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10. Riding the wave towards flourishing in STEM education: Enhancing teaching efficacy through a K-12 training program

Author

Universidad de Alicante. Departamento de Psicología Evolutiva y Didáctica, Pozo-Rico, Teresa, Scott, Ricardo, Bąk, Magdalena, Castejón, Juan Luis, Gilar-Corbi, Raquel, Universidad de Alicante. Departamento de Psicología Evolutiva y Didáctica, Pozo-Rico, Teresa, Scott, Ricardo, Bąk, Magdalena, Castejón, Juan Luis, and Gilar-Corbi, Raquel

Abstract

The research aimed to analyze the effectiveness of a training program for K-12 teachers in improving their perceptions of flourishing, job satisfaction, work as meaning, and efficacy, as well as their students' academic performance. The study involved 147 K-12 teachers and 3544 students. A 'quasi-experimental' pretest-posttest with a control group design was adopted. The results showed significant improvements in students' academic performance and in all teacher variables in the experimental group. Targeting interventions towards K-12 educators has immense potential to profoundly influence students' academic growth by increasing their interest and competence in STEM disciplines.

Published
2024

16. New Light on Prions: Putative Role of PrP c in Pathophysiology of Mood Disorders.

Author

Chrobak, Adrian Andrzej, Pańczyszyn-Trzewik, Patrycja, Król, Patrycja, Pawelec-Bąk, Magdalena, Dudek, Dominika, and Siwek, Marcin

Subjects
AFFECTIVE disorders, PATHOLOGICAL physiology, DRUG target, NEUROPLASTICITY, COGNITION disorders, MELANOPSIN
Abstract

Mood disorders are highly prevalent and heterogenous mental illnesses with devastating rates of mortality and treatment resistance. The molecular basis of those conditions involves complex interplay between genetic and environmental factors. Currently, there are no objective procedures for diagnosis, prognosis and personalization of patients' treatment. There is an urgent need to search for novel molecular targets for biomarkers in mood disorders. Cellular prion protein (PrPc) is infamous for its potential to convert its insoluble form, leading to neurodegeneration in Creutzfeldt-Jacob disease. Meanwhile, in its physiological state, PrPc presents neuroprotective features and regulates neurotransmission and synaptic plasticity. The aim of this study is to integrate the available knowledge about molecular mechanisms underlying the impact of PrPc on the pathophysiology of mood disorders. Our review indicates an important role of this protein in regulation of cognitive functions, emotions, sleep and biological rhythms, and its deficiency results in depressive-like behavior and cognitive impairment. PrPc plays a neuroprotective role against excitotoxicity, oxidative stress and inflammation, the main pathophysiological events in the course of mood disorders. Research indicates that PrPc may be a promising biomarker of cognitive decline. There is an urgent need of human studies to elucidate its potential utility in clinical practice. [ABSTRACT FROM AUTHOR]

Published
2024
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17. In defence of travel. The importance of the journey in the Romantic era in Poland.

Author

Bąk, Magdalena

Abstract

Copyright of Tematy & Konteksty is the property of University of Rzeszow and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)

Published
2024
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18. SOBIE ŚPIEWAM A POLAKOM. O AUTORYTECIE CAMOESA W LITERATURZE POLSKIEJ DOBY ROMANTYZMU.

Author

BĄK, MAGDALENA

Abstract

Copyright of Prace Filologiczne. Literaturoznawstwo is the property of University of Warsaw and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)

Published
2024
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24. The impact of mineral and organic supplements on the abundance of selected groups of culturable microorganisms in soil contaminated with heavy metals.

Author

Wolny-Koładka, Katarzyna, Jarosz, Renata, Marcińska-Mazur, Lidia, Gondek, Krzysztof, Lahori, Altaf Hussain, Szara-Bąk, Magdalena, Lošák, Tomáš, Szerement, Justyna, Mokrzycki, Jakub, Karcz, Robert, and Mierzwa-Hersztek, Monika

