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Tytuł:
Jak klasyfikujemy chondryty zwyczajne?
How we classified ordinary chondrites?
Autorzy:
Szyszka, Mateusz
Powiązania:
https://bibliotekanauki.pl/articles/1033014.pdf
Data publikacji:
2014
Wydawca:
Polskie Towarzystwo Meteorytowe
Tematy:
chondrites
chondrites classification
meteorites
shock stage
weathering grade
Opis:
Modern systems of classification has been started in XIX century. However the true progress was began at 60’s and 70’s of XX century. In this time was started modern analythic methods such as: chemical, mineralogic and pretrographic analysis. For this progress fostered also a large number of found meteorites from Antarctica. This article will be concerned about a classification of ordinary chondrites. Acquired meteorite from moroccan searchers. Has been examined and classified. The scheme of this works are presented below.
Współczesny system klasyfikacji meteorytów pochodzi z końca XIX w. Prawdziwy rozwój nastąpił dopiero w latach 60 i 70 XX, kiedy pojawiły się nowoczesne metody badawcze, umożliwiające bardziej kompleksowe analizy petrologiczne, zwłaszcza chemiczne. Rozwojowi temu też sprzyjała olbrzymia ilość meteorytów znajdowanych na Antarktydzie. Niniejsza praca przybliży czytelnikowi sposób klasyfikacji meteorytów kamiennych typu chondryty. Materiał jako przykład badawczy posłużył meteoryt kamienny zakupiony w 2012 w Maroku.
Źródło:
Acta Societatis Metheoriticae Polonorum; 2014, 5; 149-154
2080-5497
Pojawia się w:
Acta Societatis Metheoriticae Polonorum
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Two spinel-bearing compound chondrules from the Baszkówka meteorite
Autorzy:
Borucki, J.
Stępniewski, M.
Powiązania:
https://bibliotekanauki.pl/articles/2059304.pdf
Data publikacji:
2001
Wydawca:
Państwowy Instytut Geologiczny – Państwowy Instytut Badawczy
Tematy:
Baszkówka
meteorites
ordinary chondrites
spinel
Opis:
The present paper describes two compound chondrules labelled panda and chevron, discovered in the Baszkówka meteorite. Optical microscope, electron microscope and electron microprobe studies revealed an unusual mineral composition and fabric. Both chondrules include "primary" and "secondary" components. The panda and chevron chondrules have apparent diameters of ~0.86 and ~0.54 mm respectively with spinel dominant in primary components and olivine-plagioclase in secondary components overlain by thin microcrystalline rims. Euhedral or subhedral Mg, Fe2+/Al, Cr-spinel crystals from the panda's primary component (zoned, cavernous or homogeneous) were not found in Mg-Fe chondrules in Baszkówka, where Cr occurs exclusively as chromite. Olivine crystals from panda's primary (Fa27.1) and secondary (Fa26.5) component have similar compositions to those from panda's rim (Fa26.4) and comparable to olivine from other Baszkówka Mg-Fe chondrules (average ~Fa25.7). The Ca-plagioclase laths from the groundmass of panda's primary component has an extremely variable composition (~An49 to ~An60), evidently more calcic than those in other chondrules of the meteorite (mean ~An13). The primary components of the two spinel-bearing chondrules may have been formed in a fireball generated by powerful impact during early accretion of a protoplanet. After crystallisation the spinel crystals were abraded and polished, probably during rapid flight through a dense cloud of interplanetary dust. The moderately reducing conditions of the hypothetical fire ball were replaced by a more reducing environment during the condensation of the rims of both chondrules.
Źródło:
Geological Quarterly; 2001, 45, 3; 281-288
1641-7291
Pojawia się w:
Geological Quarterly
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
The Songyuan ordinary chondrite (China) - rich in alien rock fragments and its reclassification
Autorzy:
Borucki, J.
Giro, L.
Orłowski, R.
Stępniewski, M.
