Bibliografías temáticas / Lunar wake plasma

Literatura académica sobre el tema "Lunar wake plasma"

Autor: Grafiati
Publicado: 6 de septiembre de 2023

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Artículos de revistas sobre el tema "Lunar wake plasma"

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Yan, Bo, Punam K. Prasad, Sayan Mukherjee, Asit Saha y Santo Banerjee. "Dynamical Complexity and Multistability in a Novel Lunar Wake Plasma System". Complexity 2020 (16 de marzo de 2020): 1–11. http://dx.doi.org/10.1155/2020/5428548.

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Dynamical complexity and multistability of electrostatic waves are investigated in a four-component homogeneous and magnetized lunar wake plasma constituting of beam electrons, heavier ions (alpha particles, He++), protons, and suprathermal electrons. The unperturbed dynamical system of the considered lunar wake plasma supports nonlinear and supernonlinear trajectories which correspond to nonlinear and supernonlinear electrostatic waves. On the contrary, the perturbed dynamical system of lunar wake plasma shows different types of coexisting attractors including periodic, quasiperiodic, and chaotic, investigated by phase plots and Lyapunov exponents. To confirm chaotic and nonchaotic dynamics in the perturbed lunar wake plasma, 0−1 chaos test is performed. Furthermore, a weighted recurrence-based entropy is implemented to investigate the dynamical complexity of the system. Numerical results show existence of chaos with variation of complexity in the perturbed dynamics.
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Rasca, Anthony P., Shahab Fatemi y William M. Farrell. "Modeling the Lunar Wake Response to a CME Using a Hybrid PIC Model". Planetary Science Journal 3, n.º 1 (1 de enero de 2022): 4. http://dx.doi.org/10.3847/psj/ac3fba.

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Abstract In the solar wind, a low-density wake region forms downstream of the nightside lunar surface. In this study, we use a series of 3D hybrid particle-in-cell simulations to model the response of the lunar wake to a passing coronal mass ejection (CME). Average plasma parameters are derived from the Wind spacecraft located at 1 au during three distinct phases of a passing halo (Earth-directed) CME on 2015 June 22. Each set of plasma parameters, representing the shock/plasma sheath, a magnetic cloud, and plasma conditions we call the mid-CME phase, are used as the time-static upstream boundary conditions for three separate simulations. These simulation results are then compared with results that use nominal solar wind conditions. Results show a shortened plasma void compared to nominal conditions and a distinctive rarefaction cone originating from the terminator during the CME’s plasma sheath phase, while a highly elongated plasma void reforms during the magnetic cloud and mid-CME phases. Developments of electric and magnetic field intensification are also observed during the plasma sheath phase along the central wake, while electrostatic turbulence dominates along the plasma void boundaries and 2–3 lunar radii R M downstream in the central wake during the magnetic cloud and mid-CME phases. The simulations demonstrate that the lunar wake responds in a dynamic way with the changes in the upstream solar wind during a CME.
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Sreeraj, T., S. V. Singh y G. S. Lakhina. "Electrostatic waves driven by electron beam in lunar wake plasma". Physics of Plasmas 25, n.º 5 (mayo de 2018): 052902. http://dx.doi.org/10.1063/1.5032141.

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Sreeraj, T., S. V. Singh y G. S. Lakhina. "Linear analysis of electrostatic waves in the lunar wake plasma". Physica Scripta 95, n.º 4 (19 de febrero de 2020): 045610. http://dx.doi.org/10.1088/1402-4896/ab7142.

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Xu, Xiaojun, Qi Xu, Qing Chang, Jiaying Xu, Jing Wang, Yi Wang, Pingbing Zuo y Vassilis Angelopoulos. "ARTEMIS Observations of Well-structured Lunar Wake in Subsonic Plasma Flow". Astrophysical Journal 881, n.º 1 (14 de agosto de 2019): 76. http://dx.doi.org/10.3847/1538-4357/ab2e0a.

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Guo, Dawei, Xiaoping Zhang, Lianghai Xie, Xiaojun Xu, Aoao Xu, Qi Yan, Yi Xu y Fan Yang. "Diamagnetic Plasma Clouds in the Near Lunar Wake Observed by ARTEMIS". Astrophysical Journal 883, n.º 1 (17 de septiembre de 2019): 12. http://dx.doi.org/10.3847/1538-4357/ab3652.

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Halekas, J. S., S. D. Bale, D. L. Mitchell y R. P. Lin. "Correction to “Electrons and magnetic fields in the lunar plasma wake”". Journal of Geophysical Research: Space Physics 116, A7 (julio de 2011): n/a. http://dx.doi.org/10.1029/2011ja016929.

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Xu, Xiaojun, Jiaying Xu, Qi Xu, Qing Chang y Jing Wang. "Rapid Refilling of the Lunar Wake under Transonic Plasma Flow: ARTEMIS Observations". Astrophysical Journal 908, n.º 2 (1 de febrero de 2021): 227. http://dx.doi.org/10.3847/1538-4357/abd6f1.

