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. ...

Еще в разделе: (Показать все результаты (>15) - solarwind.cosmos.ru/ )

• http://solarwind.cosmos.ru/txt/2011/presentations/Sun/Ishkov/apj_691_2_1222.pdf

... Panoramic spectroscopy of the sample of 80 nearby lenticular galaxies is presented. ... By comparing the subsample of the S0s with the chemically distinct nuclei to the total sample of nearby S0s (Fig. 1), we have assured that the chemically distinct nuclei are always younger than the surrounding bulges: the mean age difference between the chemically distinct nuclei and their surrounding bulges is 2.8 Gyr while the age difference between the nuclei and the bulges for the whole sample is only 1 Gyr. ...

Еще в разделе: (Показать все результаты (>47) - sn.sai.msu.ru/ )

• http://sn.sai.msu.ru/~sil/preprints/pazh4036.pdf.gz
• http://sn.sai.msu.ru/~sil/preprints/ilyina_sil.pdf
• http://sn.sai.msu.ru/~sil/preprints/ic3653.pdf

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. ...

Еще в разделе: (Показать все результаты (>26) - www.lomoplc.com/ )

... Reports on progress and error are always recorded in the log file of the program. ... UT date of the measurement finish in YYYY-MM-DD format UT time of the measurement finish in hh:mm:ss format Average flux in A aperture Average flux in B aperture Average flux in C aperture Average flux in D aperture Normalized variance of flux in A aperture Normalized variance of flux in B aperture Normalized variance of flux in C aperture Normalized variance of flux in D ...

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

• http://curl.sai.msu.ru/mass/download/doc/new_mass_cat.pdf
• http://curl.sai.msu.ru/mass/download/doc/dimm_specs.pdf
• http://curl.sai.msu.ru/mass/download/doc/rcx_advices.pdf

Электронная библиотека астронома-любителя. ... архив RSN . ... Ru.Space.News: . Декабрь 1998 . ... Дата: 29 декабря 1998 (1998-12-29) От: Alexander Bondugin Тема: Successful NEAR Flyby Of Eros - Closeup Images Available Привет всем! ... Дата: 29 декабря 1998 (1998-12-29) От: Alexander Bondugin Тема: Lunar Prospector Update - December 21, 1998 Привет всем! ... Дата: 29 декабря 1998 (1998-12-29) От: Alexander Bondugin Тема: Sky Telescope News Bulletin - December 24, 1998 Привет всем! ...

Еще в разделе: (Показать все результаты (>137) - www.astrolib.ru/ )

• Электронная библиотека астронома-любителя. RU.SPACE.NEWS - архив за 16 марта
• Электронная библиотека астронома-любителя. RU.SPACE.NEWS - архив за 11 марта
• Электронная библиотека астронома-любителя. RU.SPACE.NEWS - архив за 01 декабря

Determination of the orbits and estimation of the masses of ADS 7251 and ADS 5983 ( Gem) Natalia A.Shakht, Elena A.Grosheva, Denis L.Gorshanov. ... For ADS 7251 we have used the observations of W. and O. Struve 1821­1878 years (see Fig. ... In the motion of ADS 5983 our astrometric observations have been shown perturbations with period from 5.6 to 6.1 years, which are repeated during all interval of observations and assumed the presence of unseen component with low limit of the mass equal to 0.2 M . ...

Еще в разделе: (Показать все результаты (>18) - www.puldb.ru/ )

• http://www.puldb.ru/laza_gao/PUB/asrph_1.pdf
• http://www.puldb.ru/laza_gao/FOR_page_11/grosheva-june2012Paris.pdf
• http://www.puldb.ru/jenam_2011/PUB_JENAM_2011/shakht_1.pdf

Crater Gassendi . ... I made this drawing was made on the 26th of november 2001. If you compare this one with the previous drawing of Gassendi (below) the differences are clear. ... This drawing was made on the 28th of september 2001. After nearly a full month without observations I had a one hour gap between the thicker clouds. ... This drawing was made on the 29th of august 2001. ... This drawing was made on the 27th of august 2001. ... This drawing was made on the 25th of august 2001. ...

