Zobrazeno 1 - 10
of 64
pro vyhledávání: '"Balmaceda, Laura"'
We study the low corona evolution of the `Cartwheel' coronal mass ejection (CME; 2008-04-09) by reconstructing its 3D path and modeling it with magneto-hydrodynamic simulations. This event exhibits a double-deflection that has been reported and analy
Externí odkaz:
http://arxiv.org/abs/2303.15998
Autor:
Verbeke, Christine, Mays, M. Leila, Kay, Christina, Riley, Pete, Palmerio, Erika, Dumbović, Mateja, Mierla, Marilena, Scolini, Camilla, Temmer, Manuela, Paouris, Evangelos, Balmaceda, Laura A., Cremades, Hebe, Hinterreiter, Jürgen
(Shortened version) Current efforts in space weather forecasting of CMEs have been focused on predicting their arrival time and magnetic structure. To make predictions, methods have been developed to derive the true CME speed, size and position, amon
Externí odkaz:
http://arxiv.org/abs/2302.00531
Autor:
Zhang, Ming, Cheng, Lei, Zhang, Ju, Riley, Pete, Kwon, Ryun Young, Lario, David, Balmaceda, Laura, Pogorelov, Nikolai
In an effort to develop computational tools for predicting radiation hazards from solar energetic particles (SEPs), we have created a data-driven physics-based particle transport model to calculate the injection, acceleration and propagation of SEPs
Externí odkaz:
http://arxiv.org/abs/2212.07259
Autor:
Cheng, Lei, Zhang, Ming, Lario, David, Balmaceda, Laura A., Kwon, Ryun Young, Cohen, Christina
This paper presents a stochastic three-dimensional (3D) focused transport simulation of solar energetic particles (SEPs) produced by a data-driven coronal mass ejection (CME) shock propagating through a data-driven model of coronal and heliospheric m
Externí odkaz:
http://arxiv.org/abs/2209.02566
Density Fluctuations in the Solar Wind Based on Type III Radio Bursts Observed by Parker Solar Probe
Autor:
Krupar, Vratislav, Szabo, Adam, Maksimovic, Milan, Kruparova, Oksana, Kontar, Eduard P., Balmaceda, Laura A., Bonnin, Xavier, Bale, Stuart D., Pulupa, Marc, Malaspina, David M., Bonnell, John W., Harvey, Peter R., Goetz, Keith, de Wit, Thierry Dudok, MacDowall, Robert J., Kasper, Justin C., Case, Anthony W., Korreck, Kelly E., Larson, Davin E., Livi, Roberto, Stevens, Michael L., Whittlesey, Phyllis L., Hegedus, Alexander M.
Radio waves are strongly scattered in the solar wind, so that their apparent sources seem to be considerably larger and shifted than the actual ones. Since the scattering depends on the spectrum of density turbulence, better understanding of the radi
Externí odkaz:
http://arxiv.org/abs/2001.03476
Akademický článek
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Autor:
López, Fernando M., Cremades, Hebe, Nuevo, Federico A., Balmaceda, Laura A., Vásquez, Alberto A.
We carry out an analysis of the evacuated mass from three coronal dimming regions observed by the {\it Atmospheric Imaging Assembly} (AIA) on board the {\it Solar Dynamics Observatory}. The three events are unambiguously identified with white-light c
Externí odkaz:
http://arxiv.org/abs/1611.00849
Autor:
Muñoz-Jaramillo, Andrés, Senkpeil, Ryan R., Longcope, Dana W., Tlatov, Andrey G., Pevtsov, Alexei A., Balmaceda, Laura A., DeLuca, Edward E., Martens, Petrus C. H.
Publikováno v:
The Astrophysical Journal, 804:68 (12pp), 2015 May 1
In this work we introduce a new way of binning sunspot group data with the purpose of better understanding the impact of the solar cycle on sunspot properties and how this defined the characteristics of the extended minimum of cycle 23. Our approach
Externí odkaz:
http://arxiv.org/abs/1508.01222
Autor:
Balmaceda, Laura Antonia
Zugl.: Braunschweig, Techn. Univ., Diss., 2007
Externí odkaz:
http://d-nb.info/985229810/04
Autor:
Muñoz-Jaramillo, Andrés, Senkpeil, Ryan R., Windmueller, John C., Amouzou, Ernest C., Longcope, Dana W., Tlatov, Andrey G., Nagovitsyn, Yury A., Pevtsov, Alexei A., Chapman, Gary A., Cookson, Angela M., Yeates, Anthony R., Watson, Fraser T., Balmaceda, Laura A., DeLuca, Edward E., Martens, Petrus C. H.
Publikováno v:
The Astrophysical Journal, Volume 800, Issue 1, Page 48, (2015)
In this work we take advantage of eleven different sunspot group, sunspot, and active region databases to characterize the area and flux distributions of photospheric magnetic structures. We find that, when taken separately, different databases are b
Externí odkaz:
http://arxiv.org/abs/1410.6281