Abstract

The impact of lignite and leonardite combined with a NaX-C composite on the abundance of selected groups of culturable micro-organisms in soil contaminated with Pb, Cd and Zn was tested. For this purpose, a 7-month incubation experiment and two-year pot experiments were conducted. The pattern of both experiments was analogous and included: soil without fertilization (C); soil fertilized with NPK mineral fertilizers (MF); soil with NPK + 3 or 6% lignite (MF+CW3%, MF+CW6%) and 3% zeolite-carbon composite (NaX-C); soil with NPK + 3 or 6% leonardite (MF+CL3%, MF+CL6%) and 3% zeolite-carbon composite (NaX-C). The test plant in the pot experiment was the Kosynier variety of maize. The soil material was used to estimate the abundance of general bacteria, mold fungi, actinomycetes (actinomycetales), ammonification bacteria and bacteria from the Azotobacter genus. The study found that the application of lignite and leonardite combined with a NaXC composite had generally contributed to a significant increase in the total nitrogen content and a decrease in the total carbon content in soil in the pot experiment. In general, the mineral-organic mixtures had a stimulating effect on the analyzed groups of soil microorganisms in both experiments, but the dominant groups in the pot experiment were total bacteria and ammonifying bacteria, while in the incubation experiment, fungi and actinomycetes were the prevalent groups. An RDA analysis indicated that mold fungi, bacteria, actinomycetes and amminofers were positively correlated with the EC, total nitrogen and carbon. [ABSTRACT FROM AUTHOR]

Published
2023
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26. Properties of slowly rotating asteroids from the Convex Inversion Thermophysical Model

Author

Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Marciniak, Anna, Ďurech, Josef, Alí-Lagoa, Víctor, Ogłoza, W., Szakáts, Róbert, Müller, Thomas G., Molnár, László, Pál, András, Monteiro, F., Arcoverde, P., Behrend, Raoul, Benkhaldoun, Zouhair, Bernasconi, Laurent, Bosch, J., Brincat, S., Brunetto, L., Butkiewicz-Bąk, Magdalena, Del Freo, F., Duffard, René, Evangelista-Santana, M., Farroni, G., Fauvaud, S., Fauvaud, M., Ferrais, Marin, Geier, Stefan, Golonka, J., Grice, Jonny, Hirsch, R., Horbowicz, J., Jehin, Emmanuel, Julien, P., Kalup, Cs., Kamiński, K., Kamińska, M.K., Kankiewicz, P., Kecskeméthy, V., Kim, D.-H., Kim, Myung-Jin, Konstanciak, I., Krajewski, J., Kudak, V., Kulczak, P., Kundera, T., Lazzaro, D., Manzini, F., Medeiros, H., Michimani-Garcia, J., Morales, Nicolás, Nadolny, J., Oszkiewicz, D., Pakštienė, E., Pawłowski, M., Perig, V., Pilcher, F., Pinel, P., Podlewska-Gaca, Edyta, Polakis, T., Richard, F., Rodrigues, T., Rondón, E., Roy, René, Sanabria, J.J., Santana-Ros, Toni, Skiff, B., Skrzypek, J., Sobkowiak, Krzysztof, Sonbas, E., Stachowski, G., Strajnic, J., Trela, P., Tychoniec, Ł., Urakawa, S., Verebelyi, E., Wagrez, K., Żejmo, M., Żukowski, K., Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Marciniak, Anna, Ďurech, Josef, Alí-Lagoa, Víctor, Ogłoza, W., Szakáts, Róbert, Müller, Thomas G., Molnár, László, Pál, András, Monteiro, F., Arcoverde, P., Behrend, Raoul, Benkhaldoun, Zouhair, Bernasconi, Laurent, Bosch, J., Brincat, S., Brunetto, L., Butkiewicz-Bąk, Magdalena, Del Freo, F., Duffard, René, Evangelista-Santana, M., Farroni, G., Fauvaud, S., Fauvaud, M., Ferrais, Marin, Geier, Stefan, Golonka, J., Grice, Jonny, Hirsch, R., Horbowicz, J., Jehin, Emmanuel, Julien, P., Kalup, Cs., Kamiński, K., Kamińska, M.K., Kankiewicz, P., Kecskeméthy, V., Kim, D.-H., Kim, Myung-Jin, Konstanciak, I., Krajewski, J., Kudak, V., Kulczak, P., Kundera, T., Lazzaro, D., Manzini, F., Medeiros, H., Michimani-Garcia, J., Morales, Nicolás, Nadolny, J., Oszkiewicz, D., Pakštienė, E., Pawłowski, M., Perig, V., Pilcher, F., Pinel, P., Podlewska-Gaca, Edyta, Polakis, T., Richard, F., Rodrigues, T., Rondón, E., Roy, René, Sanabria, J.J., Santana-Ros, Toni, Skiff, B., Skrzypek, J., Sobkowiak, Krzysztof, Sonbas, E., Stachowski, G., Strajnic, J., Trela, P., Tychoniec, Ł., Urakawa, S., Verebelyi, E., Wagrez, K., Żejmo, M., and Żukowski, K.