Еще в разделе: (Показать все результаты (>3) - aberrator.astronomy.net/ )

• Aberrator

Main . ... About meteorites . ... What to do if you found a meteorite! ... About the laboratory . ... You may have a question: what to do if you found a stone which looks like meteorite. ... According to the Meteorite Nomenclature Committee, in order for a meteorite to be officially registered in the International Meteorite Catalog, 20% by weight of the main mass of the identification sample must be contributed to a qualified scientific organization. ... The Staff of the Laboratory of Meteoritics. ...

Еще в разделе: (Показать все результаты (>19) - www.meteorites.ru/ )

Тема : Хвостатые гостьи V (информация для наблюдения комет) .. Показать сообщение отдельно . ... Хвостатые гостьи .. ... после того, как ISON приплыл мимо нас, земля находится на орбитальной траектории, которая пройдет через след частицы кометы (тот, который ISON оставил позади, когда это приближалось к солнцу и это случайно встретит или вокруг 12 января - 15, 2014 . ... лучшее время наблюдения 22:00 LDT (Northern hemisphere 45њ North) .. - радиант расположен вблизи Al'dzhabkhakh (30-Eta Leonis, ? ...

Еще в разделе: (Показать все результаты (>232) - www.starlab.ru/ )

• Жизнь в шаровых скоплениях [Архив] - Общая Астрономическая Конференция
• Странный блеск кометы McNaught (C/2006 P1) - Общая Астрономическая Конференция
• Новая [Архив] - Общая Астрономическая Конференция

... Relativistic Astrophysics . ... PhD 1965 in Astrophysics . Doctoral Degree 1970 in Astrophysics . Professor of Astrophysics 1985 . Member of Academy "Europe" 1992 . Member of Royal Datch Academy of Sciences 1996 . Member of Royal Astronomical Society 1998 . Member of Royal Belgian Academy of Sciences 1996 . Corresponding Member of Russian Academy of Sciences 2000 . ... Vice-director ASC . ... 01 (Theoretical Astrophysics) . ... Astro Space Centre . ... novikov@nordita.dk . ...

Еще в разделе: (Показать все результаты (>2) - lukash.asc.rssi.ru/ )

... SHORT TERM PREDICTION OF POWER SOLAR FLARES FROM SSRT DATA . The algorithm for short term prediction of powerful solar flares, based on SSRT data, includes microwave emission characteristics in total and polarized flux, the structure of active region (AR) magnetic field at the photospheric level, and H a patrol data. ... During this period, 7 AR's crossed the solar disk, in which 20 flares of importance ? ... Data on AR's and magnetic fields were received from the Sayan observatory by teletype. ...

Еще в разделе: (Показать все результаты (>16) - ssrt.iszf.irk.ru/ )

... 2014 . ... MAGNETIC FIELDS IN SOLAR ACTIVE REGIONS V.G.Lozitsky Taras Shevchenko National University of Kyiv, Astronomical Observatory lozitsky@observ.univ.kiev.ua, lozitsky_v@ukr.net Magnetic field measurements in solar active regions carry out on a base of the Zeeman effect. ... TRACKING OF RADIO BURST SOURCES IN SOLAR CORONA BY HELIOGRAPHIC MEANS Koval A.A. 1, Stanislavsky A.A. 1,2, Konovalenko A.A. 1 Institute of Radio Astronomy of NAS of Ukraine 2 V.N. Karazin Kharkiv National University 1 .. ...

Еще в разделе: (Показать все результаты (>11) - www.astro-soc.odessa.ua/ )

• http://www.astro-soc.odessa.ua/Public-2010.pdf
• http://www.astro-soc.odessa.ua/Program-2006.pdf
• http://www.astro-soc.odessa.ua/Public-2011.pdf

... The main field of my investigations is stellar spectrophotometry. As a result of scientific activity of our group spectrophotometric catalog was created including energy distribution data on 900 stars in the range 3200-7600AA and 250 stars in the range 6000-10800AA (Voloshina et al., Spectrophotometry of Bright Stars, ed. I.N.Glushneva, 1982, Moscow, Nauka, in Russian). ...

Еще в разделе: (Показать все результаты (>10) - uranus.sai.msu.ru/ )

• Tatjana Khruzina
• Linux on CLEVO 8750