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Savremeni model digitalizacije arhivske građe naučnog instituta i njegova primena u proučavanju itorije Matematičkog instituta SANU

Šegan-Radonjić, Marija (University of Belgrade , 2019)

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Abstract:

Предмет докторске дисертације је израда оквира за дигитално архивирање у циљу очувања, представљања и омогућавања доступности дигитализованог и дигиталног садржаја за потребе историјских и других истраживања. Предложени оквир заснива се на концепту ,,тематских колекција“ и намењен је истраживачима који желе да креирају сопствене дигиталне збирке историјских извора и текстова како би ширу научну заједницу упознали са својим истраживањем, повезали га са ширим контекстом и створили услове за умрежавање и сарадњу. Оквир, на примеру дигитализације архивског материјала Математичког института САНУ и у складу са актуелним препорукама и прописима за дигитализацију културног наслеђа у Републици Србији, нуди смернице за: 1) економичан поступак превођења у дигитални облик ради добијања оперативних копија за представљање на вебу, 2) каталогизацију и опис дигиталних докумената помоћу Dublin Core скупа елемената, 3) креирање дигиталног архива помоћу Omeka Classic платформе, 4) израду упутства за архивско истраживање одређених историјских тема и 5) састављање историјских есеја у дигиталном окружењу. Посебни циљ докторске дисертације је примена предложеног оквира у историјским и другим истраживањима, конкретно у проучавању развоја Математичког института у периоду од његовог успостављања у крилу Српске академије наука 1946. године до његовог осамостаљивања 1961. године. Резултати рада су: 1) систематски обрађено питање прошлости Математичког института САНУ у поменутом хронолошком оквиру, 2) дигитална колекција посвећена историји математике и сродних наука у Србији и југоисточној Европи и 3) предлог оквира за дигитално архивирање дигиталног и дигитализованог садржаја за потребе историјских и других истраживања.

URI:

http://hdl.handle.net/123456789/4855

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MarijaSeganDoktorat.pdf ( 29.70Mb )

S BEOGRADSKE ZVEZDARNICE

Petković, Đorđe (Astr. Soc. "Rudjer Bošković" , 2008)

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URI: http://hdl.handle.net/123456789/1242

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62.pdf ( 445.1Kb )
SBORNIK ZADAČ I UPRAŽNENII PO MATEMATIČESKOMU ANALIZU

Demidovič, B. P. (Moskva , 1956)

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URI: http://hdl.handle.net/123456789/2567

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szFR.pdf ( 32.52Mb )
SBORNIK ZADAČ PO TEORII FUNKCII KOMPLEKSNOGO PEREMENNOGO

Volkovljiskii, L. I.; Glunc, G. L.; Aramanovič, I G. (Moskva - Lningrad , 1960)

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URI: http://hdl.handle.net/123456789/2554

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kpFR.pdf ( 21.76Mb )
Science with the Virtual Observatory

Hatziminaoglou, Evanthia (Astronomical Observatory Belgrade and Faculty of Mathematics, Belgrade , 2010)

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URI: http://hdl.handle.net/123456789/2081

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hatziminaoglou2.pdf ( 3.682Mb )
SCIENTIFIC CORRESPONDENCE OF PROFESSOR DRAGOŠ CVETKOVIĆ I

Cvetković, Dragoš (MATEMATIČKI INSTITUT, BEOGRAD , 2012)

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URI: http://hdl.handle.net/123456789/1983

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DC72R.pdf ( 3.825Mb )
SCIENTIFIC CORRESPONDENCE OF PROFESSOR DRAGOŠ CVETKOVIĆ II

Cvetković, Dragoš (MATEMATIČKI INSTITUT, BEOGRAD , 2012)

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URI: http://hdl.handle.net/123456789/1984

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DC73R.pdf ( 2.248Mb )
SCIENTIFIC CORRESPONDENCE OF PROFESSOR DRAGOŠ CVETKOVIĆ III

Cvetković, Dragoš (BEOGRAD , 2012)

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URI: http://hdl.handle.net/123456789/2006

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DC1970-1974.pdf ( 9.068Mb )
SCIENTIFIC CORRESPONDENCE OF PROFESSOR DRAGOŠ CVETKOVIĆ IV

Cvetković, Dragoš (BEOGRAD , 2012)

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URI: http://hdl.handle.net/123456789/2007

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DC1974-1977.pdf ( 11.17Mb )
SCIENTIFIC CORRESPONDENCE OF PROFESSOR DRAGOŠ CVETKOVIĆ V

Cvetković, Dragoš (Beograd , 2012)

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URI: http://hdl.handle.net/123456789/2068

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Dragos 5 R.pdf ( 15.42Mb )
SCIENTIFIC CORRESPONDENCE OF PROFESSOR DRAGOŠ CVETKOVIĆ VI

