Zobrazeno 1 - 10
of 22
pro vyhledávání: '"Steslicki, Marek"'
Autor:
Ciazela, Jakub, Bakala, Jaroslaw, Kowalinski, Miroslaw, Pieterek, Bartosz, Steslicki, Marek, Ciazela, Marta, Paslawski, Grzegorz, Zalewska, Natalia, Sterczewski, Lukasz, Szaforz, Zaneta, Jozefowicz, Mateusz, Marciniak, Dariusz, Fitt, Maciej, Sniadkowski, Adam, Rataj, Mirosław, Mrozek, Tomasz
Publikováno v:
Frontiers in Earth Science 11, 1190825 (2023)
Lunar sulfides and oxides are a significant source of noble and base metals and will be vital for future human colonies' self-sustainability. Sulfide detection (pyrite and troilite) applies to many technological fields and use cases, for example, as
Externí odkaz:
http://arxiv.org/abs/2402.02614
Autor:
Awasthi, Arun Kumar, Mrozek, Tomasz, Kołomański, Sylwester, Litwicka, Michalina, Stęślicki, Marek, Kułaga, Karol
The disparate nature of thermal-nonthermal energy partition during flares, particularly during weak flares, is still an open issue. Following the Neupert effect, quantifying the relative yield of X-ray emission in different energy bands can enable in
Externí odkaz:
http://arxiv.org/abs/2402.01936
Autor:
Shih, Albert Y., Glesener, Lindsay, Krucker, Säm, Guidoni, Silvina, Christe, Steven, Reeves, Katharine K., Gburek, Szymon, Caspi, Amir, Alaoui, Meriem, Allred, Joel, Battaglia, Marina, Baumgartner, Wayne, Dennis, Brian, Drake, James, Goetz, Keith, Golub, Leon, Hannah, Iain, Hayes, Laura, Holman, Gordon, Inglis, Andrew, Ireland, Jack, Kerr, Graham, Klimchuk, James, McKenzie, David, Moore, Christopher S., Musset, Sophie, Reep, Jeffrey, Ryan, Daniel, Saint-Hilaire, Pascal, Savage, Sabrina, Seaton, Daniel B., Stęślicki, Marek, Woods, Thomas N.
Publikováno v:
Bulletin of the AAS, Vol. 55, Issue 3, Whitepaper #364 (5pp); 2023 July 31
It is essential that there be coordinated and co-optimized observations in X-rays, gamma-rays, and EUV during the peak of solar cycle 26 (~2036) to significantly advance our understanding of impulsive energy release in the corona. The open questions
Externí odkaz:
http://arxiv.org/abs/2306.11777
Autor:
Battaglia, Andrea Francesco, Saqri, Jonas, Massa, Paolo, Perracchione, Emma, Dickson, Ewan C. M., Xiao, Hualin, Veronig, Astrid M., Warmuth, Alexander, Battaglia, Marina, Hurford, Gordon J., Meuris, Aline, Limousin, Olivier, Etesi, László, Maloney, Shane A., Schwartz, Richard A., Kuhar, Matej, Schuller, Frederic, Pavai, Valliappan Senthamizh, Musset, Sophie, Ryan, Daniel F., Kleint, Lucia, Piana, Michele, Massone, Anna Maria, Benvenuto, Federico, Sylwester, Janusz, Litwicka, Michalina, Stęślicki, Marek, Mrozek, Tomasz, Vilmer, Nicole, Fárník, František, Kašparová, Jana, Mann, Gottfried, Gallagher, Peter T., Dennis, Brian R., Csillaghy, André, Benz, Arnold O., Krucker, Säm
Publikováno v:
A&A 656, A4 (2021)
The Spectrometer/Telescope for Imaging X-rays (STIX) is the HXR instrument onboard Solar Orbiter designed to observe solar flares over a broad range of flare sizes, between 4-150 keV. We report the first STIX observations of microflares recorded duri
Externí odkaz:
http://arxiv.org/abs/2106.10058
Autor:
Christe, Steven, Krucker, Samuel, Glesener, Lindsay, Shih, Albert, Saint-Hilaire, Pascal, Caspi, Amir, Allred, Joel, Battaglia, Marina, Chen, Bin, Drake, James, Dennis, Brian, Gary, Dale, Gburek, Szymon, Goetz, Keith, Grefenstette, Brian, Gubarev, Mikhail, Hannah, Iain, Holman, Gordon, Hudson, Hugh, Inglis, Andrew, Ireland, Jack, Ishikawa, Shinosuke, Klimchuk, James, Kontar, Eduard, Kowalski, Adam, Longcope, Dana, Massone, Anna-Maria, Musset, Sophie, Piana, Michele, Ramsey, Brian, Ryan, Daniel, Schwartz, Richard, Stęślicki, Marek, Turin, Paul, Warmuth, Alexander, Wilson-Hodge, Colleen, White, Stephen, Veronig, Astrid, Vilmer, Nicole, Woods, Tom
How impulsive magnetic energy release leads to solar eruptions and how those eruptions are energized and evolve are vital unsolved problems in Heliophysics. The standard model for solar eruptions summarizes our current understanding of these events.
Externí odkaz:
http://arxiv.org/abs/1701.00792
Decades of astrophysical observations have convincingly shown that soft X-ray (SXR; ~0.1--10 keV) emission provides unique diagnostics for the high temperature plasmas observed in solar flares and active regions. SXR observations critical for constra
Externí odkaz:
http://arxiv.org/abs/1701.00619
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Kawka, Adela, Pigulski, Andrzej, O'Toole, Simon, Vennes, Stephane, Nemeth, Peter, Williams, Andrew, Iliev, Lubomir, Kolaczkowski, Zbyszek, Steslicki, Marek
Publikováno v:
ASP Conf. Ser., Vol. 452 (2012), p. 121
We describe our programme to identify and analyse binary stars among the bright subdwarfs selected in the Galaxy Evolution Explorer (GALEX) survey. Radial velocity time-series helped us identify subdwarfs with low-mass or compact stellar companions:
Externí odkaz:
http://arxiv.org/abs/1204.0928