Bibliographies thématiques / Lunar wake

Littérature scientifique sur le sujet « Lunar wake »

Auteur : Grafiati
Publié le 6 septembre 2023

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Articles de revues sur le sujet "Lunar wake"

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Fatemi, S., M. Holmström, Y. Futaana, S. Barabash et C. Lue. « The lunar wake current systems ». Geophysical Research Letters 40, no 1 (16 janvier 2013) : 17–21. http://dx.doi.org/10.1029/2012gl054635.

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Yan, Bo, Punam K. Prasad, Sayan Mukherjee, Asit Saha et Santo Banerjee. « Dynamical Complexity and Multistability in a Novel Lunar Wake Plasma System ». Complexity 2020 (16 mars 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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CUI, Wei, et Lei LI. « 2D MHD Simulation of the Lunar Wake ». Chinese Journal of Space Science 28, no 3 (2008) : 189. http://dx.doi.org/10.11728/cjss2008.03.189.

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Tao, J. B., R. E. Ergun, D. L. Newman, J. S. Halekas, L. Andersson, V. Angelopoulos, J. W. Bonnell et al. « Kinetic instabilities in the lunar wake : ARTEMIS observations ». Journal of Geophysical Research : Space Physics 117, A3 (mars 2012) : n/a. http://dx.doi.org/10.1029/2011ja017364.

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Xie, LiangHai, Lei Li, YiTeng Zhang et Darren Lee De Zeeuw. « Three-dimensional MHD simulation of the lunar wake ». Science China Earth Sciences 56, no 2 (11 avril 2012) : 330–38. http://dx.doi.org/10.1007/s11430-012-4383-6.

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Zhang, H., K. K. Khurana, M. G. Kivelson, V. Angelopoulos, W. X. Wan, L. B. Liu, Q. G. Zong, Z. Y. Pu, Q. Q. Shi et W. L. Liu. « Three-dimensional lunar wake reconstructed from ARTEMIS data ». Journal of Geophysical Research : Space Physics 119, no 7 (juillet 2014) : 5220–43. http://dx.doi.org/10.1002/2014ja020111.

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Rasca, Anthony P., Shahab Fatemi et William M. Farrell. « Modeling the Lunar Wake Response to a CME Using a Hybrid PIC Model ». Planetary Science Journal 3, no 1 (1 janvier 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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Xu, Shaosui, Andrew R. Poppe, Jasper S. Halekas, David L. Mitchell, James P. McFadden et Yuki Harada. « Mapping the Lunar Wake Potential Structure With ARTEMIS Data ». Journal of Geophysical Research : Space Physics 124, no 5 (mai 2019) : 3360–77. http://dx.doi.org/10.1029/2019ja026536.

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Rubia, R., S. V. Singh et G. S. Lakhina. « Occurrence of electrostatic solitary waves in the lunar wake ». Journal of Geophysical Research : Space Physics 122, no 9 (septembre 2017) : 9134–47. http://dx.doi.org/10.1002/2017ja023972.

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Sreeraj, T., S. V. Singh et G. S. Lakhina. « Electrostatic waves driven by electron beam in lunar wake plasma ». Physics of Plasmas 25, no 5 (mai 2018) : 052902. http://dx.doi.org/10.1063/1.5032141.

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Thèses sur le sujet "Lunar wake"

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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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Birch, Paul C. « Particle-in-cell simulations of the lunar wake ». Thesis, University of Warwick, 2001. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.392768.

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Sandford, David J. « Dynamics of the stratosphere, mesosphere and thermosphere ». Thesis, University of Bath, 2008. https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.512300.

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This thesis presents observations of the dynamical features of the stratosphere, mesosphere and lower thermosphere. These are made from various observational techniques and model comparisons. A focus of the work is the two-day wave at high latitudes in the MLT region. This has revealed significant wave amplitudes in both summer and winter. However, these waves are shown to have very different origins. Using satellite data, the summertime wave is found to be the classic quasi-two-day wave which maximises at mid-latitudes in the MLT region. The wintertime wave is found to be a mesospheric manifestation of an eastward-propagating wave originating in the stratosphere and likely generated by barotropic and baroclinic instabilities in the polar night jet. The horizontal winds from Meteor and MF radars have been used to measure and produce climatologies of the Lunar M2 tide at Esrange in the Arctic (68°N), Rothera and Davis in the Antarctic (68°S), Castle Eaton at mid-latitude (52°N) and Ascension Island at Equatorial latitudes (8°S). These observations present the longest period of lunar semi-diurnal tidal observations in the MLT region to date, with a 16-year dataset from the UK meteor radar. Comparisons with the Vial and Forbes (1994) lunar tidal model are also made which reveal generally good agreement. Non-migrating lunar tides have been investigated. This uses lunar tidal results from equatorial stations, including the Ascension Island (8°S) meteor radar. Also lunar tidal results from the Rothera meteor wind radar (68°S, 68°W) and the Davis MF radar (68°S, 78°E) are considered. Both of these stations are on the edge of the Antarctic continent. It is demonstrated that there are often consistent tidal phase offsets between similar latitude stations. This suggests that non-migrating modes are likely to be present in the lunar semi-diurnal tidal structure and have significant amplitudes.
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李鍾嵐. « A Study of the Lunar Atmospheric Tidal Wave ». Thesis, 1998. http://ndltd.ncl.edu.tw/handle/07216023440513274958.

