[PDF] Top 20 Solar wind proton reflection and injection to the ACR regime at the parallel termination shock
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Solar wind proton reflection and injection to the ACR regime at the parallel termination shock
... quasi-perpendicular shock is expected during most of the time at the heliospheric bound- ary (Parker, ...bow shock, quasi-parallel shock crossings are observed, ...the solar wind ... See full document
5
Self-initialised Fermi-1 acceleration by pitch-angle re-scattering of solar wind ions reflected from the parallel termination shock
... the solar wind ter- mination shock under a parallel magnetic field ...upstream solar wind reference ...the shock, tend to attenu- ate the shock a little and lead to ... See full document
8
Spectral intensities of Anomalous Cosmic Rays derived from the injection rate at the solar wind termination shock
... the solar wind termination shock (Fisk et ...instance ACR protons are especially seen at some phases of low solar activity on top of the modulated galactic cosmic ray spectrum in ... See full document
10
Plasma Waves in the Sun
... Plasma waves are omnipresent in space plasmas and are observed in our solar system [1, 2]. They propagate energy across different space regions, transport particles in the absence of collisions, and provide ... See full document
5
A heliospheric hybrid model: hydrodynamic plasma flow and kinetic cosmic ray transport
... with solar cycle re- lated changes in the latitudinal profile of the solar ...the solar wind speed for selected periods over a 11-year cycle as three plots representing increasing solar ... See full document
11
Multi scale analysis of compressible fluctuations in the solar wind
... flow) and also implicitly assumes Taylor’s hypothesis, i.e. that there is no temporal change. Thus, the magnetic helic- ity varies between − 1 and + 1 and for this definition can be regarded as being the same as ... See full document
6
April 2000 magnetic storm: Solar wind driver and magnetospheric response
... obtained shock normal had large latitudinal angle, q ’ 40 consistent with source in the Northern Hemisphere and the longitudinal angle f ’ 170 that is consistent with the CME originating from west but the ... See full document
21
Correlation of solar wind velocity with different parameters during geomagnetic disturbances
... slower solar wind preceding ...the shock and the field compression, had investigated the effect of solar wind dynamic pressure Psw, and preconditioning over 80 large magnetic storms ... See full document
12
Using Floating Photovoltaics, Electrolyser and Fuel Cell to Decrease the Peak Load and Reduce Water Surface Evaporation
... of solar panels on the surface of water, the efficiency of panels increases and in addition, the surface evaporation of water will be ...of solar panel on surface of the Tanguie dam is studied from ... See full document
14
Magnetic reconnection associated fluctuations in the deep magnetotail: ARTEMIS results
... The “Acceleration, Reconnection, Turbulence and Electro- dynamics of Moon’s Interaction with the Sun” (ARTEMIS) NASA mission addresses the dynamics, scale size and en- ergy balance of deep-tail particle acceleration and ... See full document
9
Coronal mass ejections and Jump in solar wind plasma temperature in association with shock related geomagnetic storms
... earth solar wind, magnetic field and plasma data of omni data set, which consists of one hour resolution near earth, solar wind magnetic field and plasma data, energetic proton fluxes ... See full document
6
Perpetual Motion with Solar and Wind Energy Hybrid System
... Abstract- This paper deals with optimal design of hybrid solar and wind energy system with perpetual motion. This design gives flexibility in siting new sources of generation of electrical energy. The ... See full document
5
Fast magnetoacoustic waves in non equilibrium solar wind and coronal plasmas
... QPP are the quasi-periodic variation in time of flare generated emission in a variety of different bands. Oscillatory variations in the radio and microwave emission from flaring loops have been investigated for several ... See full document
188
The Scenario of Tsunami Propagation at the Celebes Sea and the Disaster Impacts to Tawau District
... Simulation of tsunami wave propagation shows the tsunami wave distribution from the source of the generator in Parit Cotabato and spread to Celebes Sea takes 80 [r] ... See full document
9
Effect of wind velocity on active and passive solar still
... different masses (passive stills) or different thicknesses and mass flow rates (active stills) of saline water. It has been found that for the active and multi-effect passive solar stills, the daily productivity ... See full document
5
Jump conditions for pressure anisotropy and comparison with the Earth’s bow shock
... oblique shock fol- lowing the technique performed by Erkaev et ...the WIND spacecraft to determine the input parameters, solve the set of equations, and compare our theoretical results with the ... See full document
8
Development and management of solar and wind hybrid technology for the progress of India
... Lift-style wind turbines have a theoretical maximum conversion efficiency of wind energy to mechanical energy, called the Betz Limit, of ...lift wind turbines, from wind power to electrical ... See full document
6
Cassini observations of ionospheric plasma in Saturn's magnetotail lobes
... Figure 1. Cassini’s trajectory in Kronocentric Solar Magnetospheric Coordinates (KSM) for Cassini’s rev. 27 of Saturn from 04 August to 28 August 2006 projected in the X-Y plane (top) and noon-midnight meridional ... See full document
79
Effect of Solar Influences on Earths Magnetosphere and Upper Atmosphere
... total solar eclipse (or an artificial eclipse created by a specialized telescope called a coronagraph), when it appears as a pale cloud encircling the ...The solar wind leaves the corona, it flows ... See full document
9
Cavitons and spontaneous hot flow anomalies in a hybrid Vlasov global magnetospheric simulation
... bow shock. We report on SHFAs surviving the shock crossing into the down- stream region and show that the interaction of SHFAs with the bow shock can lead to the formation of a magnetosheath cavity, ... See full document
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