Powiązania:
https://bibliotekanauki.pl/articles/2059203.pdf
Data publikacji:
2009
Wydawca:
Państwowy Instytut Geologiczny – Państwowy Instytut Badawczy
Tematy:
Songyuan
meteorites
ordinary chondrites
classification
rock fragments
Opis:
The Songyuan chondrite is composed mostly of minerals and chondrule types common in equilibrated ordinary chondrites. More distinctively, the Songyuan material includes numerous sintered cryptocrystalline rock lumps, possible chondrule precursors, and less frequent fragments of olivine-pyroxene basalt. The moderate porosity (estimated under the polarizing microscope at a few percent by volume) and un compacted metal grains, suggest that the meteorite came from very shallow horizons of the regolith. The shallow original position of the Songyuan fragment on its parent body is consistent also with the abundance of numerous euhedral crystals of the main meteoritic components present in the interstitial pores. They crystallized most probably from fluids migrating through the superficial horizons from the in ner parts of the Songyuan parent body. The structural characteristics and slight differentiation in olivine composition suggests a high degree of homogenization and, together with the median value of the fayalite content (26.2 š0.24 wt.%), corre sponds to the L5 chemical-petrologic group of equilibrated ordinary chondrites. More over, the homogenous extinction in the olivine crystals and the absence of multiple planar fractures indicate the lowest level of the shock metamorphism (S1), whereas the lack of any oxide rims around kamacite and troilite grains points to the lowest level of weathering (W0).
Źródło:
Geological Quarterly; 2009, 53, 2; 187-198
1641-7291
Pojawia się w:
Geological Quarterly
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Euhedral crystals in interstitial pores of the Baszkówka and Mt. Tazerzait L5 chondrites
Autorzy:
Wlotzka, F.
Otto, J.
Powiązania:
https://bibliotekanauki.pl/articles/2059306.pdf
Data publikacji:
2001
Wydawca:
Państwowy Instytut Geologiczny – Państwowy Instytut Badawczy
Tematy:
Baszkówka
Tazerzait Mountains
euhedral crystals
pores
chondrites
Opis:
Euhedral to anhedral crystals of the main meteoritic minerals are found in interstitial pores of the unshocked L5 chondrites Baszkówka and Mt. Tazerzait. The composition of these pore minerals is the same as elsewhere in the meteorite. They must have grown from a vapour phase during metamorphic equilibration of the meteorite minerals. The pores are primary features, i.e. open space remaining after compaction of the constituents of the meteorite.
Źródło:
Geological Quarterly; 2001, 45, 3; 257-262
1641-7291
Pojawia się w:
Geological Quarterly
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
A new classification of Nyirábrany, an ordinary chondrite from Hungary
Autorzy:
Mészáros, M.
Kereszturi, A.
Ditrói-Puskás, Z.
Powiązania:
https://bibliotekanauki.pl/articles/411486.pdf
Data publikacji:
2014
Wydawca:
Polskie Towarzystwo Meteorytowe
Tematy:
chondrite
classification
L and LL chondrites.
Opis:
The Nyirábrany meteorite is an ordinary chondrite from Hungary that fell in 1914 and, to date, has been studied very little. The aim of this work was to carry out a more detailed examination of this meteorite (using optical polarization microscope, energy dispersive X-ray spectroscopy and Raman micro spectroscopy) and re-investigate its previous classification as an LL5 type ordinary chondrite, moreover to complete its classification with a shock stage and a weathering grade. Our new results indicate that Nyirábrany could be a transition type between the L and LL chondrites. The main mineral phases of Nyirábrany are olivine, pyroxene and opaque minerals (e.g. Fe-Ni metal, troilite, chromite), minor constituents are plagioclase, Cl-apatite, cristobalite and glass. The Fe-Ni metal content (1.32 vol%) of Nyirábrany is typical of the LL group, the Fa content of olivines (26.71 mol%) is between the range of the L and LL types, while the Fs-content of the low-Ca pyroxenes (20.51 mol%) is typical of the L-chondrites. Chondrules appear in different sizes, mineral compositions and textures. The textural and mineralogical features (e.g. mostly homogeneous silicate minerals, dominance of clinopyroxenes, recrystallized matrix, well-defined chondrules) indicate petrological type 4-5 for Nyírábrány. The shock stage and the weathering grade of this meteorite were examined for the first time. On the basis of the observed optical and textural features of the olivine grains (e. g. sharp optical extinction, irregular and planar fractures) Nyirábrany has an S2 shock stage. About 30–40% of the opaque phases are affected by oxidation, which shows a W2 weathering grade.