Abstract

Context. Recent results for asteroid rotation periods from the TESS mission showed how strongly previous studies have underestimated the number of slow rotators, revealing the importance of studying those targets. For most slowly rotating asteroids (those with P > 12 h), no spin and shape model is available because of observation selection effects. This hampers determination of their thermal parameters and accurate sizes. Also, it is still unclear whether signatures of different surface material properties can be seen in thermal inertia determined from mid-infrared thermal flux fitting. Aims. We continue our campaign in minimising selection effects among main belt asteroids. Our targets are slow rotators with low light-curve amplitudes. Our goal is to provide their scaled spin and shape models together with thermal inertia, albedo, and surface roughness to complete the statistics. Methods. Rich multi-apparition datasets of dense light curves are supplemented with data from Kepler and TESS spacecrafts. In addition to data in the visible range, we also use thermal data from infrared space observatories (mainly IRAS, Akari and WISE) in a combined optimisation process using the Convex Inversion Thermophysical Model. This novel method has so far been applied to only a few targets, and therefore in this work we further validate the method itself. Results. We present the models of 16 slow rotators, including two updated models. All provide good fits to both thermal and visible data.The obtained sizes are on average accurate at the 5% precision level, with diameters found to be in the range from 25 to 145 km. The rotation periods of our targets range from 11 to 59 h, and the thermal inertia covers a wide range of values, from 2 to <400 J m−2 s−1∕2 K−1, not showing any correlation with the period. Conclusions. With this work we increase the sample of slow rotators with reliable spin and shape models and known thermal inertia by 40%. The thermal inertia values of our sample d

Published
2021

27. Nienawidzę i kocham. Miejsce Mickiewicza i rola autorytetu w korespondencji Słowackiego

Author

Bąk, Magdalena

Subjects
Juliusz Słowacki, letters, Adam Mickiewicz, autorytet, anxiety of influence, korespondencja, lęk przed wpływem, authority
Abstract

Celem artykułu jest analiza wzmianek na temat Adama Mickiewicza pojawiających się w korespondencji Juliusza Słowackiego. Ich ambiwalentny charakter potwierdzać może przypuszczenie, że skomplikowana relacja pomiędzy poetami da się analizować za pomocą teorii „lęku przed wpływem” Harolda Blooma. W niniejszym szkicu fragmenty korespondencji dotyczące Mickiewicza analizowane są jednak w szerszym kontekście zmagań Słowackiego z problemem autorytetów w dziedzinie literatury. The aim of the article is to analyse references to Adam Mickiewicz that appear in Juliusz Słowacki’s letters. Ambivalent character of these references proves that complicated relationship between the two poets can be analysed through Harold Bloom’s “anxiety of influence” theory. In this article, however, letters referring to Mickiewicz are being analysed in a broader context − as an example of how Słowacki struggled with literary authority as such.

