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91.
Vključevanje zaposlenih v delovno okolje v SPE Mehatronika v Iskri Avtoelektriki, d. d.
Ivan Anželj, 2008, undergraduate thesis

Found in: osebi
Keywords: diplomske naloge, motivacija, komunikacija, inovativnost
Published: 15.10.2013; Views: 4260; Downloads: 300
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92.
Vloga, znanje in zaželene osebnostne lastnosti mentorjev v podjetju Iskra Avtoelektrika
Tatjana Štakul, 2010, undergraduate thesis

Found in: osebi
Keywords: diplomske naloge, mentoriranje, pripravništvo, izobraževanje, mentorji
Published: 15.10.2013; Views: 3956; Downloads: 355
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93.
Trends that will shape the professions of the future information society
Tanja Urbančič, Alenka Stanič, 2009, original scientific article

Found in: osebi
Keywords: informacijska družba, upravljanje z znanjem, trajnostni razvoj, poklici prihodnosti
Published: 10.07.2015; Views: 3945; Downloads: 16
URL Fulltext (0,00 KB)

94.
Prenova proizvodnega procesa v podjetju Esal
Ana Stanič, 2011, undergraduate thesis

Found in: osebi
Keywords: diplomske naloge, vlaknocementni izdelki, proizvodnja, organizacija, prenova
Published: 15.10.2013; Views: 6597; Downloads: 378
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95.
Ugotavljanje prisotnosti polutantov btx (benzena, toluena in ksilena) iz prometa v tleh
Matjaž Stanič, 2009, undergraduate thesis

Found in: osebi
Keywords: benzen, toluen, ksilen, prometno onesnaževanje, plinska kromatografija, diplomske naloge
Published: 15.10.2013; Views: 5615; Downloads: 361
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The flux of ultra-high energy cosmic rays after ten years of operation of the Pierre Auger Observatory
Marko Zavrtanik, Danilo Zavrtanik, Lili Yang, Serguei Vorobiov, Darko Veberič, Marta Trini, Samo Stanič, Ahmed Saleh, Gašper Kukec Mezek, Andrej Filipčič, Inés Valiño, 2015, published scientific conference contribution

Abstract: The flux of ultra-high energy cosmic rays has been measured with unprecedented precision at the Pierre Auger Observatory. We report an update of the all-sky flux of cosmic rays above 3 x 10 [sup] 17 eV obtained by combining four independent data sets. These measurements are based on data from the surface detector arrays (divided into two sets according to the shower zenith angle), from a nested, denser, detector array, and hybrid events measured simultaneously with both the fluorescence detector and the surface detector array. The spectral features are presented in detail and the systematic uncertainties are addressed. The huge amount of data collected to date, with a total exposure exceeding 50,000 km2 sr yr, together with the wide range of sky observed (in declination from -90[deg] to 45[deg]) also allow us to measure the energy spectrum from different regions of the sky. We present the results of the search for a dependence of the measured flux on the declination of the incoming directions.
Found in: osebi
Keywords: ultra-high energy cosmic rays energy spectrum Pierre Auger Observatory
Published: 02.03.2016; Views: 4439; Downloads: 193
.pdf Fulltext (755,08 KB)

100.
Arrival directions of the highest-energy cosmic rays detected with the Pierre Auger Observatory
Marko Zavrtanik, Danilo Zavrtanik, Lili Yang, Serguei Vorobiov, Darko Veberič, Marta Trini, Samo Stanič, Ahmed Saleh, Gašper Kukec Mezek, Andrej Filipčič, Julien Aublin, 2015, published scientific conference contribution

Abstract: We present the results of a search for small to intermediate scale anisotropies in the distribution of arrival directions of ultra-high energy cosmic rays recorded at the Pierre Auger Observatory. The data set, gathered in ten years of operation, includes arrival directions with zenith angles up to 80◦, and is about three times larger than that used in earlier studies. We update the test based on correlations with active galactic nuclei (AGNs) from the Véron-Cetty and Véron catalog, which does not yield a significant indication of anisotropy with the present data set. We perform a blind search for localized excess fluxes and for self-clustering of arrival directions at angular scales up to 30◦ and for different energy thresholds between 40 EeV and 80 EeV. We also examine the correlation of arrival directions with relatively nearby galaxies in the 2MRS catalog, AGNs detected by Swift-BAT, and a sample of radio galaxies with jets and with the Centaurus A galaxy. None of the searches shows a statistically significant evidence of anisotropy. The two largest departures from isotropy that were found have a post-trial probability ≈ 1.4%. One is for cosmic rays with energy above 58 EeV that arrive within 15◦ of the direction toward Centaurus A. The other is for arrival directions within 18◦ of Swift-BAT AGNs closer than 130 Mpc and brighter than 10[sup]44 erg/s, with the same energy threshold.
Found in: osebi
Keywords: ultra-high energy cosmic rays anisotropy studies active galactic nuclei Pierre Auger Observatory
Published: 02.03.2016; Views: 3887; Downloads: 201
.pdf Fulltext (1,32 MB)

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