Statistics of sunspot activity . The sunspot indices . ... Visual indices of solar activity . ... n - number of spot groups . A - Waldmeier class of unipolar spot groups without penumbra . B - class of bipolar spot groups without penumbra . C - class of bipolar spot groups with one penumbra pole . D - class of small bipolar spot groups with two penumbra poles . E - class of middle bipolar spot groups with two penumbra poles . ... H - class of unipolar penumbrated spot groups . ...

... 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. ...

... A.Tsivilev (Pushchino Radio Astronomy Observatory) "Investigation of Orion A nebula by radio recombination lines". ... T.D.Dorokhova (Astronomical observatory of Odessa national university) «Researches of rapidly oscillating Ap stars». ... N.V.Grabko (Odessa State Ecological University), M.I.Ryabov (Odessa Observatory of IRA NANU) "Space Weather and us: influence of change of a condition of solar and geophysical activity on reaction of various systems of an organism of the person". ...

GENERAL INFORMA T ION ABOUT How does my LOMO® Night Vision Device Work? ... LOMO® NIGHT VISION DEVICES & FAQs When using a Night Vision Device, you are actually looking at an image that is projected by the intensifier tube located inside the unit (Fig. ... Light enters the Night Vision Device through the objective lens and hits the photocathode in front of the intensifier tube. ... Infrared (IR) Illuminator Microchannel Plate (Gen.2 Only) When do I use my LOMO® Night Vision Device? ... Fig. ...

... Les gaz de la poudre, dilatаЙs par la chaleur, repoussаИrent avec une incomparable violence les couches atmosphаЙriques, et cet ouragan artificiel, cent fois plus rapide que l'ouragan des tempаКtes, passa comme une trombe au milieu des airs. ... On n'avait pas, d'ailleurs, entendu dire que le projectile fб?t retombаЙ sur un point quelconque des аОles et des continents terrestres, et J.-T. Maston n'admettait pas un instant une chute possible dans les ocаЙans dont le globe est aux trois quarts couvert...

... Seminar archive . ... Титарчук Л. X-ray spectral index correlations vs mass accretion rate in neutron star and black hole X-ray binaries in their different spectral states. ... vs mass accretion rate as in the case of NS as well in the BH case. In BHs the spectral index should increase and then saturate with mass accretion . ... BH case the index, indeed, correlates and then saturates with mass accretion . rate. Moreover this index-mass accretion rate correlation allows us to estimate . ...

Journal of the Amateur Astronomers Association of New York March 2010 Volume 58 Number 3, ISSN 0146-7662 EYEPIECE will save significant weight. ... The JWST will be a very large space telescope. ... March 28 Moon at perigee, 224,859 miles from Earth, 12:59 a.m. March 29 Moon lies near Saturn; full Moon at 10:25 p.m. 2 Mars and Moon Shone Bright By Joseph A. Fedrick During the nights of January and the first half of February, Mars and the Moon shone bright, although the frost was cruel. ...

Elsevier Ed itorial System(tm) for JASR 2006 Manuscript Draft Manuscript Number: Title: Determination of K, Ar, Cl, S, Si and Al flare abundances from RESIK soft X-ray spectra Article Type: Contributed Paper Section/Category: E2.4 - Solar Magnetic Field and Activities Keywords: solar physics; X-ray flares ; spectroscopy; abundances Corresponding Author: Dr. J. Sylwester , Corresponding Author's Institution: Space Research Center First Author: J ... All flares were observed early Fig. ...

. Shown here is my first self made instrument, which I designed and built from 1995 to 2001. It is the 110-mm f / 7,3 Newtonian reflector on the German equatorial mounting. Your can see two versions of the mounting and some fotos of details.