Published
2020

28. The large trans-Neptunian object 2002 TC302 from combined stellar occultation, photometry, and astrometry data

Author

Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante. Instituto Universitario de Investigación Informática, Ortiz Moreno, José Luis, Santos Sanz, Pablo, Sicardy, B., Benedetti-Rossi, G., Duffard, René, Morales Palomino, Nicolás, Braga-Ribas, F., Fernández-Valenzuela, Estela, Nascimbeni, V., Nardiello, D., Carbognani, A., Buzzi, Luca, Aletti, A., Bacci, P., Maestripieri, M., Mazzei, L., Mikuz, H., Skvarc, J., Ciabattari, F., Lavalade, F., Scarfi, G., Mari, J.M., Conjat, M., Sposetti, S., Bachini, M., Succi, G., Mancini, F., Alighieri, M., Dal Canto, E., Masucci, M., Vara-Lubiano, M., Gutiérrez, P.J., Desmars, Josselin, Lecacheux, J., Vieira-Martins, R., Camargo, J.I.B., Assafin, M., Colas, François, Beisker, W., Behrend, Raoul, Mueller, T.G., Meza, E., Gomes-Junior, A.R., Roques, F., Vachier, Frédéric, Mottola, S., Hellmich, S., Campo Bagatin, Adriano, Alvarez-Candal, Alvaro, Cikota, S., Cikota, A., Christille, J.M., Pál, András, Kiss, C., Pribulla, T., Komžík, R., Madiedo, J.M., Charmandaris, V., Alikakos, J., Szakáts, Róbert, Farkas, Anikó, Varga-Verebélyi, E., Marton, G., Marciniak, Anna, Bartczak, Przemyslaw, Butkiewicz-Bąk, Magdalena, Dudziński, Grzegorz, Alí-Lagoa, Víctor, Gazeas, K., Paschalis, N., Tsamis, V., Guirado, J.C., Peris, V., Iglesias-Marzoa, R., Schnabel, C., Manzano, F., Navarro, A., Perelló, C., Vecchione, A., Noschese, A., Morrone, L., Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante. Instituto Universitario de Investigación Informática, Ortiz Moreno, José Luis, Santos Sanz, Pablo, Sicardy, B., Benedetti-Rossi, G., Duffard, René, Morales Palomino, Nicolás, Braga-Ribas, F., Fernández-Valenzuela, Estela, Nascimbeni, V., Nardiello, D., Carbognani, A., Buzzi, Luca, Aletti, A., Bacci, P., Maestripieri, M., Mazzei, L., Mikuz, H., Skvarc, J., Ciabattari, F., Lavalade, F., Scarfi, G., Mari, J.M., Conjat, M., Sposetti, S., Bachini, M., Succi, G., Mancini, F., Alighieri, M., Dal Canto, E., Masucci, M., Vara-Lubiano, M., Gutiérrez, P.J., Desmars, Josselin, Lecacheux, J., Vieira-Martins, R., Camargo, J.I.B., Assafin, M., Colas, François, Beisker, W., Behrend, Raoul, Mueller, T.G., Meza, E., Gomes-Junior, A.R., Roques, F., Vachier, Frédéric, Mottola, S., Hellmich, S., Campo Bagatin, Adriano, Alvarez-Candal, Alvaro, Cikota, S., Cikota, A., Christille, J.M., Pál, András, Kiss, C., Pribulla, T., Komžík, R., Madiedo, J.M., Charmandaris, V., Alikakos, J., Szakáts, Róbert, Farkas, Anikó, Varga-Verebélyi, E., Marton, G., Marciniak, Anna, Bartczak, Przemyslaw, Butkiewicz-Bąk, Magdalena, Dudziński, Grzegorz, Alí-Lagoa, Víctor, Gazeas, K., Paschalis, N., Tsamis, V., Guirado, J.C., Peris, V., Iglesias-Marzoa, R., Schnabel, C., Manzano, F., Navarro, A., Perelló, C., Vecchione, A., Noschese, A., and Morrone, L.

Abstract

Context. Deriving physical properties of trans-Neptunian objects is important for the understanding of our Solar System. This requires observational efforts and the development of techniques suitable for these studies. Aims. Our aim is to characterize the large trans-Neptunian object (TNO) 2002 TC302. Methods. Stellar occultations offer unique opportunities to determine key physical properties of TNOs. On 28 January 2018, 2002 TC302 occulted a mv ~ 15.3 star with designation 593-005847 in the UCAC4 stellar catalog, corresponding to Gaia source 130957813463146112. Twelve positive occultation chords were obtained from Italy, France, Slovenia, and Switzerland. Also, four negative detections were obtained near the north and south limbs. This represents the best observed stellar occultation by a TNO other than Pluto in terms of the number of chords published thus far. From the 12 chords, an accurate elliptical fit to the instantaneous projection of the body can be obtained that is compatible with the near misses. Results. The resulting ellipse has major and minor axes of 543 ± 18 km and 460 ± 11 km, respectively, with a position angle of 3 ± 1 degrees for the minor axis. This information, combined with rotational light curves obtained with the 1.5 m telescope at Sierra Nevada Observatory and the 1.23 m telescope at Calar Alto observatory, allows us to derive possible three-dimensional shapes and density estimations for the body based on hydrostatic equilibrium assumptions. The effective diameter in equivalent area is around 84 km smaller than the radiometrically derived diameter using thermal data from Herschel and Spitzer Space Telescopes. This might indicate the existence of an unresolved satellite of up to ~300 km in diameter, which is required to account for all the thermal flux, although the occultation and thermal diameters are compatible within their error bars given the considerable uncertainty of the thermal results. The existence of a potential satellite also a

