Zobrazeno 1 - 10
of 109
pro vyhledávání: '"Valentin Martínez"'
Publikováno v:
Holos, Vol 7, Iss 0, Pp 1-7 (2020)
En este artículo sobre Gaspar Melchor de Jovellanos (1744-1811) se recuerdan algunas de las contribuciones educativas del egregio ilustrado, un modernizador. En el texto se destaca sobre todo su condición de pedagogo, su preocupación por la instru
Externí odkaz:
https://doaj.org/article/3d1042c764ea48b3b9bbbe0bc21fd812
Autor:
Dennis Tilipman, Maria Kazachenko, Benoit Tremblay, Ivan Milić, Valentin Martínez Pillet, Matthias Rempel
Publikováno v:
The Astrophysical Journal, Vol 956, Iss 2, p 83 (2023)
Poynting flux is the flux of magnetic energy, which is responsible for chromospheric and coronal heating in the solar atmosphere. It is defined as a cross product of the electric and magnetic fields, and in ideal MHD conditions it can be expressed in
Externí odkaz:
https://doaj.org/article/5daf4d7150e1435d96db9d2244924099
Autor:
Tilipman, Dennis, Kazachenko, Maria, Tremblay, Benoit, Milic, Ivan, Pillet, Valentin Martinez, Rempel, Matthias
Poynting flux is the flux of magnetic energy, which is responsible for chromospheric and coronal heating in the solar atmosphere. It is defined as a cross product of electric and magnetic fields, and in ideal MHD conditions it can be expressed in ter
Externí odkaz:
http://arxiv.org/abs/2307.02445
Autor:
Roy, Anirban, Valentín-Martínez, Dariannette, Wang, Kailai, Battaglia, Nicholas, van Engelen, Alexander
Mapping of multiple lines such as the fine-structure emission from [CII] (157.7 $\mu \text{m}$), [OIII] (52 \& 88.4 $\mu \text{m}$), and rotational emission lines from CO are of particular interest for upcoming line intensity mapping (LIM) experiment
Externí odkaz:
http://arxiv.org/abs/2304.06748
Publikováno v:
INFAD, Vol 1, Iss 1, Pp 295-306 (2014)
The interest for child stress has increased during recent years. Previously it was thought that childhood was certainly a “happy period” and consequently it was ignored the possibility that children could suffer this psychological condition. Even
Externí odkaz:
https://doaj.org/article/71466ea66ebc42658ae45d69fd0cd08c
Autor:
Wang, Shuo, Jenkins, Jack M., Muglach, Karin, Pillet, Valentin Martinez, Beck, Christian, Long, David M., Choudhary, Debi Prasad, McAteer, James
Solar filaments exist as stable structures for extended periods of time before many of them form the core of a CME. We examine the properties of an erupting filament on 2017 May 29--30 with high-resolution He I 10830 A and Halpha spectra from the Dun
Externí odkaz:
http://arxiv.org/abs/2111.07830
Autor:
Criscuoli, Serena, Kazachenko, Maria, Kitashvili, Irina, Kosovichev, Alexander, Pillet, Valentín Martínez, Nita, Gelu, Sadykov, Viacheslav, Wray, Alan
The next decade will be an exciting period for solar astrophysics, as new ground- and space-based instrumentation will provide unprecedented observations of the solar atmosphere and heliosphere. The synergy between modeling effort and comprehensive a
Externí odkaz:
http://arxiv.org/abs/2101.00011
Autor:
Rast, Mark P., González, Nazaret Bello, Rubio, Luis Bellot, Cao, Wenda, Cauzzi, Gianna, DeLuca, Edward, De Pontieu, Bart, Fletcher, Lyndsay, Gibson, Sarah E., Judge, Philip G., Katsukawa, Yukio, Kazachenko, Maria D., Khomenko, Elena, Landi, Enrico, Pillet, Valentin Martínez, Petrie, Gordon J. D., Qiu, Jiong, Rachmeler, Laurel A., Rempel, Matthias, Schmidt, Wolfgang, Scullion, Eamon, Sun, Xudong, Welsch, Brian T., Andretta, Vincenzo, Antolin, Patrick, Ayres, Thomas R., Balasubramaniam, K. S., Ballai, Istvan, Berger, Thomas E., Bradshaw, Stephen J., Carlsson, Mats, Casini, Roberto, Centeno, Rebecca, Cranmer, Steven R., DeForest, Craig, Deng, Yuanyong, Erdélyi, Robertus, Fedun, Viktor, Fischer, Catherine E., Manrique, Sergio J. González, Hahn, Michael, Harra, Louise, Henriques, Vasco M. J., Hurlburt, Neal E., Jaeggli, Sarah, Jafarzadeh, Shahin, Jain, Rekha, Jefferies, Stuart M., Keys, Peter H., Kowalski, Adam F., Kuckein, Christoph, Kuhn, Jeffrey R., Liu, Jiajia, Liu, Wei, Longcope, Dana, McAteer, R. T. James, McIntosh, Scott W., McKenzie, David E., Miralles, Mari Paz, Morton, Richard J., Muglach, Karin, Nelson, Chris J., Panesar, Navdeep K., Parenti, Susanna, Parnell, Clare E., Poduval, Bala, Reardon, Kevin P., Reep, Jeffrey W., Schad, Thomas A., Schmit, Donald, Sharma, Rahul, Socas-Navarro, Hector, Srivastava, Abhishek K., Sterling, Alphonse C., Suematsu, Yoshinori, Tarr, Lucas A., Tiwari, Sanjiv, Tritschler, Alexandra, Verth, Gary, Vourlidas, Angelos, Wang, Haimin, Wang, Yi-Ming, NSO, project, DKIST, scientists, DKIST instrument, Group, the DKIST Science Working, Community, the DKIST Critical Science Plan
The Daniel K. Inouye Solar Telescope (DKIST) will revolutionize our ability to measure, understand and model the basic physical processes that control the structure and dynamics of the Sun and its atmosphere. The first-light DKIST images, released pu
Externí odkaz:
http://arxiv.org/abs/2008.08203
Autor:
Zeuner, Franziska, Sainz, Rafael Manso, Feller, Alex, van Noort, Michiel, Solanki, Sami K., Iglesias, Francisco A., Reardon, Kevin, Pillet, Valentín Martínez
Publikováno v:
The Astrophysical Journal Letters 893:L44 (2020)
Magnetic fields in turbulent, convective high-$\beta$ plasma naturally develop highly tangled and complex topologies---the solar photosphere being the paradigmatic example. These fields are mostly undetectable by standard diagnostic techniques with f
Externí odkaz:
http://arxiv.org/abs/2004.03679
Autor:
Wang, Shuo, Jenkins, Jack M., Pillet, Valentin Martinez, Beck, Christian, Long, David M., Choudhary, Debi Prasad, Muglach, Karin, McAteer, James
Publikováno v:
ApJ, 2020, 892, 75
The full 3-D vector magnetic field of a solar filament prior to eruption is presented. The filament was observed with the Facility Infrared Spectropolarimeter at the Dunn Solar Telescope in the chromospheric He i line at 10830 {\AA} on May 29 and 30,
Externí odkaz:
http://arxiv.org/abs/2002.02104