Zobrazeno 1 - 10
of 196
pro vyhledávání: '"Palmaerts, A."'
Autor:
Palmaerts, B., Grodent, D., Bonfond, B., Yao, Z.H., Guo, R.L., Gérard, J.-C., Haewsantati, K., Gladstone, G.R., Greathouse, T.K., Hue, V., Nichols, J.D.
Publikováno v:
In Icarus 15 January 2024 408
Autor:
Yao, Z. H., Bonfond, B., Grodent, D., Chané, E., Dunn, W. R., Kurth, W. S., Connerney, J. E. P., Nichols, J. D., Palmaerts, B., Guo, R. L., Hospodarsky, G. B., Mauk, B. H., Kimura, T., Bolton, S. J.
Although mass and energy in Jupiter's magnetosphere mostly come from the innermost Galilean moon Io's volcanic activities, solar wind perturbations can play crucial roles in releasing the magnetospheric energy and powering aurorae in Jupiter's polar
Externí odkaz:
http://arxiv.org/abs/2004.10140
Autor:
Roussos, Elias, Allanson, Oliver, André, Nicolas, Bertucci, Bruna, Branduardi-Raymont, Graziella, Clark, George, Dialynas, Kostantinos, Dandouras, Iannis, Desai, Ravindra, Futaana, Yoshifumi, Gkioulidou, Matina, Jones, Geraint, Kollmann, Peter, Kotova, Anna, Kronberg, Elena, Krupp, Norbert, Murakami, Go, Nénon, Quentin, Nordheim, Tom, Palmaerts, Benjamin, Plainaki, Christina, Rae, Jonathan, Santos-Costa, Daniel, Sarris, Theodore, Shprits, Yuri, Sulaiman, Ali, Woodfield, Emma, Wu, Xin, Yao, Zhonghua
Jupiter has the most energetic and complex radiation belts in our solar system. Their hazardous environment is the reason why so many spacecraft avoid rather than investigate them, and explains how they have kept many of their secrets so well hidden,
Externí odkaz:
http://arxiv.org/abs/1908.02339
Recently, a transient localized brightness enhancement has been observed in Jupiter's main auroral emission close to noon by Palmaerts et al. (2014). We use results from three-dimensional global MHD simulations to understand what is causing this loca
Externí odkaz:
http://arxiv.org/abs/1804.10564
Autor:
Roussos, E., Kollmann, P., Krupp, N., Kotova, A., Regoli, L., Paranicas, C., Mitchell, D. G., Krimigis, S. M., Hamilton, D., Brandt, P., Carbary, J., Christon, S., Dialynas, K., Dandouras, I., Hill, M. E., Ip, W. H., Jones, G. H., Livi, S., Mauk, B. H., Palmaerts, B., Roelof, E. C., Rymer, A., Sergis, N., Smith, H. T.
Publikováno v:
Science, 2018 Oct 01. 362(6410), 47-47.
Externí odkaz:
https://www.jstor.org/stable/26568277
Autor:
B. Bonfond, Z. H. Yao, G. R. Gladstone, D. Grodent, J.‐C. Gérard, J. Matar, B. Palmaerts, T. K. Greathouse, V. Hue, M. H. Versteeg, J. A. Kammer, R. S. Giles, C. Tao, M. F. Vogt, A. Mura, A. Adriani, B. H. Mauk, W. S. Kurth, S. J. Bolton
Publikováno v:
AGU Advances, Vol 2, Iss 1, Pp n/a-n/a (2021)
Abstract Dawn storms are among the brightest events in the Jovian aurorae. Up to now, they had only been observed from Earth‐based observatories, only showing the Sun‐facing side of the planet. Here, we show for the first time global views of the
Externí odkaz:
https://doaj.org/article/9c6034768a7446e6bf5afb93ec339397
Publikováno v:
In Icarus June 2016 271:1-18
Autor:
Roussos, E., Krupp, N., Mitchell, D.G., Paranicas, C., Krimigis, S.M., Andriopoulou, M., Palmaerts, B., Kurth, W.S., Badman, S.V., Masters, A., Dougherty, M.K.
Publikováno v:
In Icarus 1 January 2016 263:101-116
Autor:
B. Bonfond, J. Gustin, J.-C. Gérard, D. Grodent, A. Radioti, B. Palmaerts, S. V. Badman, K. K. Khurana, C. Tao
Publikováno v:
Annales Geophysicae, Vol 33, Pp 1203-1209 (2015)
The main auroral emission at Jupiter generally appears as a quasi-closed curtain centered around the magnetic pole. This auroral feature, which accounts for approximately half of the total power emitted by the aurorae in the ultraviolet range, is
Externí odkaz:
https://doaj.org/article/baacf8a851fb48958de3c422e12a8155