Published
2020

29. Physical parameters of selected Gaia mass asteroids

Author

Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Podlewska-Gaca, Edyta, Marciniak, Anna, Alí-Lagoa, Víctor, Bartczak, Przemyslaw, Müller, Thomas G., Szakáts, Róbert, Duffard, René, Molnár, László, Pál, András, Butkiewicz-Bąk, Magdalena, Dudziński, Grzegorz, Dziadura, Karolina, Antonini, Pierre, Asenjo, Víctor, Audejean, Maurice, Benkhaldoun, Zouhair, Behrend, Raoul, Bernasconi, Laurent, Bosch, Josep M., Chapman, Andrés, Dintinjana, Bojan, Farkas, Anikó, Ferrais, Marin, Geier, Stefan, Grice, Jonny, Hirsh, Roman, Jacquinot, Herve, Jehin, Emmanuel, Jones, A., Molina, David, Morales, Nicolás, Parley, Neil, Poncy, R., Roy, René, Santana-Ros, Toni, Seli, Bálint, Sobkowiak, Krzysztof, Verebélyi, Erika, Żukowski, K., Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Podlewska-Gaca, Edyta, Marciniak, Anna, Alí-Lagoa, Víctor, Bartczak, Przemyslaw, Müller, Thomas G., Szakáts, Róbert, Duffard, René, Molnár, László, Pál, András, Butkiewicz-Bąk, Magdalena, Dudziński, Grzegorz, Dziadura, Karolina, Antonini, Pierre, Asenjo, Víctor, Audejean, Maurice, Benkhaldoun, Zouhair, Behrend, Raoul, Bernasconi, Laurent, Bosch, Josep M., Chapman, Andrés, Dintinjana, Bojan, Farkas, Anikó, Ferrais, Marin, Geier, Stefan, Grice, Jonny, Hirsh, Roman, Jacquinot, Herve, Jehin, Emmanuel, Jones, A., Molina, David, Morales, Nicolás, Parley, Neil, Poncy, R., Roy, René, Santana-Ros, Toni, Seli, Bálint, Sobkowiak, Krzysztof, Verebélyi, Erika, and Żukowski, K.

Abstract

Context. Thanks to the Gaia mission, it will be possible to determine the masses of approximately hundreds of large main belt asteroids with very good precision. We currently have diameter estimates for all of them that can be used to compute their volume and hence their density. However, some of those diameters are still based on simple thermal models, which can occasionally lead to volume uncertainties as high as 20–30%. Aims. The aim of this paper is to determine the 3D shape models and compute the volumes for 13 main belt asteroids that were selected from those targets for which Gaia will provide the mass with an accuracy of better than 10%. Methods. We used the genetic Shaping Asteroids with Genetic Evolution (SAGE) algorithm to fit disk-integrated, dense photometric lightcurves and obtain detailed asteroid shape models. These models were scaled by fitting them to available stellar occultation and/or thermal infrared observations. Results. We determine the spin and shape models for 13 main belt asteroids using the SAGE algorithm. Occultation fitting enables us to confirm main shape features and the spin state, while thermophysical modeling leads to more precise diameters as well as estimates of thermal inertia values. Conclusions. We calculated the volume of our sample of main-belt asteroids for which the Gaia satellite will provide precise mass determinations. From our volumes, it will then be possible to more accurately compute the bulk density, which is a fundamental physical property needed to understand the formation and evolution processes of small Solar System bodies.

Published
2020

33. Zbrodnia to niesłychana, / Pani zabija pana

Author

Bąk, Magdalena

Subjects
Adam Mickiewicz, cytat, ballada
Abstract

Cytat ten otwiera balladę Lilije pochodzącą ze zbioru Ballady i romanse, wydrukowanego w pierwszym tomie Poezji Adama Mickiewicza w 1822 roku (Fragment tekstu).

Published
2018

34. Precz z moich oczu!… posłucham od razu

Author

Bąk, Magdalena

Subjects
Adam Mickiewicz, cytat, poezja
Abstract

Fraza pochodzi z liryku Mickiewicza Do M***. Wiersz napisany w 1823 roku rozpoczyna się następującą strofą... (Fragment tekstu)

Published
2018

35. Chodzi mi o to, aby język giętki / Powiedział wszystko, co pomyśli głowa

Author

Bąk, Magdalena

Subjects
Juliusz Słowacki, poemat, cytat
Abstract

Słowa te pochodzą z Pieśni V poematu Beniowski Juliusza Słowackiego i podejmują ważną dla romantyzmu kwestię języka oraz możliwości wyrażenia w nim wszystkiego, o czym pomyśli poeta (Fragment tekstu).

Published
2018

36. Znasz ty Ewangeliją?

Author

Bąk, Magdalena

Subjects
Adam Mickiewicz, cytat, poezja
Abstract

Słowa te pochodzą z części IV cyklu Dziady Adama Mickiewicza. Wypowiada je Ksiądz, który, widząc, że jego gość – Pustelnik (będący, jak się później okaże, jego dawnym uczniem), pragnie popełnić samobójstwo z powodu nieszczęśliwej miłości, oburza się na „taką myśl bezbożną” i zadaje cytowane pytanie: „Znasz ty Ewangeliją?” (Fragment tekstu).

