Zobrazeno 1 - 10
of 401
pro vyhledávání: '"Liu, Terry"'
Autor:
Raptis, Savvas, Lindberg, Martin, Liu, Terry Z., Turner, Drew L., Lalti, Ahmad, Zhou, Yufei, Kajdič, Primož, Kouloumvakos, Athanasios, Sibeck, David G., Vuorinen, Laura, Michael, Adam, Shumko, Mykhaylo, Osmane, Adnane, Krämer, Eva, Turc, Lucile, Karlsson, Tomas, Katsavrias, Christos, Wilson III, Lynn B., Madanian, Hadi, Blanco-Cano, Xóchitl, Cohen, Ian J., Escoubet, C. Philippe
Shock-generated transients, such as hot flow anomalies (HFAs), upstream of planetary bow shocks, play a critical role in electron acceleration. Using multi-mission data from NASA's Magnetospheric Multiscale (MMS) and ESA's Cluster missions, we demons
Externí odkaz:
http://arxiv.org/abs/2411.12815
Autor:
Kajdič, Primož, Blanco-Cano, Xóchitl, Turc, Lucile, Archer, Martin, Raptis, Savvas, Liu, Terry Z., Pfau-Kempf, Yann, LaMoury, Adrian T., Hao, Yufei, Escoubet, Philippe C., Omidi, Nojan, Sibeck, David G., Wang, Boyi, Zhang, Hui, Lin, Yu
Publikováno v:
Front. Astron. Space Sci., (2024), Sec. Space Physics, Volume 11 - 2024
In recent years, it has become increasingly clear that space weather disturbances can be triggered by transient upstream mesoscale structures (TUMS), independently of the occurrence of large-scale solar wind (SW) structures, such as interplanetary co
Externí odkaz:
http://arxiv.org/abs/2411.07145
Interaction of the Prominence Plasma within the Magnetic Cloud of an ICME with the Earth's Bow Shock
Autor:
Madanian, Hadi, Chen, Li-Jen, Ng, Jonathan, Starkey, Michael J., Fuselier, Stephen A., Bessho, Naoki, Gershman, Daniel J., Liu, Terry Z.
The magnetic cloud within an interplanetary coronal mass ejection (ICME) is characterized by high magnetic field intensities. In this study, we investigate the interaction of a magnetic cloud carrying a density structure with the Earth's bow shock du
Externí odkaz:
http://arxiv.org/abs/2410.15989
Autor:
An, Xin, Artemyev, Anton, Angelopoulos, Vassilis, Liu, Terry Z., Vasko, Ivan, Malaspina, David
Publikováno v:
Physical Review Letters 133, 225201 (2024)
In space plasmas, large-amplitude Alfv\'en waves can drive compressive perturbations, accelerate ion beams, and lead to plasma heating and the excitation of ion acoustic waves at kinetic scales. This energy channelling from fluid to kinetic scales re
Externí odkaz:
http://arxiv.org/abs/2406.14782
The ion foreshock is highly dynamic, disturbing the bow shock and the magnetosphere-ionosphere system. To forecast foreshock-driven space weather effects, it is necessary to model foreshock ions as a function of upstream shock parameters. Case studie
Externí odkaz:
http://arxiv.org/abs/2402.01978
Plasma turbulence is a ubiquitous dynamical process that transfers energy across many spatial and temporal scales and affects energetic particle transport. Recent advances in the understanding of compressible magnetohydrodynamic (MHD) turbulence demo
Externí odkaz:
http://arxiv.org/abs/2305.12507
Plasma turbulence is a ubiquitous dynamical process that transfers energy across many spatial and temporal scales in astrophysical and space plasma systems. Although the theory of anisotropic magnetohydrodynamic (MHD) turbulence has successfully desc
Externí odkaz:
http://arxiv.org/abs/2301.06709
Autor:
Shi, Xiaofei, Liu, Terry, Artemyev, Anton, Angelopoulos, Vassilis, Zhang, Xiao-Jia, Turner, Drew L.
Thermalization and heating of plasma flows at shocks result in unstable charged-particle distributions which generate a wide range of electromagnetic waves. These waves, in turn, can further accelerate and scatter energetic particles. Thus, the prope
Externí odkaz:
http://arxiv.org/abs/2211.05398
We present three-dimensional magnetic power spectra in wavevector space to investigate anisotropy and scalings of sub-Alfv\'enic solar wind turbulence at magnetohydrodynamic (MHD) scale using the Magnetospheric Multiscale spacecraft. The magnetic pow
Externí odkaz:
http://arxiv.org/abs/2204.05410
Autor:
Zhao, S. Q., Zhang, H., Liu, Terry Z., Yan, Huirong, Xiao, C. J., Liu, Mingzhe, Zong, Q. -G., Wang, Xiaogang, Shi, Mijie, Teng, Shangchun, Wang, Huizi, Rankin, R., Pollock, C., Le, G.
Solar wind parameters play a dominant role in reconnection rate, which controls the solar wind-magnetosphere coupling efficiency at Earth's magnetopause. Besides, low-energy ions from the ionosphere, frequently detected on the magnetospheric side of
Externí odkaz:
http://arxiv.org/abs/2109.10943