Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Szymon Gburek"'
Publikováno v:
Sensors, Vol 23, Iss 19, p 8095 (2023)
The Gas Electron Multiplier (GEM) was introduced by Fabio Sauli in 1997. This technology is broadly used in current and planned High-Energy Physics (HEP) experiments. One of the key components of these detectors is a readout board, which collects cha
Externí odkaz:
https://doaj.org/article/9d36b102425a4e96824083c2b3c3732d
Autor:
Jakub Ciazela, Jaroslaw Bakala, Miroslaw Kowalinski, Stefan Plocieniak, Natalia Zalewska, Bartosz Pieterek, Tomasz Mrozek, Marta Ciazela, Grzegorz Paslawski, Marek Steslicki, Zaneta Szaforz, Jaromir Barylak, Mateusz Kuzaj, Alessandro Maturilli, Joern Helbert, Andrzej Muszynski, Miroslaw Rataj, Szymon Gburek, Mateusz Jozefowicz, Dariusz Marciniak
Publikováno v:
Remote Sensing, Vol 14, Iss 12, p 2799 (2022)
Sulfide ores are a major source of noble (Au, Ag, and Pt) and base (Cu, Pb, Zn, Sn, Co, Ni, etc.) metals and will, therefore, be vital for the self-sustainment of future Mars colonies. Martian meteorites are rich in sulfides, which is reflected in re
Externí odkaz:
https://doaj.org/article/2e9eab2296cf473c896f546bf2a6d9fe
Autor:
M. Steslicki, Marek Siarkowski, Szymon Gburek, M. Gryciuk, Tomasz Mrozek, J. Barylak, A. Barylak, Piotr Podgorski
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 179:94-96
The Spectrometer Telescope for Imaging X-rays (STIX) is one of the instruments installed onboard Solar Orbiter mission which will be launched in February 2020. After 1.5 years of cruise phase it will start to gather scientific data from the orbit wit
Autor:
Barbara Sylwester, Szymon Gburek, Anna Kepa, Janusz Sylwester, Magdalena Gryciuk, Tomasz Mrozek, Marek Siarkowski
Publikováno v:
Solar Physics. 293
In 2009, the Russian Complex Orbital Observations Near-Earth of Activity of the Sun (CORONAS-Photon) spacecraft was launched, carrying the Polish Solar PHotometer In X-rays (SphinX). The SphinX was most sensitive in the spectral range 1.2 – 15 keV,
Autor:
Piotr Podgorski, Anna Kepa, Magdalena Gryciuk, Szymon Gburek, Janusz Sylwester, Tomasz Mrozek, Marek Siarkowski
Publikováno v:
Proceedings of the International Astronomical Union. 11:89-94
We propose a new model for description of solar flare lightcurve profile observed in soft X-rays. The method assumes that single-peaked ‘regular’ flares seen in lightcurves can be fitted with the elementary time profile being a convolution of Gau
Autor:
Barbara Sylwester, Anna Kepa, Janusz Sylwester, M. Gryciuk, Szymon Gburek, Marek Siarkowski, Piotr Podgorski, Tomasz Mrozek
Publikováno v:
Solar Physics. 292
A new methodology is given to determine basic parameters of flares from their X-ray light curves. Algorithms are developed from the analysis of small X-ray flares occurring during the deep solar minimum of 2009, between Solar Cycles 23 and 24, observ
Autor:
O. V. Dudnik, Szymon Gburek, Miroslaw Kowalinski, Piotr Podgorski, Marek Siarkowski, Jaroslaw Bakala, S. Płocieniak, Janusz Sylwester
Publikováno v:
Solar System Research. 46:160-169
A joint analysis is carried out of data obtained with the help of the solar X-ray SphinX spectrophotometer and the electron and proton satellite telescope STEP-F in May 2009 in the course of the scientific space experiment CORONAS-PHOTON. In order to
Autor:
Barbara Sylwester, K. J. H. Phillips, S. Płocieniak, Fabio Reale, Jaroslaw Bakala, Marek Siarkowski, Yu. D. Kotov, W. Trzebiński, Szymon Gburek, Sergey Kuzin, Piotr Podgorski, A. A. Pertsov, František Fárník, Miroslaw Kowalinski, Janusz Sylwester, Z. Kordylewski
Publikováno v:
Solar System Research. 45:189-199
The goals and construction details of a new design Polish-led X-ray spectrophotometer are described. The instrument is aimed to observe emission from entire solar corona and is placed as a separate block within the Russian TESIS X- and EUV complex ab
Autor:
Anna Kepa, W. Trzebiński, Barbara Sylwester, Piotr Podgorski, Z. Kordylewski, Szymon Gburek, Janusz Sylwester, S. Płocieniak, Sergey Kuzin, Miroslaw Kowalinski, Jaroslaw Bakala, Marek Siarkowski
Publikováno v:
Solar System Research. 45:182-187
Solar Photometer in X-rays (SphinX) is an instrument designed to observe the Sun in X-rays in the energy range 0.85–15.00 keV. SphinX is incorporated within the Russian TESIS X and EUV telescope complex aboard the CORONAS-Photon satellite which was
Publikováno v:
Advances in Space Research. 42:822-827
We use simultaneous observations from RESIK and RHESSI instruments to compare plasma properties of a major solar flare in its rise and gradual phase. This event occurred on 2002 August 3 (peak time at 19:06 UT). The flare had a very good coverage wit