Published
2018

37. Nie miecz, nie tarcz bronią Języka, / Lecz – arcydzieła!

Author

Bąk, Magdalena

Subjects
cytat, Cyprian Kamil Norwid, poezja
Abstract

Słowa te pochodzą z wiersza Cypriana Kamila Norwida Język-ojczysty. Są one odpowiedzią, której Lirnik udziela Energumenowi, domagającemu się czynów zbrojnych w sytuacji, kiedy „Wróg pokalał już i Ojców mowę” (Fragment tekstu).

Published
2018

38. Bez serc, bez ducha, to szkieletów ludy

Author

Bąk, Magdalena

Subjects
Adam Mickiewicz, cytat, poezja
Abstract

Jest to inicjalny wers Ody do młodości Adama Mickiewicza, wiersza napisanego w grudniu 1820 roku. Słowa te odnoszą się do ludzi, którzy żyją bez uczuć, nie znają życiowych prawd, postrzegają świat jedynie w kategoriach nauk ścisłych, są pozbawieni wrażliwości i wyobraźni. Ich rzeczywistość opisuje poeta jako starą, chylącą się ku upadkowi i przeciwstawia jej świat nowy, należący do młodych zapaleńców. Sformułowana w utworze pochwała młodości („ty nad poziomy wylatuj”) ukazuje ją jako siłę, która pozwala sięgać po więcej, przełamywać wszystkie ograniczenia i osiągać najwyższe cele: „Tam sięgaj, gdzie wzrok nie sięga, / Łam, czego rozum nie złamie”. Młodość w ujęciu poety ma również siłę jednoczącą, a wspólne wysiłki jej wyznawców mogą „pchnąć z posad bryłę świata”. Finał ody jest zapowiedzią nadejścia nowych czasów, triumfu wolności i swobody (Fragment tekstu).

Published
2018

39. Miej serce i patrzaj w serce!

Author

Bąk, Magdalena

Subjects
Adam Mickiewicz, cytat, poezja
Abstract

Cytat jest pointą ballady Romantyczność z cyklu Ballady i romanse zawartego w pierwszym tomie Poezji Adama Mickiewicza z 1822 roku. Stanowi podsumowanie wyrażonego w dwóch ostatnich strofach utworu romantycznego światopoglądu, w którym najważniejszą rolę odgrywają „czucie i wiara” przeciwstawione „szkiełku i oku” reprezentującym w wierszu metody poznawcze charakterystyczne dla minionej epoki oświecenia (Fragment tekstu).

Published
2018

40. Polały się łzy me czyste

Author

Bąk, Magdalena

Subjects
Adam Mickiewicz, cytat, poezja
Abstract

Utwór został napisany w czasie pobytu Mickiewicza w Lozannie i wchodzi w skład cyklu liryków lozańskich. Ten „wiersz-płacz” (jak go genialnie określił Julian Przyboś) jest swoistym rozrachunkiem z życiem, którego trzy kluczowe etapy (dzieciństwo, młodość, wiek męski) podmiot próbuje ocenić i podsumować (Fragment tekstu).

Published
2018

41. Już był w ogródku, już witał się z gąską

Author

Bąk, Magdalena

Subjects
Adam Mickiewicz, cytat, bajka
Abstract

Słowa te otwierają bajkę Lis i kozioł, stanowiącą Mickiewiczowską wersję popularnego motywu obecnego zarówno w utworach Ezopa, jak i La Fontaine’a. Apolog (krótki alegoryczny utwór dydaktyczno--moralizatorski) opowiada o lisie, który w pogoni za zdobyczą nie zauważa wkopanej w ziemię beczki na deszczówkę i wpada w pułapkę (Fragment tekstu).

Published
2018

42. Jękły głuche kamienie – / Ideał sięgnął bruku – –

Author

Bąk, Magdalena

Subjects
cytat, Cyprian Kamil Norwid, poezja
Abstract

Słowa te pochodzą z finału wiersza Cypriana Kamila Norwida Fortepian Szopena. Został on włączony do zbioru Vade-mecum, a nawoływanie kończące utwór w całości brzmi: „Ciesz się, późny wnuku!… / Jękły głuche kamienie – / Ideał sięgnął bruku – – ”. Słowa te są poetycką interpretacją obrazu przedstawionego w drugiej części wiersza, a ukazującego fortepian Chopina wyrzucany na bruk z płonącego budynku (Fragment tekstu).

