Zobrazeno 1 - 10
of 66
pro vyhledávání: '"Simoes, Paulo J. A."'
Autor:
Simões, Paulo J. A., Fletcher, Lyndsay, Hudson, Hugh S., Kerr, Graham S., Penn, Matt, Lopez, Karla F.
Solar flares are powerful particle accelerators, and in the accepted standard flare model most of the flare energy is transported from a coronal energy-release region by accelerated electrons which stop collisionally in the chromosphere, heating and
Externí odkaz:
http://arxiv.org/abs/2406.11361
Autor:
Wedemeyer, Sven, Barta, Miroslav, Brajsa, Roman, Chai, Yi, Costa, Joaquim, Gary, Dale, de Castro, Guillermo Gimenez, Gunar, Stanislav, Fleishman, Gregory, Hales, Antonio, Hudson, Hugh, Kirkaune, Mats, Mohan, Atul, Motorina, Galina, Pellizzoni, Alberto, Saberi, Maryam, Selhorst, Caius L., Simoes, Paulo J. A., Shimojo, Masumi, Skokic, Ivica, Sudar, Davor, Menezes, Fabian, White, Stephen, Booth, Mark, Klaassen, Pamela, Cicone, Claudia, Mroczkowski, Tony, Cordiner, Martin A., Di Mascolo, Luca, Johnstone, Doug, van Kampen, Eelco, Lee, Minju, Liu, Daizhong, Maccarone, Thomas, Orlowski-Scherer, John, Saintonge, Amelie, Smith, Matthew, Thelen, Alexander E.
Observations at (sub-)millimeter wavelengths offer a complementary perspective on our Sun and other stars, offering significant insights into both the thermal and magnetic composition of their chromospheres. Despite the fundamental progress in (sub-)
Externí odkaz:
http://arxiv.org/abs/2403.00920
Autor:
da Silva, Douglas Félix, Hui, Li, Simões, Paulo J. A., Valio, Adriana, R., Joaquim C. E., Hudson, Hugh S., Simoes, Paulo J. A., Fletcher, Lyndsay, Hayes, Laura A., Hannah, Iain G.
Understanding the physical processes that trigger solar flares is paramount to help with forecasting space weather and mitigating the effects on our technological infrastructure. A previously unknown phenomenon was recently identified in solar flares
Externí odkaz:
http://arxiv.org/abs/2308.11017
Autor:
de Castro, C. Guillermo Giménez, Raulin, Jean-Pierre, Valio, Adriana, Correia, Emilia, Simoes, Paulo J. A., Szpigel, Sergio
The Solar Submillimeter Telescope (SST) is an unique instrument that has been observing the Sun daily since 2001 bringing a wealth of information and raising new questions about the particle acceleration and transport, and emission mechanisms during
Externí odkaz:
http://arxiv.org/abs/2307.06977
Autor:
Glesener, Lindsay, Shih, Albert Y., Caspi, Amir, Milligan, Ryan, Hudson, Hugh, Oka, Mitsuo, Buitrago-Casas, Juan Camilo, Guo, Fan, Ryan, Dan, Kontar, Eduard, Veronig, Astrid, Hayes, Laura A., Inglis, Andrew, Golub, Leon, Vilmer, Nicole, Gary, Dale, Reid, Hamish, Hannah, Iain, Kerr, Graham S., Reeves, Katharine K., Allred, Joel, Guidoni, Silvina, Yu, Sijie, Christe, Steven, Musset, Sophie, Dennis, Brian, Oliveros, Juan Carlos Martínez, Athiray, P. S., Vievering, Juliana, White, Stephen, Winebarger, Amy, Drake, James, Jeffrey, Natasha, Antiochos, Spiro, Duncan, Jessie, Zhang, Yixian, Alaoui, Meriem, Simões, Paulo J. A., Battaglia, Marina, Setterberg, William, Masek, Reed, Chen, Thomas Y., Peterson, Marianne, Krucker, Säm, Temmer, Manuela, Saint-Hilaire, Pascal, Petrosian, Vahe, Knuth, Trevor, Moore, Christopher S.
Publikováno v:
Bulletin of the AAS, Vol. 55, Issue 3, Whitepaper #129 (14pp); 2023 July 31
Understanding the nature of energetic particles in the solar atmosphere is one of the most important outstanding problems in heliophysics. Flare-accelerated particles compose a huge fraction of the flare energy budget; they have large influences on h
Externí odkaz:
http://arxiv.org/abs/2306.05447
Autor:
Carlsson, Mats, Fletcher, Lyndsay, Allred, Joel, Heinzel, Petr, Kasparova, Jana, Kowalski, Adam, Mathioudakis, Mihalis, Reid, Aaron, Simoes, Paulo J. A.
Publikováno v:
A&A 673, A150 (2023)
Context: Solar flares are the result of the sudden release of magnetic energy in the corona. Much of this energy goes into accelerating charged particles to high velocity. These particles travel along the magnetic field and the energy is dissipated w
Externí odkaz:
http://arxiv.org/abs/2304.02618
Autor:
McLaughlin, Shaun A., Milligan, Ryan O., Kerr, Graham S., Monson, Aaron J., Simões, Paulo J. A., Mathioudakis, Mihalis
The Lyman Continuum (LyC; $<911.12$\AA) forms at the top of the chromosphere in the quiet-Sun, making LyC a powerful tool for probing the chromospheric plasma during solar flares. To understand the effects of non-thermal energy deposition in the chro
Externí odkaz:
http://arxiv.org/abs/2301.01648
Autor:
Silva, Alexandre José de Oliveira e, Selhorst, Caius L., Costa, Joaquim E. R., Simões, Paulo J. A., de Castro, C. Guillermo Giménez, Wedemeyer, Sven, White, Stephen M., Brajša, Roman, Valio, Adriana
In recent decades our understanding of solar active regions (ARs) has improved substantially due to observations made with better angular resolution and wider spectral coverage. While prior AR observations have shown that these structures were always
Externí odkaz:
http://arxiv.org/abs/2205.03385
Autor:
Labrosse, Nicolas, Rodger, Andrew S., Radziszewski, Krzysztof, Rudawy, Paweł, Antolin, Patrick, Fletcher, Lyndsay, Levens, Peter J., Peat, Aaron W., Schmieder, Brigitte, Simões, Paulo J. A.
We present the first observation of a solar prominence at $84-116$ GHz using the high resolution interferometric imaging of ALMA. Simultaneous observations in H$\alpha$ from Bia{\l}kaw Observatory and with SDO/AIA reveal similar prominence morphology
Externí odkaz:
http://arxiv.org/abs/2202.12434
Publikováno v:
In Advances in Space Research 15 October 2024 74(8):4210-4222