Zobrazeno 1 - 10
of 32
pro vyhledávání: '"Rudawy, Pawel"'
Autor:
Dabrowski, Bartosz, Mikula, Katarzyna, Flisek, Pawel, Vocks, Christian, Zhang, PeiJin, Magdalenić, Jasmina, Warmuth, Alexander, Morosan, Diana E., Froń, Adam, Fallows, Richard A., Bisi, Mario M., Krankowski, Andrzej, Mann, Gottfried, Blaszkiewicz, Leszek, Carley, Eoin P., Gallagher, Peter T., Zucca, Pietro, Rudawy, Pawel, Hajduk, Marcin, Kotulak, Kacper, Sidorowicz, Tomasz
Publikováno v:
A&A 669, A52 (2023)
The Sun is the source of different types of radio bursts that are associated with solar flares, for example. Among the most frequently observed phenomena are type III solar bursts. Their radio images at low frequencies (below 100 MHz) are relatively
Externí odkaz:
http://arxiv.org/abs/2211.12756
Autor:
Heinzel, Petr, Berlicki, Arkadiusz, Bárta, Miroslav, Rudawy, Paweł, Gunár, Stanislav, Labrosse, Nicolas, Radziszewski, Krzysztof
We present first prominence observations obtained with ALMA in Band 3 at the wavelength of 3 mm. High-resolution observations have been coaligned with the MSDP H$\alpha$ data from Wroclaw-Bialk\'{o}w large coronagraph at similar spatial resolution. W
Externí odkaz:
http://arxiv.org/abs/2202.12761
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
We analyze here variations of the position and the vertical extent of the energy deposition layer (EDL) inthe C1.6 GOES-class solar flare observed at 10:20 UT on 2012 September 10. The variations of the EDL arecontrasted with the variations of the sp
Externí odkaz:
http://arxiv.org/abs/2009.06064
Solar flare precursors depict constrained rate of energy release contrasting the imminent rapid energy release which calls for different regime of plasma processes to be at play. Due to subtle emission during the precursor phase, its diagnostics rema
Externí odkaz:
http://arxiv.org/abs/1804.02632
Autor:
Malherbe, Jean-Marie, Mein, Pierre, Sayède, Frédéric, Rudawy, Pawel, Phillips, Kenneth, Keenan, Francis, Rybák, Jan
Publikováno v:
In Advances in Space Research 15 September 2022 70(6):1562-1569
Autor:
Błaszkiewicz, Leszek, Pazderski, Eugeniusz, Wolak, Paweł, Marecki, Andrzej, Rudawy, Paweł, Olech, Mateusz, Flisek, Paweł, Krankowski, Andrzej, Lewandowki, Wojciech
Publikováno v:
In Measurement November 2021 184
Autor:
Soffitta, Paolo, Barcons, Xavier, Bellazzini, Ronaldo, Braga, João, Costa, Enrico, Fraser, George W., Gburek, Szymon, Huovelin, Juhani, Matt, Giorgio, Pearce, Mark, Poutanen, Juri, Reglero, Victor, Santangelo, Andrea, Sunyaev, Rashid A., Tagliaferri, Gianpiero, Weisskopf, Martin, Aloisio, Roberto, Amato, Elena, Attiná, Primo, Axelsson, Magnus, Baldini, Luca, Basso, Stefano, Bianchi, Stefano, Blasi, Pasquale, Bregeon, Johan, Brez, Alessandro, Bucciantini, Niccoló, Burderi, Luciano, Burwitz, Vadim, Casella, Piergiorgio, Churazov, Eugene, Civitani, Marta, Covino, Stefano, da Silva, Rui Miguel Curado, Cusumano, Giancarlo, Dadina, Mauro, D'Amico, Flavio, De Rosa, Alessandra, Di Cosimo, Sergio, Di Persio, Giuseppe, Di Salvo, Tiziana, Dovciak, Michal, Elsner, Ronald, Eyles, Chris J., Fabian, Andrew C., Fabiani, Sergio, Feng, Hua, Giarrusso, Salvatore, Goosmann, René W., Grandi, Paola, Grosso, Nicolas, Israel, Gianluca, Jackson, Miranda, Kaaret, Philip, Karas, Vladimir, Kuss, Michael, Lai, Dong, La Rosa, Giovanni, Larsson, Josefin, Larsson, Stefan, Latronico, Luca, Maggio, Antonio, Maia, Jorge, Marin, Frédéric, Massai, Marco Maria, Mineo, Teresa, Minuti, Massimo, Moretti, Elena, Muleri, Fabio, O'Dell, Stephen L., Pareschi, Giovanni, Peres, Giovanni, Pesce, Melissa, Petrucci, Pierre-Olivier, Pinchera, Michele, Porquet, Delphine, Ramsey, Brian, Rea, Nanda, Reale, Fabio, Rodrigo, Juana Maria, Różańska, Agata, Rubini, Alda, Rudawy, Pawel, Ryde, Felix, Salvati, Marco, Júnior, Valdivino Alexandre de Santiago, Sazonov, Sergey, Sgró, Carmelo, Silver, Eric, Spandre, Gloria, Spiga, Daniele, Stella, Luigi, Tamagawa, Toru, Tamborra, Francesco, Tavecchio, Fabrizio, Dias, Teresa Teixeira, van Adelsberg, Matthew, Wu, Kinwah, Zane, Silvia
Publikováno v:
Experimental Astronomy (Aug. 2013)
X-ray polarimetry, sometimes alone, and sometimes coupled to spectral and temporal variability measurements and to imaging, allows a wealth of physical phenomena in astrophysics to be studied. X-ray polarimetry investigates the acceleration process,
Externí odkaz:
http://arxiv.org/abs/1309.6995
Autor:
Zapiór, Maciej, Rudawy, Paweł
We present an estimation of the lower limits of local magnetic fields in quiescent, activated, and active (surges) promineces, based on reconstructed 3-dimensional (3D) trajectories of individual prominence knots. The 3D trajectories, velocities, tan
Externí odkaz:
http://arxiv.org/abs/1207.2005
Autor:
Zapior, Maciej, Rudawy, Pawel
In this paper we present a new method of restoration of the true thee-dimensional trajectories of the prominence knots based on ground-based observations taken with a single telescope, which is equipped with a Multi-Channel Subtractive Double Pass im
Externí odkaz:
http://arxiv.org/abs/1010.3152