Źródło:
Meteorites; 2014, 3, No. 1-2; 19-32
2299-0313
2299-1220
Pojawia się w:
Meteorites
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Badanie składu pierwiastkowego i mineralnego chondrytu węglistego NWA 4967 za pomocą analitycznej mikroskopii elektronowej
Investigation of Elemental and Mineral Composition of NWA 4967 Carbonaceous Chondrite by Analytical Electron Microscopy
Autorzy:
Szurgot, Marian
Polański, Krzysztof
Kosiński, Janusz W.
Powiązania:
https://bibliotekanauki.pl/articles/1032790.pdf
Data publikacji:
2011
Wydawca:
Polskie Towarzystwo Meteorytowe
Tematy:
analytical electron microscopy
carbonaceous chondrites
extraterrestrial matter
meteorites
Opis:
New NWA 4967 carbonaceous chondrite found in 2007 was investigated by scanning electron microscopy. Elemental composition, mineral composition and microstructure have been analyzed. The composition and distribution of olivines have been determined, and kamacite, taenite, troilite, spinel and melilite identified.
Źródło:
Acta Societatis Metheoriticae Polonorum; 2011, 2; 147-157
2080-5497
Pojawia się w:
Acta Societatis Metheoriticae Polonorum
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Petrography of the Baszkówka chondrite
Autorzy:
Siemiątkowski, J.
Powiązania:
https://bibliotekanauki.pl/articles/2059299.pdf
Data publikacji:
2001
Wydawca:
Państwowy Instytut Geologiczny – Państwowy Instytut Badawczy
Tematy:
Baszkówka
ordinary chondrites
chondrules
structure
petrography
classification
origin
Opis:
The Baszkówka chondrite comprises chondrules, individual crystals of olivine, xenomorphic concentrations of kamacite and troilite, matrix and pores up to 3.0 mm in diameter; porosity reaches 20% by volume. Measurements of 697 chondrules in an area of 250 m2 enabled distinction of three populations. The chondrules and olivine crystals have been sintered at high temperatures. Six structural types showing transitions between porphyritic and granular structures have been discriminated. Rims showing a similar diversity surround about 10% of chondrules. The composition and structure of the chondrules suggest a source from the nebular dust disk around the Sun. The abudance of voids and their relatively large size and a lack of fissures, indicate a small size of the host body, which must have been derived from an early phase of protoplanet formation.
Źródło:
Geological Quarterly; 2001, 45, 3; 263-280
1641-7291
Pojawia się w:
Geological Quarterly
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Oxygen-isotopic compositions of minerals from the Baszkówka chondrite
Autorzy:
Maruyama, S.
Powiązania:
https://bibliotekanauki.pl/articles/2059312.pdf
Data publikacji:
2001
Wydawca:
Państwowy Instytut Geologiczny – Państwowy Instytut Badawczy
Tematy:
Baszkówka
meteorites
ordinary chondrites
chondrules
spinel
oxygen isotopes
Opis:
Oxygen isotopic compositions of two picotite-bearing chondrules from Baszkówka L5(S1) equilibrated ordinary chondrite have been determined by secondary ion mass spectrometry. The O-isotopic compositions of the minerals in the picotite-bearing chondrules are slightly more 16O-rich than the bulk O-isotopic composition of Baszkówka. The petrological properties and the O-isotopic compositions of these chondrules suggest that they have closer relationship to ferromagnesian chondrules than CAIs. The 16O-enrichment of the picotite-bearing chondrules may result from incomplete O exchange reaction between 16O-rich chondrule precursors and the 16O-poor solar nebular gas. This implies that the picotite-bearing chondrules are more primitive than ordinary ferromagnesian chondrules in Baszkówka. The O-isotopic compositions of the minerals in one of these chondrules relate to the crystallization sequence. These O-isotopic variations of minerals within the chondrule may result from incomplete O exchange between the chondrule melt droplet and the nebular gas. The heterogeneity of the O-isotopic composition in Baszkówka indicates that Baszkówka has not been homogenized completely during thermal metamorphism and/or secondary alteration.
