Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Emily I Mason"'
Publikováno v:
The Astrophysical Journal, Vol 943, Iss 2, p 84 (2023)
We present numerical models from the field-aligned HYDrodynamics and RADiation code (HYDRAD) of a highly asymmetric closed coronal loop with near-singular expansion factor. This loop was chosen to simulate a coronal magnetic flux tube that passes clo
Externí odkaz:
https://doaj.org/article/13d00d2861a44245b535dcb1512e9224
Autor:
Yeimy. J. Rivera, Aleida Higginson, Susan T. Lepri, Nicholeen M. Viall, B. L. Alterman, Enrico Landi, Sarah A. Spitzer, Jim M. Raines, Steven R. Cranmer, John M. Laming, Emily I. Mason, Samantha Wallace, John C. Raymond, Benjamin J. Lynch, Chris R. Gilly, Thomas Y. Chen, Ryan M. Dewey
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
This paper outlines key scientific topics that are important for the development of solar system physics and how observations of heavy ion composition can address them. The key objectives include, 1) understanding the Sun’s chemical composition by
Externí odkaz:
https://doaj.org/article/eb65fa1f577943f594d20304a914abb1
Autor:
Vincent E. Ledvina, Erika Palmerio, Ryan M. McGranaghan, Alexa J. Halford, Aidan Thayer, Laura Brandt, Elizabeth A. MacDonald, Ankush Bhaskar, Chuanfei Dong, Ilkay Altintas, James Colliander, Meng Jin, Richa N. Jain, Subhamoy Chatterjee, Zubair Shaikh, Nathaniel A. Frissell, Thomas Y. Chen, Ryan J. French, Brianna Isola, Scott W. McIntosh, Emily I. Mason, Pete Riley, Tim Young, Wayne Barkhouse, Maria D. Kazachenko, Martin Snow, Dogacan S. Ozturk, Seth G. Claudepierre, Francesca Di Mare, Andy Witteman, Jeremy Kuzub
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
Space weather refers to conditions around a star, like our Sun, and its interplanetary space that may affect space- and ground-based assets as well as human life. Space weather can manifest as many different phenomena, often simultaneously, and can c
Externí odkaz:
https://doaj.org/article/e189aca5d33240758f379cd8694dd8ce
The physical mechanisms by which solar prominences (or filaments) form are still not well understood. The presently favored scenario invokes the evaporation of chromospheric plasma via localized heating at the footprints of a magnetic flux rope (MFR)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::83acc09d03941001a0ea9e89b8f0d293
https://doi.org/10.5194/egusphere-egu23-2300
https://doi.org/10.5194/egusphere-egu23-2300
We present numerical models from the field-aligned Hydrodynamics and Radiation Code (HYDRAD) of a highly asymmetric closed coronal loop with near-singular expansion factor. This loop was chosen to simulate a coronal magnetic flux tube that passes clo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::da1c68ef559dfe3e15f65d7f16c4b973
http://arxiv.org/abs/2212.08529
http://arxiv.org/abs/2212.08529
Autor:
Emily I. Mason, Vadim M. Uritsky
Much of coronal hole (CH) research is focused upon determining the boundary and calculating the open flux as accurately as possible. However, the observed boundary itself is worthy of investigation, and holds important clues to the physics transpirin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::424ed71098908b6da95bf32b751e5959
http://arxiv.org/abs/2209.02833
http://arxiv.org/abs/2209.02833
Autor:
Emily I. Mason, Roberto Lionello, Cooper Downs, Jon A. Linker, Ronald M. Caplan, Marc L. DeRosa
Publikováno v:
The Astrophysical Journal Letters, Vol 959, Iss 1, p L4 (2023)
We present in this Letter the first global comparison between traditional line-tied steady-state magnetohydrodynamic models and a new, fully time-dependent thermodynamic magnetohydrodynamic simulation of the global corona. To approximate surface magn
Externí odkaz:
https://doaj.org/article/7ad7f2295dd1485ea38ae051b4692f97
Publikováno v:
The Astrophysical Journal, Vol 958, Iss 1, p 43 (2023)
One systematic limitation of solar coronal hole (CH) detection at extreme ultraviolet (EUV) wavelengths is the obscuration of dark regions of the corona by brighter structures along the line of sight. Another problem arises when using CHs to compute
Externí odkaz:
https://doaj.org/article/606c46a4abee460e8dcaaa1131d7148c
Autor:
Roberto Lionello, Cooper Downs, Emily I. Mason, Jon A. Linker, Ronald M. Caplan, Pete Riley, Viacheslav S. Titov, Marc L. DeRosa
Publikováno v:
The Astrophysical Journal, Vol 959, Iss 2, p 77 (2023)
We describe, test, and apply a technique to incorporate full-Sun, surface flux evolution into an MHD model of the global solar corona. Requiring only maps of the evolving surface flux, our method is similar to that of Lionello et al., but we introduc
Externí odkaz:
https://doaj.org/article/7434e047920a4e618ea1086c6743f0af