Zobrazeno 1 - 10
of 1 731
pro vyhledávání: '"JAROLIM P"'
Autor:
Krenn, A. F., Lendl, M., Sulis, S., Deleuil, M., Hofmeister, S. J., Jannsen, N., Fossati, L., De Ridder, J., Seynaeve, D., Jarolim, R., Veronig, A. M.
Context. The PLAnetary Transits and Oscillations of stars (PLATO) mission will observe the same area of the sky continuously for at least two years in an effort to detect transit signals of an Earth-like planet orbiting a solar-like star. Aims. We ai
Externí odkaz:
http://arxiv.org/abs/2410.20077
On 2024 May 10/11, the strongest geomagnetic storm since November 2003 has occurred, with a peak Dst index of -412 nT. The storm was caused by NOAA Active Region (AR) 13664, which was the source of a large number of coronal mass ejections and flares,
Externí odkaz:
http://arxiv.org/abs/2409.08124
Autor:
Purkhart, Stefan, Veronig, Astrid M., Kliem, Bernhard, Jarolim, Robert, Dissauer, Karin, Dickson, Ewan C. M., Podladchikova, Tatiana, Krucker, Säm
We studied the rapid filament evolution in AR 12975 during a confined C2 flare on 28 March 2022, which led to an eruptive M4 flare 1.5 h later. It is characterized by the breakup of the filament, the disappearance of its southern half, and the flow o
Externí odkaz:
http://arxiv.org/abs/2407.07777
Autor:
Diercke, Andrea, Jarolim, Robert, Kuckein, Christoph, Manrique, Sergio J. González, Ziener, Marco, Veronig, Astrid M., Denker, Carsten, Pötzi, Werner, Podladchikova, Tatiana, Pevtsov, Alexei A.
Publikováno v:
A&A 686, A213 (2024)
Filaments are omnipresent features in the solar atmosphere. Their location, properties and time evolution can provide information about changes in solar activity and assist the operational space weather forecast. Therefore, filaments have to be ident
Externí odkaz:
http://arxiv.org/abs/2402.15407
Autor:
Jarolim, Robert, Tremblay, Benoit, Muñoz-Jaramillo, Andrés, Bintsi, Kyriaki-Margarita, Jungbluth, Anna, Santos, Miraflor, Vourlidas, Angelos, Mason, James P., Sundaresan, Sairam, Downs, Cooper, Caplan, Ronald M.
Publikováno v:
ApJL 961 L31 (2024)
To understand its evolution and the effects of its eruptive events, the Sun is permanently monitored by multiple satellite missions. The optically-thin emission of the solar plasma and the limited number of viewpoints make it challenging to reconstru
Externí odkaz:
http://arxiv.org/abs/2401.16388
Autor:
McKevitt, James, Jarolim, Robert, Matthews, Sarah, Baker, Deborah, Temmer, Manuela, Veronig, Astrid, Reid, Hamish, Green, Lucie
The cause of excess spectral line broadening (non-thermal velocity) is not definitively known, but given its rise before and during flaring, the causal processes hold clues to understanding the triggers for the onset of reconnection and the release o
Externí odkaz:
http://arxiv.org/abs/2401.07982
Autor:
Jarolim, Robert, Tremblay, Benoit, Rempel, Matthias, Molnar, Momchil, Veronig, Astrid M., Thalmann, Julia K., Podladchikova, Tatiana
Non-linear force-free extrapolations are a common approach to estimate the 3D topology of coronal magnetic fields based on photospheric vector magnetograms. The force-free assumption is a valid approximation at coronal heights, but for the dense plas
Externí odkaz:
http://arxiv.org/abs/2312.06823
Autor:
Purkhart, Stefan, Veronig, Astrid M., Dickson, Ewan C. M., Battaglia, Andrea Francesco, Krucker, Säm, Jarolim, Robert, Kliem, Bernhard, Dissauer, Karin, Podladchikova, Tatiana
Publikováno v:
A&A 679, A99 (2023)
We present a case study of an M4-class flare on 28 March 2022, near Solar Orbiter's first science perihelion (0.33 AU). Solar Orbiter was 83.5{\deg} west of the Sun-Earth line, making the event appear near the eastern limb, while Earth-orbiting space
Externí odkaz:
http://arxiv.org/abs/2310.02038
Autor:
Jamil Azzi, Qian Yin, Mayuko Uehara, Shunsuke Ohori, Li Tang, Kaimin Cai, Takaharu Ichimura, Martina McGrath, Omar Maarouf, Eirini Kefaloyianni, Scott Loughhead, Jarolim Petr, Qidi Sun, Mincheol Kwon, Stefan Tullius, Ulrich H. von Andrian, Jianjun Cheng, Reza Abdi
Publikováno v:
Cell Reports, Vol 15, Iss 6, Pp 1202-1213 (2016)
Active-targeted delivery to lymph nodes represents a major advance toward more effective treatment of immune-mediated disease. The MECA79 antibody recognizes peripheral node addressin molecules expressed by high endothelial venules of lymph nodes. By
Externí odkaz:
https://doaj.org/article/1c98e1bb63474c90aa0e9a1d403db62a
Autor:
Temmer, M., Scolini, C., Richardson, I. G., Heinemann, S. G., Paouris, E., Vourlidas, A., Bisi, M. M., teams, writing, Al-Haddad, N., Amerstorfer, T., Barnard, L., Buresova, D., Hofmeister, S. J., Iwai, K., Jackson, B. V., Jarolim, R., Jian, L. K., Linker, J. A., Lugaz, N., Manoharan, P. K., Mays, M. L., Mishra, W., Owens, M. J., Palmerio, E., Perri, B., Pomoell, J., Pinto, R. F., Samara, E., Singh, T., Sur, D., Verbeke, C., Veronig, A. M., Zhuang, B.
The ISWAT clusters H1+H2 have a focus on interplanetary space and its characteristics, especially on the large-scale co-rotating and transient structures impacting Earth. SIRs, generated by the interaction between high-speed solar wind originating in
Externí odkaz:
http://arxiv.org/abs/2308.04851