Published
2018

43. Na wyrywki : 100 cytatów z polskiej poezji i dramatu, które powinien znać także cudzoziemiec

Author

Cudak, Romuald, Hajduk-Gawron, Wioletta, Madej, Agnieszka, Antoniewicz, Adam, Bąk, Magdalena, Gęsina, Tomasz, Morcinek-Abramczyk, Barbara, Romaniszyn-Ziomek, Lidia, and Smereczniak, Małgorzata

Subjects
quotations from Polish, drama, Polish literature, dictionary, poetry
Abstract

The book is addressed to young people and can be used as a language and literature handbook. It is said that to truly know a foreign language is to know its resource of lexicalized phrases and to use it without hindrance, on a random basis. The aim of the Lexicon is to help foreigners develop their linguistic and cultural competence in the field of Polish language and culture. The entries were collected on the basis of research published so far concerning quotations and winged words, as well as a survey conducted among humanists, active philologists teaching Polish language, literature and culture as native and foreign. The results of the survey allowed to verify the knowledge accumulated in the texts with the certified “life” of quotations. The excerpts from various periods of Polish literature are collected here and concern a wide range of its thematic areas. In general, they can be divided into the following categories: classical poetry, poetry and drama until the beginning of the 20th century, contemporary poetry, patriotic and religious songs. However, in the descriptions of individual entries, the authors do not note these categories. Each quotation is described according to a fixed structure. Readers will find here information about a literary fragment (its source), about the author of a quotation and his works, references, that is a reference to the functioning of a quotation in various texts of culture – in other poems, films, often in songs, or advertising slogans. The “It is worth knowing” section usually contains literary terms, but they are often explanations of the historical or political context. The authors of the entries also used excerpts from the publications of Polish researchers concerning a specific quotation, work or life of an artist. Each entry also includes a bibliography, which can be a source of further research for people interested in the topic. The indexes at the end of the publication are an element that organizes the entries and helps to search for quotations, their sources and authors’ names.

Published
2018

44. Samotność – cóż po ludziach

Author

Bąk, Magdalena

Subjects
Adam Mickiewicz, cytat, Dziady
Abstract

Słowa: „Samotność – cóż po ludziach, czym śpiewak dla ludzi?”, otwierają słynną Wielką Improwizację wygłoszoną przez Konrada w scenie II aktu I Dziadów części III (Fragment tekstu).

Published
2018

45. Odpowiednie dać rzeczy słowo!

Author

Bąk, Magdalena

Subjects
cytat, Cyprian Kamil Norwid, poezja
Abstract

Słowa te pochodzą z wiersza Ogólniki ze zbioru Vade-mecum Cypriana Kamila Norwida i opisują istotę sztuki poetyckiej, której zadaniem jest według poety właśnie „odpowiednie dać rzeczy słowo”. „Odpowiednie” można tu rozumieć na wiele sposobów (Fragment tekstu).

