... Other Characteristics of the Sun: Variability of Rotation, Magnetism, Chemical Structure, Planetary System. ... Methods of Solar Magnetic Fields Measuring: Visual, Photografic, Photoelectric. ... Empiric Datas of Magnetic Fields in Photosphere, Chromosphere and Corona. ... Characteristics of Magnetic Field in Balanced Force Tubes by Potential and Forceless Field. ... Phenomenons in Active Region (Magnetic Field, Spots, Torches, Solar Prominences, Flares, Discharges. ... Magnetic Fields in Flares. ...

... Муфта Basko серая с белым мехом Farla позволит родителям быть в тепле даже в морозную погоду. ... Утеплена искусственным мехом. ... Цвет: Серый . Артикул: 1-1-28174-34-486/200 Цвет: коричневый, белый Материал верха: кожа Материал подкладки: искусственный материал Материал стельки: текстиль Материал подошвы: искусственный материал Параметры изделия: ширина голенища 38 мм Уход за изделием: протирать губкой Страна дизайна: Германия Страна производства: Италия Товар сертифицирован. ... Цвет: Белый . ...

Proposal Identification No.: ... Proposal Type: General Category : Observation Category : Total Time Requested: Minimum Useful Time: Regular Astronomy 61.5 Hours 2.5 hours Prop osal Title: AN UPDATED PROPOSAL TO MEASURE MAGNETIZED ELECTRON DENSITY FLUCTUATIONS IN MIRA-VARIABLE-STAR CORONAE ABSTRACT: We have recently realized a technique for measuring electron density The technique uses the propagation effects on a spacecraft downlink carrier. ...

... AstroGuide | ... Constellations | ... Canis Major . Canis Minor . ... Corona Australis . Corona Borealis . ... Leo . Leo Minor . ... Ursa Minor . ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . are trademarks of John Huggins ...

Data format (up to June 1957) . ... 1957 (red+green) . 1958 (green) 1958 (red) . 1959 (green) 1959 (red) . 1960 (green) 1960 (red) . 1961 (green) 1961 (red) . 1962 (green) 1962 (red) . 1963 (green) 1963 (red) . 1964 (green) 1964 (red) . 1965 (green) 1965 (red) . 1966 (green) 1966 (red) . 1967 (green) 1967 (red) . 1968 (green) 1968 (red) . 1969 (green) 1969 (red) . 1970 (green) 1970 (red) . 1971 (green) 1971 (red) . 1972 (green) 1972 (red) . ...

... ATNF Colloquium . Found: The Original 1945 Records of Australian Radio Astronomy - Collaroy Observations . ... In July 2014, Miller Goss, Ron Ekers and Helen Sim found the original records of the first published Australian radio astronomy observations. These were obtained by Joseph L. Pawsey and Ruby Payne-Scott in early October 1945. The observations gave strong evidence of a hot million degree corona as well as frequent radio bursts. ... today * ATNF | ...

Next: Transparency of the Stochastic Up: Model of the Galaxy Previous: Frequency distribution of galactic . ... The parameters of the model resulted from a numerical fitting of various data, such as the observed distribution of the young star population and neutral hydrogen, the density of population II stars in the vicinity of the Sun, the galactic rotation curve and the dynamics and distribution of globular clusters   and dwarf irregular satellites of the Galaxy. ...

... Кометы . ... Зря гостью светлую в знакомых небесах, Мудрец любуется игрой в ее лучах; Но робко путь ее и близость расчисляет. ... Но, между ними путь особый пролагая, Комета яркая - системам не верна, И кажется, грозит другим мирам она, Блистательным хвостом полнеба застилая. ... Всю ночь льют свет в твои селенья Берлин, и Лондон, и Париж, И мы не знаем удивленья, Следя твой путь сквозь стекла крыш. ... Комета светится сердито. ... Я - искра, искра из хвоста кометы, всего лишь искра, я погасну скоро...

. A filament stretches across the lower half of the Sun in this image captured by NASA s Solar Dynamics Observatory on February 10, 2015. Filaments are huge tubes of relatively cool solar material held high up in the corona by magnetic fields. Researchers simulated how the material moves in filament threads to explore how a particular type of motion could contribute to the extremely hot temperatures in the Sun s upper atmosphere, the corona. NASA/SDO

El perfil de temperatura no es el nico requerimiento para la convecci n. La fuerza que impulsa la convecci n---la diferencia de peso entre un fluido caliente y uno fr o---debe vencer la resistencia natural del fluido al movimiento, conocida como viscosidad . ... Es dif cil sacarla de la botella. ... De chimeneas de lava a torrentes de lava . ... Debido a que las burbujas transportan roca caliente desde el interior del planeta hacia la superficie, ellas abastecen a los volcanes con lava. ...