Źródło:
Geological Quarterly; 2001, 45, 3; 303-312
1641-7291
Pojawia się w:
Geological Quarterly
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Morocco meteorite falls and finds: some statistics
Autorzy:
Ibhi, A.
Powiązania:
https://bibliotekanauki.pl/articles/412159.pdf
Data publikacji:
2014
Wydawca:
Przedsiębiorstwo Wydawnictw Naukowych Darwin / Scientific Publishing House DARWIN
Tematy:
meteorites
Find
fall
NWA
chondrites
achondrites
Statistic
Morocco
Opis:
Since the first recorded discovery of a meteorite in 1937 near the Mrirt village (Khenifra, Morocco), a total of 946 authenticated meteorites have been recorded in Morocco. The material, including 10 observed falls, comprises 918 stones, 13 irons and 15 stony-irons. A low ratio of falls to finds (represent only 0.01 % of the Moroccan declared meteorites) compared with other countries (e.g., USA 14.3 %). However the rate of recovery of meteorites (falls + finds) in Morocco exceeds that of most other countries of similar size and range of climatic conditions. More than 95 % of documented meteorites from Morocco have been recovered from Eastern Morocco (Eastern Sahara Moroccan) including many rare types. This Region has proved to be one of the most prolific areas in the world for meteorite finds.
Źródło:
International Letters of Chemistry, Physics and Astronomy; 2014, 1; 18-25
2299-3843
Pojawia się w:
International Letters of Chemistry, Physics and Astronomy
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Próby klasyfikowania chondrytów zwyczajnych przez zastosowanie spektroskopii mössbauerowskiej
Attempts of classification of ordinary chondrites by application of Mössbauer spectroscopy
Autorzy:
Gałązka-Friedman, Jolanta
Woźniak, Marek
Duda, Przemysław
Jakubowska, Martyna
Bogusz, Patrycja
Karwowski, Łukasz
Powiązania:
https://bibliotekanauki.pl/articles/1032381.pdf
Data publikacji:
2019
Wydawca:
Polskie Towarzystwo Meteorytowe
Tematy:
Mössbauer spectroscopy
classification of meteorites
ordinary chondrites
Opis:
Mössbauer spectra of equilibrated ordinary chondrites consist of two sextets due to magnetically ordered iron present in metallic phases and troilite and two doublets due to paramagnetic iron present in olivines and pyroxenes. The Mössbauer spectral areas of the different mineralogical phases in meteorites are proportional to the number of iron ions present in olivines, pyroxenes, metallic phase and troilite. This property of Mössbauer spectra was the basis for constructing various methods for the classification of ordinary chondrites. Review of these methods will be presented.
Źródło:
Acta Societatis Metheoriticae Polonorum; 2019, 10; 23-28
2080-5497
Pojawia się w:
Acta Societatis Metheoriticae Polonorum
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
NWA 14360 – Nowy meteoryt z Nigru
A new meteorite from Niger: NWA 14360
Autorzy:
Karwowski, Łukasz
Szopa, Krzysztof
Powiązania:
https://bibliotekanauki.pl/articles/2034032.pdf
Data publikacji:
2022-03
Wydawca:
Polskie Towarzystwo Meteorytowe
Tematy:
ordinary chondrites
NWA 14360
meteorite
meteorites classification
Opis:
The new meteorite was bought as one single stone in 2019 from a dealer in Niger by Tomasz Jakubowski. The meteorite has fusion crust. It contains chondrules of different types with dominance of barred olivine chondrules, with diameter to 1.5 mm. Px and Ol are 78.1 vol%. of the meteorite mass. Pl is up 11.8 vol%. Average fayalite content is 24.93. Metallic phases are 3.0 vol%. Troilite is up to 5.9 vol%. Spinel (Cr-spinel) is up to 0.9 vol%. Average content of the secondary Fe-rich minerals (e.g. hydroxides) is 0.4 vol%. Feldspar composition is: Ab80.2Or5.0An14.8. Mean content of Al2O3, MgO and TiO2 in chromium spinel is 6.70 wt%, 2.05 wt% and 2.02 wt%, respectively. Metal phases are kamacite and tetrataenite. The kamacite has a Ni content in the range 5.83–6.81 wt%, while the Co content is in the range 0.39 to 0.56 wt%. Tetrataenite is has Ni content from 49.68 to 50.46 wt%, and Co up to 0.05 wt%. High-Ca monoclinic pyroxene, similar to diopside, is very rare. Accessory minerals are: chlorapatite and merrylite. Base on chemistry and petrography, the meteorite is classified as ordinary chondrite (L5). The main mass, a 9190 g specimen, is in Krzysztof Socha private collection. Small fragments with the total mass 71 g are stored in Museum of Earth Sciences (catalogue no: WNoZ/Mt/110) at University of Silesia in Katowice, Poland. 39 g was used for thin-section preparation and spectroscopic investigation (Mössbauer spectroscopy).
