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DATACENTRES, DATABASES & CATALOGUES
Main actors in astronomy research in the country  There are 7 Research Institutes in the structure of the National Academy of Sciences of Ukraine (NAS of Ukraine), 2 Research Institutes in the structure of the Ministry of Education and Science, Youth and Sport of Ukraine (MESYS of Ukraine); 15 astronomical observatories and Departments in the structure of the Universities of the MESYS of Ukraine; 1 Private Astronomical Observatory play a main role in the development and teaching Astronomy in Ukraine.
 
The XPM Catalog  Absolute proper motions of 280 million stars distributed all over the sky without gaps in the magnitude range 10m < V <20m on the basis of combined data from 2MASS and USNO-A2.0 catalogues.
 
MAO NASU Plate Archive   Digital archive of MAO NAS of Ukraine (GPA) comprises data of about 26 thousands of direct photographic plates, obtained with 14 instruments in 9 observational sites, and more than 2000 digital images of different resolution available via GPA search pages.
 
Mykolaiv AO Plate Archive   Digital archive of Mykolaiv Aastronomical Observatory (MykAO) includes astronomical data obtained during observations with photo plates and CCD frames. The digitization of the archive is near its completion. Digitized images are available via a web browser and Aladin.
 
AO LNU Plate Archive   Astronomical Observatory of Lviv National University (AO LNU) is the owner of valuable archive that stores approximately 8 000 of photographic plates from 1939, including nearly 6 000 direct images of the northern sky. The archive is partly digitized and images are available via the joint search pages of AO LNU and MAO NASU.
 
IRA UTR-2 catalogue of RS   The very-low frequency sky survey of discrete sources has been obtained in the Institute of Radio Astronomy of the Ukrainian National Academy of Sciences (Kharkov, Ukraine) with the UTR-2 radio telescope at a number of the lowest frequencies used in contemporary radio astronomy within the range from 10 to 25 MHz.
 
Mykolaiv AO stellar catalogues   27 astrometric stellar catalogues of Mykolaiv Aastronomical Observatory (MykAO) in VOTable format are available for downloading
 
AO KNU Historic Plate Archive   AO KNU glass collection contains about 20 thousand photographic plates. Historical part of the archive was received during 1898-1946 and now is being digitized.
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ASTRO INFO NET
The Role of Data Science in Astronomy and Interstellar Exploration 
Space has always been a fascinating frontier for humans. From the first satellite, Sputnik 1, in 1957, to the amazing Mars rovers, our adventures in space show our love for discovery, creativity, and courage. Exploring space is a big dream, always pushing us to learn more and go further. Nowadays, data science is making a meaningful contribution to space technology. It's changing how we think about space. Being able to gather, understand, and use lots of data has helped us get to know the universe better and has changed how we explore and move through space...
 
GRID-based Virtual Observatory VIRGO.UA 
VO VIRGO.UA for cosmology and astrophysics is a segment of VO «Infrastructure»- a virtual organization, which deals with ensuring the provision of standards for Grid Services for virtual organizations, to ensure reliability functioning of the Ukrainian power grid, Grid training for users and administrators of the Grid sites, as well as the creation of technical conditions UNG for entry into the international grid community...
 
WDC-Ukraine 
WDC-Ukraine is a part of World Data Center System of the International Council of Science (ICSU). Among the basic tasks of WDC-Ukraine there is collection, handling and storage of science data and giving access to it for usage both in science research and study process. That include contemporary tutoring technologies and resources of e-libraries and archives; remote access to own information resources for the wide circle of scientists from the universities and science institutions of Ukraine...
 
IVOA NEWSLETTER
US VAO Data Discovery Portal 
Find datasets from thousands of astronomical collections known to the VO and over wide areas of the sky. This includes important collections from archives around the world. Feedback on your experience with the tool is appreciated -- please send your comments, suggestions, and questions to the VAO Help Desk.
 
US VAO Cross-Comparison Tool 
Perform fast positional cross-matches between an input table of up to 1 million sources and common astronomical source catalogs, such as 2MASS, SDSS DR7 and USNO-B. Feedback on your experience with the tool is appreciated -- please send your comments, suggestions, and questions to the VAO Help Desk.
 
VOPlot v1.8 Beta 
VOPlot v1.8Beta includes many enhancements and bug fixes. To name a few v1.8Beta supports multi-grid plots for 2D Scatter-Plot which allows the user to have multiple plots having grid size from 1x1 to 3x3 in a single window. Paginated view is added to see data in tabular format which allows user to navigate systematically. Provision to label Lat/Long lines is also added. Users can now plot a cumulative histogram for all histogram types. VOPlot 1.8Beta shows the metadata of a FITS file instantaneously while the actual loading happens in background. VOPlot v1.8Beta also provides better handling of "faulty data" while parsing an ASCII file.
 


