements of stars and objects ("Properties/Measurement"), . b) a choice of reference stars. ... 1) necessity of presence on an image of a plenty of stars (we recommend to apply this mode, if on the frame of reference stars is more 100) . ... Sx and Sy depend from residuals at all reference stars (reference stars are marked by blue color). ... These residuals are the image of the star a minus function of a profile for each pixel. ...

Distribution of the analyzed SEPs with different >100 MeV proton fluxes ( J 100 ) at the microwave flux density plane ' S 9 vs. ... 1) General correspondence takes place between intensities of microwave bursts and proton fluxes - J 100 increases when S 9 and S 15 rise. ... 3) Powerful microwave bursts ( S 9 , S 15 >3000-10000 sfu ) with hard radio spectra ( S 9 < S 15 ) correspond to majority of powerful proton fluxes ( J 100 >10 pfu ). ...

Journal of Crystal Growth 191 (1998) 779 --782 Growth of sapphire shaped crystals with continuously modulated dopants V.N. Kurlov*, S.V. Belenko Institute of Solid State Physics, Russian Academy of Sciences, Chernogolovka, Moscow District 142432, Russian Federation Received 6 March 1998 Abstract Dopant-modulated sapphire crystals with combinations of various structures in one sample have been prepared in situ by the growth from an element of shape (GES) method. ...

spaceweb@oulu.fi - last update: 28 May 1995, 0800 UT . Advanced plasma theories are extremely important when one tries to explain, for example, the various waves and instabilities found in the plasma environment. ... In the kinetic theory it is necessary to know only the distribution function for the system of particles. ... The dependence of the distribution function on the independent variables r , v , and t is governed by an equation known as the Boltzmann equation . ... Hot plasma theory . ...

... In this case, the distribution skewness increases near the 11 year cycle maximum phase. ... In medium and large 11 year cycles, the average distribution skewness for a cycle is always positive and its value is related to the cycle amplitude. ... It is clear that the skewness index (DMM) value is positive for all phases from the range 2 < T < 9 and increases toward the cycle center, when the mean latitude is far from the equa tor and the upper sunspot generation boundary. ...

. Name . Last Modified . Size . Type . Parent Directory / . - . Directory . 10.2 / . 2009-Dec-06 17:59:27 . - . Directory . lighttpd/1.4.37

. Made using Google Earth 2007 . Above: The GMRT antennas of the central array from space. The white, blurry objects are the antennas dishes. Above: The GMRT antennas of the central array from space. The position of the antennas are maked by symbols. Above: The GMRT antennas of the outer array from space. The position of antennas are maked by symbols. Last modified: Tue Apr 24 18:19:47 EST 2007

... At least some of them were inside a star that later exploded, says Foothill College Astronomy and Physics Instructor Andrew Fraknoi, who has been answering questions like that for students, on the radio and in books and articles, for more than 30 years. ... For 14 years, Fraknoi served as the executive director of the Astronomical Society of the Pacific, an international scientific and educational organization founded in 1889. ... About the American Institute of Physics . ...

... Gravitational wave search provides insights into galaxy evolution and mergers . ... galaxies . ... Four spiral galaxies in Leo . ... Study predicts distribution of gravitational-wave sources . ... The new study suggests that astronomers might not want to look in the nearest galaxies for these "optical counterparts" of gravitational waves. ... Detecting the optical counterparts of gravitational-wave detections will be a lot easier if they are not within galaxies," Ramirez-Ruiz said. ...

... It is reasonable to expect that UV part of the irradiating spectrum is most influenced by the grain evolution (growth and sedimentation ) which marks the very initial stage of planet formation. 2 log J [erg s­1 cm­2] 1 0 -1 -2 -3 1000 BB 40 0 0 (A5 ) BB 20 0 00 (A5) Drai ne (A5 ) BP Ta u (A5) BB 40 0 0 (GS) BB 20 0 00 (GS) Drai ne (GS) BP Ta u (GS) Disk Model Density distribution is based on a 1+1D disk ... Green lines are used for a model with dust growth and sedimentation. ...

... Pre-university education . ... The certificate obtained by the University proves compliance of the nanosatellite SamSat-218 with safety requirements when performing works on preparation, d