Źródło:
Acta Societatis Metheoriticae Polonorum; 2022, 13; 47-59
2080-5497
Pojawia się w:
Acta Societatis Metheoriticae Polonorum
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Comparative analysis of the Baszkówka and Mt. Tazerzait chondrites: genetic conclusions based on astrophysical data and the mineralogical and petrological data
Autorzy:
Pilski, A. S.
Przylibski, T. A.
Zagożdżon, P. P.
Powiązania:
https://bibliotekanauki.pl/articles/2059300.pdf
Data publikacji:
2001
Wydawca:
Państwowy Instytut Geologiczny – Państwowy Instytut Badawczy
Tematy:
meteorites
chondrites
solar system
asteroids
asteroid-collisions
Opis:
The L5 chondrites Baszkówka and Mt. Tazerzait are characterised. Their astronomical, mineralogical and petrological characteristics confirm that these meteorites are similar. They could be derived from the same parent body, though from the different depths below its surface. A third meteorite - the Tjerebon - might have arisen from the same swarm of meteoroids. The parent body to these meteorites in the asteroid belt can not be established at present. The porosity, of these chondrites suggests that they formed close to the surface of their parent asteroid. The process of formation of the parent rock of the Baszkówka chondrite is similar in some respects to sedimentation of a weakly compacted terrestrial sandstone. Thus, a two-stage geological history may be envisaged: firstly formation of the component minerals and mineral aggregates of this meteorite. Then, later in a different environment, the accretion of fragments of this parent material, together with a small amount of matrix, into a strongly porous sedimentary rock.
Źródło:
Geological Quarterly; 2001, 45, 3; 331-342
1641-7291
Pojawia się w:
Geological Quarterly
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Mineralogy of the Baszkówka chondrite (L5 S1): new data on silicates, opaques and minor minerals
Autorzy:
Borucki, J.
Stępniewski, M.
Powiązania:
https://bibliotekanauki.pl/articles/2059302.pdf
Data publikacji:
2001
Wydawca:
Państwowy Instytut Geologiczny – Państwowy Instytut Badawczy
Tematy:
Baszkówka
meteorites
ordinary chondrites
minerals
spinel
picotite
Opis:
The mineral composition of the Baszkówka meteorite comprises: olivine, pyroxenes, plagioclase, Fe,Ni metal, troilite and chromite with minor chlorapatite, whitlockite, magnetite, haematite, spinel, idaite, calcite and native Cu. A rare variety of spinel (picotite), probably the oldest among the minerals of Baszkówka, was identified in the only two chondrules named: panda and chevron. The composition of the olivine (Fa 26.2š1.8 wt.%) and the high degree of chondrite homogenisation, a result of thermal metamorphism, are consistent with earlier results and indicate the L5 group. No distinct shock effects were observed in Baszkówka, classified as S1. Troilite-Fe,Ni and Fe,Ni metal lumps are defined and interpreted as molten planetesimals impact splashes.
Źródło:
Geological Quarterly; 2001, 45, 3; 229-256
1641-7291
Pojawia się w:
Geological Quarterly
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Klast stopu impaktowego w brekcji pułtuskiej
Impact melt clast in the Pułtusk breccia
Autorzy:
Krzesińska, Agata M.