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 Gopasuk Stepan Ilyich 

General data:

07.07.1930 - 08.08.2005

Place of birth: Legaty village, Brest region, Byelorussian SSR

Studied in: Ivan Franko Lviv State University (since 1999 Ivan Franko Lviv National University) (1954);

Key interests: solar physics, magnetic fields of the Sun and stars. PhD Thesis: Development of flares and magnetic fields on the Sun (1963 ); ScD Thesis: Magnetic fields and motions in the solar atmosphere (1975 );


Biography:

He was born on July 7, 1930 in the Legates village of the Brest region of the Byelorussian SSR.

In 1954 he graduated from Ivan Franko Lviv State University.

Since 1954 he has been an employee of the Crimean Astrophysical Observatory. Since 1987 he worked as the head of the laboratory of solar physics, since 1989 he was the chief researcher.

In 1963 he defended his dissertation "Development of flares and magnetic fields in the Sun" and in 1975 his doctoral dissertation "Magnetic fields and motions in the solar atmosphere".

Since 1967 he has been a member of the International Astronomical Union.

In 2000 he was awarded the title of "Honored Worker of Science and Technology of Ukraine".

in the 1980s, together with V. I. Abramenko and M. B. Ogir, they studied the structure of vertical electric currents and Hα-flares of two active regions. Electric currents were calculated on the basis of the transverse component of the observed photospheric magnetic field. Hα-flares appear mainly in places where electric currents are directed upwards.

in the 80's of the twentieth century together with Lazareva L. F. on maps of the magnetic field and the field of radial velocities, which were built on magnetographic observations in the line Fel λ 5250.2 A for AO №251 September 1961 in the localization of solar flares, analyzed fluxes and the velocity of the plasma in the time interval ± 7'from the moment of the event.

He died on August 8, 2005 in the Naukovy urban village.

The main scientific works are devoted to solving the fundamental problems of solar physics, in particular the problems of solar magnetism. He showed important patterns in the movements of plasma and magnetic field at the stage of appearance and disappearance of sunspots, which makes it possible to understand the physical mechanisms that lead to the concentration and decay of the magnetic field on the Sun's surface. He obtained a number of results on the nature of active and quiet areas: found a global electric current in the active industry, justified its role in the formation and sustainability of the active industry; showed that local currents are concentrated mainly in short and low magnetic loops; a significant part of the photospheric magnetic field is due to currents flowing in the photosphere; found that photospheric movements play an important role in the generation of electric currents. He created a method for studying the structure of the magnetic field in the upper layers of the solar atmosphere. Together with O. S. Gopasyuk proved that the observed magnetic field in the solar chromosphere is a superposition of potential and current fields. Derived equations that describe such a field as powerless. Detected torsional vibrations of sunspots with periods of 40 minutes and 6 days. Conducted a comprehensive study of solar flares. He found a close connection between the appearance of flashes and the intensification of motion and rotation of spots as sources of accumulation of magnetic energy of electric currents. He proved the presence of shock waves in flares and studied their role in the development of Hα-flares. He established the connection between the occurrence of flashes and the direction of electric current, found asymmetry in Hα flows and rigid X-ray emission of flashes. He studied the role of compression and expansion of the field of magnetic loops filled with cold plasma and accelerated electrons in changing the intensity of synchrotron and hard X-rays. Obtained the characteristics of the acceleration spectrum of electrons, cold plasma and magnetic field.

He is the author and co-author of more than 190 scientific papers, a review of solar electrodynamics and a monograph on solar physics.




Main publications:
  1. Эволюция активной области, ее токовых систем /Абраменко В. И., Гопасюк С. И., Огирь М. Б.// Изв. Крым. астрофиз. обсерв., 1988, С. 151-170
  2. Потоки вещества и поле фотосферных скоростей в районах возникновения солнечных вспышек/Гопасюк С. И., Лазарева Л. Ф. Препр. Владивосток: Инт-т Космофиз. исслед. и распростан. радио волн, 1988, 16 с.



Sources:
  1  Астрономы России 1917-2017/ науч. ред. А.М.Черепащук, Казань, Казан. фед. ун-т, 2017.- 568с- C.114, 115
  2  Реферативный журнал. 51 астрономия., М.: ВИНИТИ, 1988, №12, С.76

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