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碩士
輔仁大學
物理學研究所
86
The study tends to analyze geopotential which measured by radiosondes using the vertical phase and group velocities calculation methods within Taiwan area. There are oscillations phenomenon in 29. 5 day period from January 1996 to February 1998. We also noticed the phenomenon is caused by the interaction of gravity between the earth and moon. We named the phenomenon as lunar atmospheric tidal. From the calculation of vertical group velocities, we find that the vertical group velocities is upward behind the troposphere; the direction of vertical group velocities below troposphere is downward. This shows us the energy of the waving should generate from stir up of atmosphere near troposphere. Furthermore through the characteristics of transmission of wave, we can understand more about mechanism of waves caused by lunar atmospheric tidal in lower atmosphere.
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Livres sur le sujet "Lunar wake"

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Lunar wake. Winnipeg, Man : Turnstone Press, 1994.

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Birch, Paul Colin. Particle-in-cell simulations of the lunar wake. [s.l.] : typescript, 2001.

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Simon, Charnan. Luna the Wake-up Cat. New York : Children's Press, 2011.

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Noi conquisteremo la luna : Scritti sulla new wave italiana, 1980-1985. [Rome, Italy] : Rave up books, 2013.

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D, Sokolski Henry, Riisager Thomas et Army War College (U.S.). Strategic Studies Institute., dir. Beyond Nunn-Lugar : Curbing the next wave of weapons proliferation threats from Russia. Carlisle, PA : Strategic Studies Institute, U.S. Army War College, 2002.

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Simon, Charnan. Luna the Wake-up Cat (Rookie Readers). Children's Press (CT), 2007.

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Simon, Charnan. Luna the Wake-up Cat (Rookie Readers). Children's Press (CT), 2006.

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Wake Me When It's Over. Selena Press, 2012.

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Wave Good-bye (Luna Bay). Turtleback Books Distributed by Demco Media, 2003.

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Lantz, Francess Lin. Wave Good-bye (Luna Bay (Turtleback)). Tandem Library, 2003.

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Chapitres de livres sur le sujet "Lunar wake"

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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 ». Dans 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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Brodbeck, Simon. « The Yuga Cycle in the Mahābhārata ». Dans Divine Descent and the Four World-Ages in the Mahābhārata – or, Why Does the Kṛṣṇa Avatāra Inaugurate the Worst Yuga ?, 13–46. Cardiff University Press, 2022. http://dx.doi.org/10.18573/book9.b.

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Chapter 2 initiates discussion of the cycle of four yugas. The Manusmṛti passage on this topic is presented and discussed, as are the various Mahābhārata passages. Chapter 2 is a long chapter because the yuga cycle is peculiar in various ways, and resists easy conceptualisation. One section discusses the fact that many parameters – notably lifespan, goodness (dharmicness), and length of yuga – are part of one complex variable, which is shifted down through levels and up again. One section differentiates this sawtooth cycle of levels (from 4, to 3, to 2, to 1, then right back up to 4 again) from the smooth sine-wave alternations within the diurnal, lunar, and annual cycles. A final section differentiates the Mahābhārata’s (and the Manusmṛti’s) yuga scheme from the longer yuga scheme found in various Purāṇas.
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Brown, Mike. « A Fourth Wave of Education for Sustainability (EfS) in Higher Education ». Dans Advancing Knowledge in Higher Education, 151–69. IGI Global, 2014. http://dx.doi.org/10.4018/978-1-4666-6202-5.ch010.

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Education for Sustainability (EfS) in Higher Education (HE) is described as developing through three waves. These are overviewed in this chapter and given due acknowledgement but are shown to fall short of what is needed going forward. Consequently, a fourth wave of EfS in HE is proposed. The fourth wave of EfS in HE needs to be directed at the collaborative project of constructing “sustainable universities” (Sterling, Maxey, & Luna, 2013). The concept of “neo-sustainability” (Farley & Smith, 2014) is adopted as the basis of this next wave, as is the three nested rings model of sustainability. The argument for a strategy to educate the HE educators is outlined. It is suggested that contemporary global and local sustainability issues need to become part of student engagement within all HE courses. Finally, effort needs to be exerted by HE lecturers to develop pedagogical practices that align to the aims and principles of EfS.
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Lindsey, Susan E. « May I But Safely Reach My Home ». Dans Liberty Brought Us Here, 1–8. University Press of Kentucky, 2020. http://dx.doi.org/10.5810/kentucky/9780813179339.003.0001.