Published
2018

49. The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation

Author

Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Ortiz Moreno, José Luis, Santos Sanz, Pablo, Sicardy, B., Benedetti-Rossi, G., Bérard, D., Morales Palomino, Nicolás, Duffard, René, Braga-Ribas, F., Hopp, U., Ries, C., Nascimbeni, V., Marzari, F., Granata, V., Pál, András, Kiss, C., Pribulla, T., Komžík, R., Hornoch, K., Pravec, Petr, Bacci, P., Maestripieri, M., Nerli, L., Mazzei, L., Bachini, M., Martinelli, F., Succi, G., Ciabattari, F., Mikuz, H., Carbognani, A., Gaehrken, B., Mottola, S., Hellmich, S., Rommel, F.L., Fernández-Valenzuela, Estela, Campo Bagatin, Adriano, Cikota, S., Cikota, A., Lecacheux, J., Vieira-Martins, R., Camargo, J.I.B., Assafin, M., Colas, François, Behrend, Raoul, Desmars, Josselin, Meza, E., Alvarez-Candal, Alvaro, Beisker, W., Gomes-Junior, A.R., Morgado, B.E., Roques, F., Vachier, Frédéric, Berthier, Jérôme, Mueller, T.G., Madiedo, J.M., Unsalan, O., Sonbas, E., Karaman, N., Erece, O., Koseoglu, D.T., Ozisik, T., Kalkan, S., Guney, Y., Niaei, M.S., Satir, O., Yesilyaprak, C., Puskullu, C., Kabas, A., Demircan, O., Alikakos, J., Charmandaris, V., Leto, G., Ohlert, J., Christille, J.M., Szakáts, Róbert, Takácsné Farkas, A., Varga-Verebélyi, E., Marton, G., Marciniak, Anna, Bartczak, Przemyslaw, Santana-Ros, Toni, Butkiewicz-Bąk, Magdalena, Dudziński, Grzegorz, Alí-Lagoa, Víctor, Gazeas, K., Tzouganatos, L., Paschalis, N., Tsamis, V., Sánchez-Lavega, A., Pérez-Hoyos, S., Hueso, R., Guirado, J.C., Peris, V., Iglesias-Marzoa, R., Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Ortiz Moreno, José Luis, Santos Sanz, Pablo, Sicardy, B., Benedetti-Rossi, G., Bérard, D., Morales Palomino, Nicolás, Duffard, René, Braga-Ribas, F., Hopp, U., Ries, C., Nascimbeni, V., Marzari, F., Granata, V., Pál, András, Kiss, C., Pribulla, T., Komžík, R., Hornoch, K., Pravec, Petr, Bacci, P., Maestripieri, M., Nerli, L., Mazzei, L., Bachini, M., Martinelli, F., Succi, G., Ciabattari, F., Mikuz, H., Carbognani, A., Gaehrken, B., Mottola, S., Hellmich, S., Rommel, F.L., Fernández-Valenzuela, Estela, Campo Bagatin, Adriano, Cikota, S., Cikota, A., Lecacheux, J., Vieira-Martins, R., Camargo, J.I.B., Assafin, M., Colas, François, Behrend, Raoul, Desmars, Josselin, Meza, E., Alvarez-Candal, Alvaro, Beisker, W., Gomes-Junior, A.R., Morgado, B.E., Roques, F., Vachier, Frédéric, Berthier, Jérôme, Mueller, T.G., Madiedo, J.M., Unsalan, O., Sonbas, E., Karaman, N., Erece, O., Koseoglu, D.T., Ozisik, T., Kalkan, S., Guney, Y., Niaei, M.S., Satir, O., Yesilyaprak, C., Puskullu, C., Kabas, A., Demircan, O., Alikakos, J., Charmandaris, V., Leto, G., Ohlert, J., Christille, J.M., Szakáts, Róbert, Takácsné Farkas, A., Varga-Verebélyi, E., Marton, G., Marciniak, Anna, Bartczak, Przemyslaw, Santana-Ros, Toni, Butkiewicz-Bąk, Magdalena, Dudziński, Grzegorz, Alí-Lagoa, Víctor, Gazeas, K., Tzouganatos, L., Paschalis, N., Tsamis, V., Sánchez-Lavega, A., Pérez-Hoyos, S., Hueso, R., Guirado, J.C., Peris, V., and Iglesias-Marzoa, R.

Abstract

Haumea—one of the four known trans-Neptunian dwarf planets—is a very elongated and rapidly rotating body1, 2, 3. In contrast to other dwarf planets4, 5, 6, its size, shape, albedo and density are not well constrained. The Centaur Chariklo was the first body other than a giant planet known to have a ring system7, and the Centaur Chiron was later found to possess something similar to Chariklo’s rings8, 9. Here we report observations from multiple Earth-based observatories of Haumea passing in front of a distant star (a multi-chord stellar occultation). Secondary events observed around the main body of Haumea are consistent with the presence of a ring with an opacity of 0.5, width of 70 kilometres and radius of about 2,287 kilometres. The ring is coplanar with both Haumea’s equator and the orbit of its satellite Hi’iaka. The radius of the ring places it close to the 3:1 mean-motion resonance with Haumea’s spin period—that is, Haumea rotates three times on its axis in the time that a ring particle completes one revolution. The occultation by the main body provides an instantaneous elliptical projected shape with axes of about 1,704 kilometres and 1,138 kilometres. Combined with rotational light curves, the occultation constrains the three-dimensional orientation of Haumea and its triaxial shape, which is inconsistent with a homogeneous body in hydrostatic equilibrium. Haumea’s largest axis is at least 2,322 kilometres, larger than previously thought, implying an upper limit for its density of 1,885 kilograms per cubic metre and a geometric albedo of 0.51, both smaller than previous estimates1, 10, 11. In addition, this estimate of the density of Haumea is closer to that of Pluto than are previous estimates, in line with expectations. No global nitrogen- or methane-dominated atmosphere was detected.

Published
2017

50. 'Fado' po polsku : o portugalskim motywie w tytułach polskich dzieł (nie tylko) literackich (Danilewicz-Zielińska, Stasiuk, Kadłubek, Słabuszewska-Krauze)

Author

Bąk, Magdalena

Subjects
literatura polska, Maria Danilewicz-Zielińska, Zbigniew Kadłubek, Andrzej Stasiuk, Iwona Słabuszewska-Krauze, kultura portugalska
Abstract

The aim of the text is to examine the way in which the word fado, one of the most recognisable keywords of Portuguese culture, was used in the titles of contemporary Polish texts representing various genres and types of literature. The selection of the titles as a material for the analysis was determined by the belief (justified by research works) that the title constitutes an exceptionally important element of the work, entering in complex interactions of various kinds with the text of the work.

Published
2016

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