نتایج جستجو برای: wind and solar dgs

تعداد نتایج: 16885312  

2007
E. Marsch

The magnetic field of the Sun and the plasma properties of its atmosphere, such as temperature distribution, density stratification, photospheric convection and waves in the corona, determine the origin, energetics and evolution of the solar wind. The solar wind comes in three main kinds, as steady fast streams, variable slow flows and transient slow and fast coronal mass ejections. The three t...

2017
G R Gladstone M H Versteeg T K Greathouse V Hue M W Davis J-C Gérard D C Grodent B Bonfond J D Nichols R J Wilson G B Hospodarsky S J Bolton S M Levin J E P Connerney A Adriani W S Kurth B H Mauk P Valek D J McComas G S Orton F Bagenal

Juno ultraviolet spectrograph (UVS) observations of Jupiter's aurora obtained during approach are presented. Prior to the bow shock crossing on 24 June 2016, the Juno approach provided a rare opportunity to correlate local solar wind conditions with Jovian auroral emissions. Some of Jupiter's auroral emissions are expected to be controlled or modified by local solar wind conditions. Here we com...

2009
J. Klačka

Action of solar wind on arbitrarily shaped interplanetary dust particle is investigated. The final relativistically covariant equation of motion of the particle contains both orbital evolution and change of particle’s mass. Non-radial solar wind velocity vector is also included. The covariant equation of motion reduces to the Poynting-Robertson effect in the limiting case when spherical particl...

خراسانی‌زاده, حسین, سبزپوشانی, مجید, عبداللهی طاهری, رضا,

Considering problems associated with nonrenewable fuels such as pollution and high cost, efforts are being made to develop use of renewable energy sources like solar energy. Solar collectors could often be employed as important devices for thermal applications. Unglazed Transpired Collector (UTC) is a modern preheating and heating equipment used for ventilating air or drying crops. Heat transfe...

2016
M. Volwerk I. Richter B. Tsurutani C. Götz K. Altwegg T. Broiles J. Burch C. Carr E. Cupido M. Delva M. Dósa N. J. T. Edberg A. Eriksson P. Henri C. Koenders J.-P. Lebreton K. E. Mandt H. Nilsson A. Opitz M. Rubin K. Schwingenschuh G. Stenberg Wieser K. Szegö C. Vallat X. Vallieres

The data from all Rosetta plasma consortium instruments and from the ROSINA COPS instrument are used to study the interaction of the solar wind with the outgassing cometary nucleus of 67P/Churyumov-Gerasimenko. During 6 and 7 June 2015, the interaction was first dominated by an increase in the solar wind dynamic pressure, caused by a higher solar wind ion density. This pressure compressed the d...

2016
A K Pradhan S K Kar M K Mohanty

The continuous power supply for rural areas can be possible by using renewable hybrid power generation system and also reduction of the energy storage devices for the system. The impact of the shortage of power supply probability, surpluspower power generation, ratio of the energy supply to load demand, renewable fraction of different types of energy resources (solar and wind) and the combined ...

Journal: :Frontiers in Energy Research 2023

Microgrids have benefited energy systems by getting rid of the abundant use traditional resources, replacing them with distributed generations (DGs). The DGs in microgrids not only provides clean and green but also reduces gigantic losses transmission distribution lines. Widespread adoption renewable saves customers from high fuel prices a sustainable replacement for future fossil depletion. pr...

M. Lajevardi S.A. ZanjaniGhayur

With regard to the importance of scientific decision-making in power plants prioritization to produce electrical energy (power) from renewable energies (purified), in this paper, research with specialists opinions with respond to questionnaires provided upon three efficient operational criterion in position of three presented power plant in country which used wind, solar water energies for prod...

2006
M. H. Denton J. E. Borovsky R. M. Skoug M. F. Thomsen B. Lavraud M. G. Henderson R. L. McPherron J. C. Zhang M. W. Liemohn

[1] The interaction of the solar wind and the Earth’s magnetosphere is complex and the phenomenology of the interaction is very different for solar wind dominated by interplanetary coronal mass ejections (ICMEs) compared to solar wind dominated by corotating interaction regions (CIRs). We perform a superposed epoch study of the effects of ICMEand CIR-dominated solar wind upon the storm-time pla...

1998
G. P. Zank W. H. Matthaeus C. W. Smith

The deposition of energy into the solar wind beyond 1 AU is thought to result from the dissipation of low frequency magnetohydrodynamic (MHD) turbulence via kinetic processes at spatial scales comparable to the ion gyroradius. Beyond 1 AU, solar wind turbulence is comprised of both a decaying component generated in the corona and turbulence generated dynamically in situ by processes such as str...

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