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Halekas, J. S., V. Angelopoulos, D. G. Sibeck, K. K. Khurana, C. T. Russell, G. T. Delory, W. M. Farrell et al. "First Results from ARTEMIS, a New Two-Spacecraft Lunar Mission: Counter-Streaming Plasma Populations in the Lunar Wake". Space Science Reviews 165, n.º 1-4 (20 de enero de 2011): 93–107. http://dx.doi.org/10.1007/s11214-010-9738-8.

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Yu, William, Joseph Wang y Kevin Chou. "Laboratory Measurement of Lunar Regolith Simulant Surface Charging in a Localized Plasma Wake". IEEE Transactions on Plasma Science 43, n.º 12 (diciembre de 2015): 4175–81. http://dx.doi.org/10.1109/tps.2015.2492551.

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Tesis sobre el tema "Lunar wake plasma"

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Fatemi, Shahab. "Modeling the Lunar plasma wake". Licentiate thesis, Luleå tekniska universitet, Rymdteknik, 2011. http://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-17543.

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This thesis discusses the solar wind interaction with the Moon and the formation of the lunar plasma wake from a kinetic perspective. The Moon is essentially a non-conducting body which has a tenuous atmosphere and no global magnetic fields. The solar wind plasma impacts directly the lunar day-side and is absorbed by the lunar surface. This creates a plasma void and forms a wake at the night side of the Moon.We study the properties and structure of the lunar wake for typical solar wind conditions using a three-dimensional hybrid plasma solver. Also, we study the solar wind proton velocity space distribution functions at close distances to the Moon in the lunar wake and investigate the effects of lunar surface plasma absorption and non-isothermal solar wind velocity space distribution functions on the solar wind protons there.Finally, we compare the simulation results with the observations and show that a hybrid model of plasma can explain the kinetic aspects of the lunar wake and we investigate the effects of the lunar surface plasma absorption and non-isothermal solar wind velocity distribution on the solar wind proton properties there.

Godkänd; 2011; 20111114 (shafat); LICENTIATSEMINARIUM Ämnesområde: Rymdteknik/Space Engineering Examinator: Docent Mats Holmström, IRF Kiruna Diskutant: Senior Scientist Bengt Eliasson, Institute for Theoretical Physics, Ruhr-University, Germany Tid: Måndag den 19 december 2011 kl 10.00 Plats: Sal C, Rymdcampus i Kiruna, Luleå tekniska universitet

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Libros sobre el tema "Lunar wake plasma"

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Long-Range Transhorizon Lunar Surface Radio Wave Propagation in the Presence of a Regolith and a Sparse Exospheric Plasma. Independently Published, 2020.

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Capítulos de libros sobre el tema "Lunar wake plasma"

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Halekas, J. S., V. Angelopoulos, D. G. Sibeck, K. K. Khurana, C. T. Russell, G. T. Delory, W. M. Farrell et al. "First Results from ARTEMIS, a New Two-Spacecraft Lunar Mission: Counter-Streaming Plasma Populations in the Lunar Wake". En The ARTEMIS Mission, 93–107. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4614-9554-3_5.

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Actas de conferencias sobre el tema "Lunar wake plasma"

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Nishino, Masaki N., Yoshifumi Saito, Yoshiya Kasahara, Yoshiharu Omura, Kozo Hashimoto, Takayuki Ono, Hideo Tsunakawa, Futoshi Takahashi, Shoichiro Yokota y Masaki Fujimoto. "Plasma and wave observations in the deep lunar wake". En 2014 XXXIth URSI General Assembly and Scientific Symposium (URSI GASS). IEEE, 2014. http://dx.doi.org/10.1109/ursigass.2014.6929934.

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Popel, Sergey I., Sergey I. Kopnin y A. Yu Dubinskii. "Dusty Plasmas over Hydrogen-Rich Areas of Lunar Surface". En 2019 Russian Open Conference on Radio Wave Propagation (RWP). IEEE, 2019. http://dx.doi.org/10.1109/rwp.2019.8810249.

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Kassem, Attia Ibrahem, Sergey Popel, Yulya Izvekova y Lev Zelenyi. "LOWER-HYBRID WAVES IN THE EXOSPHERE OF THE MOON". En ФУНДАМЕНТАЛЬНЫЕ И ПРИКЛАДНЫЕ КОСМИЧЕСКИЕ ИССЛЕДОВАНИЯ. ИКИ РАН, 2020. http://dx.doi.org/10.21046/kmu-2020-49-60.

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A description is given of the wave processes in the interaction of the tail of the Earth's magnetosphere with the dusty exosphere of the Moon. The significance of the lower-hybrid waves appears in this case. It is found that the development of linear hydrodynamic instability leads to the excitation of the lower-hybrid waves. Furthermore, the development of the instability is due to the relative motion of magnetosphere ions and charged dust particles. The processes of development of lower-hybrid turbulence, which is considered from the standpoint of strong turbulence, are investigated. Based on wave-ion interaction, the effective collision frequency which characterizes the anomalous loss of ion momentum is determined. Moreover, the electric fields which arise in the region of interaction of the dusty plasma near the Moon and the Earth's magnetosphere are evaluated. The excitation of the electric fields produced due to the development of lower-hybrid turbulence is thought to play a significant role from the viewpoint of the electric field pattern at the Moon. The effects of lower-hybrid turbulence in the near-surface lunar dusty plasma should be taken into account when interpreting the observational data.
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