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On Tolbert Major’s last day in America, he wakes at dawn in a room at the Staten Island Quarantine Grounds. He rouses his sons and then walks down to the pier to see the Luna, the vessel that will take him and his family to Liberia, Africa. Tolbert recalls the send-off ceremony held the previous day, July 4, 1836, when officials from the New York Colonization Society joined dozens of newly emancipated slaves and freeborn black people in singing hymns, praying, and listening to speeches. (The emigrants weren’t ill; the mayor had temporarily housed them at the quarantine grounds.) The next morning, Tolbert, his sons, his brother Austin, their former neighbor Agnes Harlan, and the other emigrants board the ship Luna and prepare to sail. The passengers endure seasickness and weeks of anticipation as they sail across the Atlantic. Every sunset leaves behind loved ones and everything that is familiar. Every sunrise tugs them toward a new life.
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« Hudson River Fishes and their Environment ». Dans Hudson River Fishes and their Environment, sous la direction de Alan F. Blumberg et Ferdi L. Hellweger. American Fisheries Society, 2006. http://dx.doi.org/10.47886/9781888569827.ch2.

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<em>Abstract.</em>—The Hudson River Estuary can be classified as a drowned river valley, partially mixed, tidally dominated estuary. Originally, it had a fjord-like morphology as a result of glacial scour which filled in over the past 3,000 years with river sediments. The hydrodynamics of the estuary are best described by the drivers of circulation, including the upstream river inflows, the oceanographic conditions at the downstream end, and meteorological conditions at the water surface and the response of the waters to these drivers in terms of tides and surges, currents, temperature, and salinity. Freshwater inflow is predominantly from the Mohawk and Upper Hudson rivers at Troy (average flow = 400 m<sup>3</sup>/s, highest in April, lowest in August). At the downstream end at the Battery the dominant tidal constituent is the semidiurnal, principal lunar constituent (the M<sub>2</sub> tide), with an evident spring/neap cycle. The amplitude of the tide is highest at the Battery (67 cm), lower at West Point (38 cm), and higher again at Albany (69 cm), a function of friction, geometry, and wave reflection. Meteorological events can also raise the water surface elevation at the downstream end and propagate into the estuary. Freshwater pulses can raise the water level at the upstream end and propagate downstream. Tidal flows are typically about an order of magnitude greater than net flows. The typical tidal excursion in the Hudson River Estuary is 5–10 km, but it can be as high as 20 km. Temperature varies seasonally in response to atmospheric heating and cooling with a typical August maximum of 25°C and January-February minimum of 1°C. Power plants cause local heating. The salinity intrusion varies with the tide and amount of upstream freshwater input. The location of the salt front is between Yonkers and Tappan Zee in the spring and just south of Poughkeepsie in the summer. Vertical salinity stratification exists in the area of salt intrusion setting up an estuarine circulation. The effect of wind is limited due to a prevailing wind direction perpendicular to the main axis and the presence of cliffs and hills. Dispersive processes include shear dispersion and tidal trapping, resulting in an overall longitudinal dispersion coefficient of 3–270 m<sup>2</sup>/s. The residence or flushing time in the freshwater reach is less than 40 d in the spring and about 200 d in the summer. In the area of salt intrusion, it is about 8 d.
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« Hudson River Fishes and their Environment ». Dans Hudson River Fishes and their Environment, sous la direction de Alan F. Blumberg et Ferdi L. Hellweger. American Fisheries Society, 2006. http://dx.doi.org/10.47886/9781888569827.ch2.

