Zobrazeno 1 - 10
of 219
pro vyhledávání: '"Valentin Martínez"'
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
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:
Mª del Prado Sánchez Ayllón
Publikováno v:
Revista Complutense de Educación, Vol 11, Iss 2 (2000)
Sin resumen
Externí odkaz:
https://doaj.org/article/aaf0ab9c889d442c96b3a3082770eea7
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
We describe how the accurate characterization of exoplanetary atmospheres in the ELT and JWST era will inevitably require taking into consideration the stellar inhomogeneities caused by convection and magnetic fields. The existing evidence that demon
Externí odkaz:
http://arxiv.org/abs/1904.05976
Autor:
Pillet, Valentin Martinez, Hill, Frank, Hammel, Heidi, de Wijn, Alfred G., Gosain, Sanjay, Burkepile, Joan, Henney, Carl J., McAteer, James R. T., Bain, Hazel M., Manchester IV, Ward B., Lin, Haosheng, Roth, Markus, Ichimoto, Kiyoshi, Suematsu, Yoshinori
Ground-based solar observations provide key contextual data (i.e., the 'big picture') to produce a complete description of the only astrosphere we can study in situ: our Sun's heliosphere. The next decade will see the beginning of operations of the D
Externí odkaz:
http://arxiv.org/abs/1903.06944