Powiązania:
https://bibliotekanauki.pl/articles/1033107.pdf
Data publikacji:
2018
Wydawca:
Polskie Towarzystwo Meteorytowe
Tematy:
H chondrites
Late Heavy Bombardment
Pułtusk
impact melt
Opis:
The Pułtusk H chondritic breccia records a complex impact history and contains various products of impact metamorphism. Here, impact melt lithology is described, which is embedded into the Pułtusk breccia. The impact melt clast is formed by microcrystalline quenched silicates and metal-troilite globules and chondritic relicts are retained in the melt. The relicts record strong shock deformation, S4–S5 and they have well developed foliated fabric of metal grains. The melt formed by severe collision and impact melting on the parent body. The chondritic material was superheated and molten. Silicate melt unmixed from the metal-sulphide melt and both were rapidly quenched. Most likely the event occurred during Late Heavy Bombardment, ~3.6 Ga.
Źródło:
Acta Societatis Metheoriticae Polonorum; 2018, 9; 74-91
2080-5497
Pojawia się w:
Acta Societatis Metheoriticae Polonorum
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Osłabianie promieniowania gamma w chondrytach zwyczajnych
Gamma rays attenuation in ordinary chondrites
Autorzy:
Kaczmarzyk, Marcin
Powiązania:
https://bibliotekanauki.pl/articles/1032387.pdf
Data publikacji:
2019
Wydawca:
Polskie Towarzystwo Meteorytowe
Tematy:
ISRU
asteroids
astronautics
cosmic rays
gamma rays attenuation
ordinary chondrites
Opis:
This paper elaborates on gamma rays attenuation in ordinary chondrites. Highly penetrating gamma radiation is emitted as a result of inelastic collisions of ultra-high energy cosmic particles with bulk matter, such as spacecraft hulls. Resources mined from Solar System small bodies may present an alternative construction material for spacecraft cosmic rays shields, which explains research on ionizing radiation attenuation in meteorites. A custom-made, shielded research workstation was constructed to analyse ionizing radiation absorption in pulverized materials. Using the workstation, gamma rays attenuation experiment was performed on pulverized ordinary chondrite – a meteorite originating from S-type asteroid. The experiment resulted in obtaining gamma ray mass attenuation coefficient of S-type chondritic asteroid matter. Obtained results were analysed and final conclusions were formulated. Per unit mass, ordinary chondrites exhibit better gamma rays attenuation properties than any radiation shielding material contemporarily used in astronautics.
W niniejszej pracy poruszono zagadnienie pochłaniania promieniowania gamma w materiale budującym meteoryty należące do grupy chondrytów zwyczajnych, które pochodzą z planetoid typu S. Wysoce przenikliwe promieniowanie gamma powstaje w przestrzeni kosmicznej m.in. jako efekt oddziaływania pierwotnego promieniowania kosmicznego z ośrodkami materialnymi. Materiał pozyskany z małych ciał Układu Słonecznego może stanowić alternatywny budulec ciężkich osłon radiacyjnych statków kosmicznych, co uzasadnia prowadzenie badań nad pochłanianiem promieniowania jonizującego w meteorytach. Opisano tu eksperyment, do celów którego wykonano autorskiej konstrukcji stanowisko badawcze do analizy pochłaniania promieniowania jonizującego w materiałach sypkich. Przy pomocy tego stanowiska, wykorzystując radioaktywny izotop 60Co, określono masowy współczynnik absorbcji promieniowania gamma w sproszkowanym chondrycie zwyczajnym, a otrzymany wynik porównano z wartością obliczoną teoretycznie. W pracy przeprowadzono szczegółową analizę uzyskanych wyników i sformułowano wnioski płynące z przeprowadzonego eksperymentu. Na jednostkę masy, chondryty zwyczajne lepiej osłabiają promieniowanie gamma niż jakiekolwiek materiały osłonowe stosowane obecnie w astronautyce.
Źródło:
Acta Societatis Metheoriticae Polonorum; 2019, 10; 40-50
2080-5497
Pojawia się w:
Acta Societatis Metheoriticae Polonorum
Dostawca treści:
Biblioteka Nauki
Artykuł
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