... 2006: . ... 1) A study of the solar corona. ... 2) The study of the solar northern polar region. A powerful radio source above the solar North Pole in the region of the polar coronal hole was discovered. ... A transition boundary from brightening to darkening at the wavelength of 3.5cm was found in the emission of the polar coronal hole. These facts are decisive for the choice of the solar cycle model. 3) Polarized radio emission of a high-latitude prominence was registered. ... Archive . ...

ПУБЛИКАЦИИ - 1994 год . G.Ya.Smolkov , V.P.Nefedyev, A.M.Uralov , N.N.Kardapolova. Step-wise emergence and development of microwave emission of active regions-a fundamental property of active solar corona. Solar coronal structures, Proc of 144th IAU Coll, Veda, Publhouse of SAS, - 1994. ... The observations of solar microwave bursts at the Siberian solar radio telescope with 50-millisecond resolution. ... Nato Rubl/Nauka, - 1994. ... Electron beam propagation in the solar corona. ... 1994. ...

... click image to view discuss) . ... Bert improved his composite image showing details of the corona. ... He also did a better job of color correction, avoiding a false light bluish hue that was present near the 6 o'clock position on the moon's limb in the earlier image. ... of this image is the seventh-magnitude star SAO 109216. Submitted by Bernie Volz on 05/08/2006 22:12:59 . ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

INTEGRAL observations of SS433 : new results Anatol Cherepashchuk Sternberg Astronomical Institute, Moscow University, Russia In collaboration with: Rashid Sunyaev ... Eleonora Antokhina, Nikolai Shakura, Darja Kosenko, Elena Seifina,Sergey Molkov (IKI) 1 Overview · Introduction · · · · Observations Analysis of hard X-ray spectra Analysis of hard X-ray eclipses Discussion and conclusions December 26, 2007 ...

2005 10-15 , 2005 , -2005 22.63 431 K 71 : .. ... e-mail: sis@coronas.ru -, . ... GOES ACE, "-". 2005 , ( 11- ) , , , , "-", 20 2005 . ... 2005 , , , , "-" ( 20 2005 ) . ... e-mail: zhuravl@sv.ulsu.ru , , . NORAD (www.celestrak.com). ... 1971, 584 . ... 179 C. .., .. , , e-mail: zhuravl@sv.ulsu.ru [1] . NORAD (www.celestrak.com). : mdp . ... e-mail: zhuravl@sv.ulsu.ru NORAD (www.celestrak.com) . ... 179 C. .., .. , , e-mail: "" (), ( ) () , . ... Zi , tN L V > Vth,i , Vth,i Ai ­ (, ), , , . ...

... Анк а дня . ... Созвездия . ... До сих пор считалась, что RXJ1856 представляет собой нейтронную звезду. ... Однако американские астрономы определили, что диаметр RXJ 1856 оказался меньше 16 км. ... Хелфанд проводил наблюдение за расположенном в созвездии Кассиопеи объектом 3С58, находящемся немного подальше от нас - уже в десяти тысячах световых лет. ... Особенности 3С58 можно объяснить лишь в том случае, если предположить, что это - кварковая звезда. ... Созвездие Орион (Ori) . ... Звезда перемен ....

... Galactocentric distance dependences of the physical parameters of globular clusters. ... The straight line in (a) is the rms regression. The large circles in (b) show mean masses within narrow R intervals, and the solid lines show the rms regression fits for thick-disk and old-halo (left) and young-halo and corona (right) clusters. The dashed lines in (c) and (d) are upper and lower envelopes drawn by eye. discussion in the text | privious figure | next figure . ...

ПЕРЕЛ?К ПУБЛ?КАЦ?Й СП?ВРОБ?ТНИК?В ГАО . ... Rosenbush V.K. Rosenbush A.E. Shakhovskoi N.M. Comet Hale- Bopp: Linear and Circular Polarization derived from observations of a stellar occultation . ... Rosenbush A.E. О возможности систематизации классических новых по типам кривых блеска. ... Rosenbush A.E. On evolutionary status of stars with the R CrB phenomenon . ... Rosenbush A.E. What causes the R Coronae Borealis type minimum: dust cloud or dust shell? ...

Coronal "hole" on the Sun . ... As a result of the observations of solar eclipse on February 15, 1961 at wavelength 21 cm the lower brightness region of corona was discovered (detail N5 on figure 1) and it's location on east nimbus of the Sun was determined (figure 2). ... Subsegently such phenomena were named "Coronal Holes". Figure 1. ... The detail N5 is Coronal Hole. ... The location on disk of the Sun radiation details of corona at wavelength 21 cm. ...

PECULIARITIES OF QPOS OF MICROWAVE EMISSION OF THE FLARING SOLAR ACTIVE REGIONS V.E. Abramov-Maximov, G.B. Gelfreikh Central Astronomical Observatory at Pulkovo, Saint-Petersburg, Russia gbg@saoran.spb.su Quasi-p erio dic oscillations of solar coronal structures are effectively registered in particular at microwave waves. The physical nature of p erio dical pro cesses in the corona is clearly connected with plasma structures of the solar atmosphere. ...