Cvetković, Dragoš (BEOGRAD , 2012)

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URI: http://hdl.handle.net/123456789/2069

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Dragos 6 R.pdf ( 19.39Mb )
SCIENTIFIC CORRESPONDENCE OF PROFESSOR DRAGOŠ CVETKOVIĆ VII

Cvetković, Dragoš (BEOGRAD , 2012)

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URI: http://hdl.handle.net/123456789/2070

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Dragos 7 R.pdf ( 16.01Mb )
Scientific Review

Perović, Slobodan; Todorović, Jovan (Belgrade , 1996)

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URI: http://hdl.handle.net/123456789/2272

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ScR FR.pdf ( 5.694Mb )
SDSS Spectroscopic Surveys

Ivezić, Željko (Nenad Milovanović & Milan S. Dimitrijević, Astronomical Observatory, Belgrade , 2007)

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URI: http://hdl.handle.net/123456789/1455

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I07.pdf ( 3.882Mb )
SEARCH FOR OPTICAL VARIABILITY IN TWO SEYFERT GALAXIES (Conf. II)

Bachev, Rumen; Slavcheva - Mihova, Luba (Astronomical Observatory, Belgrade , 2000)

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URI: http://hdl.handle.net/123456789/758

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01.pdf ( 141.5Kb )
Searching for extrasolar planetsusing microlensing

Dominis Prester, Dijana (Astronomical Observatory Belgrade , 2007)

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URI: http://hdl.handle.net/123456789/1520

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dominis-prester1.pdf ( 2.761Mb )
SEĆANJE NA MILUTINA MILANKOVIĆA

Programski odbor (Beograd , 2009)

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URI: http://hdl.handle.net/123456789/3387

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Secanja_na_Milutina_Milankovica_2009.pdf ( 4.150Mb )
Sećanje na minuli život

Pantelić, Milan (Omega , 1972)

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URI: http://hdl.handle.net/123456789/5557

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bmo.pdf ( 4.243Mb )
Second order eliptic integro-differential problems

Garroni, Maria Giovanna; Menaldi, Jose Luis (CRC Press , 2002)

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URI: http://hdl.handle.net/123456789/3741

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mer9.pdf ( 14.75Mb )

SECULAR DYNAMICS OF SELECTED ASTEROID FAMILIES

Tsirvoulis, Georgios (Beograd , 2019)

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Abstract:

Asteroid families are populations of asteroids in the Main Belt that share a common origin, that is they are the fragments of energetic collisions between two asteroids. Their study over the years has produced a number of important results concerning the collisional and dynamical evolution of the Main Belt, the physical properties of the primordial bodies of the Solar System and the physics of energetic collisions, to name a few. The contribution of the present thesis can be summarized into two main topics: The first is the discovery of a new mechanism that leads to significant perturbations on the orbits of asteroids, and consequently on the evolution of asteroid families affected by it, and the second is the discovery of a couple of new families, each with its own peculiarities. The first part of this thesis was initially motivated by the irregular shape of the (1726) Hoffmeister asteroid family. In an effort to explain this peculiarity we carried out a thorough dynamical analysis of its past evolution and found out that none of the mechanisms known to affect the orbits of asteroids could explain it. Investigating further we discovered that the linear nodal secular resonance with the most massive asteroid (1) Ceres, is the mechanism responsible for the anisotropic inclination distribution of Hoffmeister family members. Having established the importance of the nodal secular resonance with Ceres, we sought to expand on the subject with the study of all linear secular resonances, nodal and periapsidal, involving not only (1) Ceres, but (4) Vesta, the second most massive asteroid, as well. To do so we utilized numerical integrations of test particles across the whole Main Belt, and evaluated the impact of these resonances on their orbits. Furthermore we identified all asteroid families crossed by one or more of these resonances. Two of these cases, the families of (1251) Seinajoki and (1128) Astrid were then studied in more detail, confirming the importance of the previously ignored secular resonances with massive asteroids. The second part details the discovery of two new asteroid families. The first one, that of (326) Tamara family, was motivated by the unexpectedly high number of dark asteroids in the Phocaea region, a part of the inner Main Belt which is expected to consist mostly of bright ones. Using all available physical data we were able to show that most of the dark asteroids therein belong to a single dynamical family, which we then further analyzed finding that it is 264 ± 43 Myrs old and that it could have a significant contribution to the influx of small dark asteroids toward the Near Earth region. The second discovered family, that of (633) Zelima, is a small cluster, sub-family of the large (221) Eos family. After identifying its members, we derived the age of the Zelima family, which turned out to be only about 3.66 Myrs.

URI:

http://hdl.handle.net/123456789/4752

Files in this item: 1

Tsirvoulis_Georgios.pdf ( 76.51Mb )

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