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<em>Abstract.</em>—The Hudson River Estuary can be classified as a drowned river valley, partially mixed, tidally dominated estuary. Originally, it had a fjord-like morphology as a result of glacial scour which filled in over the past 3,000 years with river sediments. The hydrodynamics of the estuary are best described by the drivers of circulation, including the upstream river inflows, the oceanographic conditions at the downstream end, and meteorological conditions at the water surface and the response of the waters to these drivers in terms of tides and surges, currents, temperature, and salinity. Freshwater inflow is predominantly from the Mohawk and Upper Hudson rivers at Troy (average flow = 400 m<sup>3</sup>/s, highest in April, lowest in August). At the downstream end at the Battery the dominant tidal constituent is the semidiurnal, principal lunar constituent (the M<sub>2</sub> tide), with an evident spring/neap cycle. The amplitude of the tide is highest at the Battery (67 cm), lower at West Point (38 cm), and higher again at Albany (69 cm), a function of friction, geometry, and wave reflection. Meteorological events can also raise the water surface elevation at the downstream end and propagate into the estuary. Freshwater pulses can raise the water level at the upstream end and propagate downstream. Tidal flows are typically about an order of magnitude greater than net flows. The typical tidal excursion in the Hudson River Estuary is 5–10 km, but it can be as high as 20 km. Temperature varies seasonally in response to atmospheric heating and cooling with a typical August maximum of 25°C and January-February minimum of 1°C. Power plants cause local heating. The salinity intrusion varies with the tide and amount of upstream freshwater input. The location of the salt front is between Yonkers and Tappan Zee in the spring and just south of Poughkeepsie in the summer. Vertical salinity stratification exists in the area of salt intrusion setting up an estuarine circulation. The effect of wind is limited due to a prevailing wind direction perpendicular to the main axis and the presence of cliffs and hills. Dispersive processes include shear dispersion and tidal trapping, resulting in an overall longitudinal dispersion coefficient of 3–270 m<sup>2</sup>/s. The residence or flushing time in the freshwater reach is less than 40 d in the spring and about 200 d in the summer. In the area of salt intrusion, it is about 8 d.
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Actes de conférences sur le sujet "Lunar wake"

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Nishino, Masaki N., Yoshifumi Saito, Yoshiya Kasahara, Yoshiharu Omura, Kozo Hashimoto, Takayuki Ono, Hideo Tsunakawa, Futoshi Takahashi, Shoichiro Yokota et Masaki Fujimoto. « Plasma and wave observations in the deep lunar wake ». Dans 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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Nishino, Masaki N., Yoshifumi Saito, Yoshiya Kasahara, Yoshiharu Omura, Kozo Hashimoto, Takayuki Ono, Hideo Tsunakawa, Futoshi Takahashi et Masaki Fujimoto. « Wave excitation in the lunar wake associated with solar-wind proton entry ». Dans 2011 XXXth URSI General Assembly and Scientific Symposium. IEEE, 2011. http://dx.doi.org/10.1109/ursigass.2011.6051091.

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Okten, M. Baran, et Zehra Can. « Effect of the Earth's Magnetosphere on the Lunar Wake ». Dans 2021 XXXIVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS). IEEE, 2021. http://dx.doi.org/10.23919/ursigass51995.2021.9560470.

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Peng, Song, Yang Jia, He Tian et Tianyi Zhang. « Research on dormancy and wake-up control strategy of Chang’e-4 lunar rover ». Dans 2021 WRC Symposium on Advanced Robotics and Automation (WRC SARA). IEEE, 2021. http://dx.doi.org/10.1109/wrcsara53879.2021.9612689.

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Johnson, Warren W. « The moon as a gravitational wave detector, using seismometers ». Dans Physics and Astrophysics from a Lunar Base. AIP, 1990. http://dx.doi.org/10.1063/1.39102.

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Stebbins, R. T., et P. L. Bender. « A lunar gravitational wave antenna using a laser interferometer ». Dans Physics and Astrophysics from a Lunar Base. AIP, 1990. http://dx.doi.org/10.1063/1.39103.

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Yushkov, Vyacheslav, Roman Rudamenko, Taisia Dymova et Olga Yushkova. « Modeling Bictatic Radio Sounding of the Lunar Soil ». Dans 2019 Russian Open Conference on Radio Wave Propagation (RWP). IEEE, 2019. http://dx.doi.org/10.1109/rwp.2019.8810377.

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Wang, Zhenzhan, Yun Li, Dehai Zhang, Jingshan Jiang, Jin Zhao, Fenglei Hua et Xiaohui Zhang. « Prelaunch calibration of Chang'E-2 Lunar Microwave radiometer ». Dans 2010 International Conference on Microwave and Millimeter Wave Technology (ICMMT). IEEE, 2010. http://dx.doi.org/10.1109/icmmt.2010.5524886.

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Rodeghiero, Gabriele, Claudio Pernechele, Matteo Munari, Riccardo Pozzobon, Maurizio Pajola, Ivan Di Antonio, Alice Lucchetti et al. « Radiance values inside lunar caves and lava tubes ». Dans Space Telescopes and Instrumentation 2022 : Optical, Infrared, and Millimeter Wave, sous la direction de Laura E. Coyle, Marshall D. Perrin et Shuji Matsuura. SPIE, 2022. http://dx.doi.org/10.1117/12.2628901.

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

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Rapports d'organisations sur le sujet "Lunar wake"

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Sokolski, Henry D., et Thomas Riisager. Beyond Nunn-Lugar : Curbing the Next Wave of Weapons Proliferation Threat from Russia. Fort Belvoir, VA : Defense Technical Information Center, avril 2002. http://dx.doi.org/10.21236/ada401464.

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