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[PDF] Top 20 WIND observations of coherent electrostatic waves in the solar wind

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WIND observations of coherent electrostatic waves in the solar wind

WIND observations of coherent electrostatic waves in the solar wind

... consider the question of how the electrostatic activity observed by the WIND/WAVES experiment depends on the local parameters of the solar ... See full document

14

Lidar observations of atmospheric internal waves in the boundary layer of
the atmosphere on the coast of Lake Baikal

Lidar observations of atmospheric internal waves in the boundary layer of the atmosphere on the coast of Lake Baikal

... total of six cases of AIW formation have been revealed, which always occurred in the presence of one or two (in five out of six cases) narrow jet streams at heights ... See full document

10

First simultaneous measurements of waves generated at the bow shock in the solar wind, the magnetosphere and on the ground

First simultaneous measurements of waves generated at the bow shock in the solar wind, the magnetosphere and on the ground

... position of Geotail. Upstream generated waves were sub- sequently observed by Geotail between 18:30 and 18:48 UT, during times the IMF cone angle dropped below values of 10 ◦ ...increase ... See full document

15

Solar-wind control of plasma sheet dynamics

Solar-wind control of plasma sheet dynamics

... and the occurrence rate of fast flow bursts have also been studied during two differ- ent AE index ...levels. The results are shown in Fig. 8. AE describes the geomagnetic disturbance ... See full document

11

Effects of a solar wind dynamic pressure increase in the magnetosphere and in the ionosphere

Effects of a solar wind dynamic pressure increase in the magnetosphere and in the ionosphere

... observing the solar wind, the magneto- sphere, and the ...ionosphere. Solar wind data are from the Advanced Composition Explorer (ACE), Solar and Helio- ... See full document

15

Turbulent wind waves on a water current

Turbulent wind waves on a water current

... θ=β+π. The uncertainty zero divided by zero at K=0, θ =β, θ=β+π in the formula (19) is prescribed the value zero, since any κ-waves at K 6 =0 at the directions θ=β, θ =β+π have ... See full document

11

The effect of the high-speed stream following the corotating interaction region on the geomagnetic activities

The effect of the high-speed stream following the corotating interaction region on the geomagnetic activities

... studied the statistics of solar-wind parameters, which were observed by the Pioneer Venus Orbiter (PVO) between 1979 and 1988, in coronal mass ejections (CMEs) and ...than ... See full document

9

How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation

How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation

... estimates of the three-dimensional ve- locity structure of the inner heliosphere on a continuous ba- ...use the interplanetary scintillation observations of natural radio ... See full document

5

Simulated solar wind plasma interaction with the Martian exosphere: influence of the solar EUV flux on the bow shock and the magnetic pile-up boundary

Simulated solar wind plasma interaction with the Martian exosphere: influence of the solar EUV flux on the bow shock and the magnetic pile-up boundary

... asymmetry in the magnetic field intensity is ob- served in the XY plane ...while the field distribu- tion in the XZ plane ...to the action of the ... See full document

8

Modeling of short scale turbulence in the solar wind

Modeling of short scale turbulence in the solar wind

... Solar wind is a turbulent supersonic outflow of plasma from the solar ...Fluctuations in the density,the ve- locity and the magnetic fields exist on several ... See full document

7

Wavevector anisotropy of plasma turbulence at ion kinetic scales: solar wind observations and hybrid simulations

Wavevector anisotropy of plasma turbulence at ion kinetic scales: solar wind observations and hybrid simulations

... anisotropy of ion-scale plasma turbu- lence is studied at various values of ion ...measurements of magnetic field in the near-Earth solar wind as provided by the ... See full document

9

Velocity fluctuations in polar solar wind: a comparison between different solar cycles

Velocity fluctuations in polar solar wind: a comparison between different solar cycles

... passes in 1994 (South) and 1995 (North), during the declining phase of solar cycle ...22. In con- trast, the second set of polar passes in 2000–2001 occurred at ... See full document

7

Technical reconfiguration for optimal operation of integrated distributed system

Technical reconfiguration for optimal operation of integrated distributed system

... - The fuel in the earth will be exhausted in a thousand or more years, and its mineral wealth, but man will find substitutes for these in the winds, the waves, ... See full document

8

Dawn-dusk asymmetry in particles of solar wind origin within the magnetosphere

Dawn-dusk asymmetry in particles of solar wind origin within the magnetosphere

... to the equator and a period of ...to the orbital plane. The data set used in this study is from the Magnetospheric Ion Composition Sensor (MICS) in the Charge and ... See full document

9

Plasma waves above the ion cyclotron frequency in the solar wind: a review on observations

Plasma waves above the ion cyclotron frequency in the solar wind: a review on observations

... heat. The evolution of the first part of the diagram (low frequencies) is compatible with the WKB prop- agation of fluctuations in a spherically expanding ... See full document

11

Direct observations of the formation of the solar wind halo from the strahl

Direct observations of the formation of the solar wind halo from the strahl

... As the solar wind propagates away from the sun, the mir- ror force should focus the strahl in ...and the lo- cal plasma. The broadening begins where ... See full document

13

The solar wind at solar maximum: comparisons of EISCAT IPS and in situ observations

The solar wind at solar maximum: comparisons of EISCAT IPS and in situ observations

... between in situ and radio-scintillation obser- vations of the solar wind have been carried out in the past, us- ing both measurements of IPS (Behannon et ...but ... See full document

19

Magnetosheath waves under very low solar wind dynamic pressure: Wind/Geotail observations

Magnetosheath waves under very low solar wind dynamic pressure: Wind/Geotail observations

... fluxes of solar wind origin. Judging from the behavior of the proton density, temperature, and magnetic field strength and the spectral characteristics, the first ... See full document

17

Application of the Aventech AIMMS20AQ airborne probe for turbulence measurements during the Convective Storm Initiation Project

Application of the Aventech AIMMS20AQ airborne probe for turbulence measurements during the Convective Storm Initiation Project

... application in the United States. In conse- quence, economies of scale ensure the probe is robust, reliable, relatively low cost and easy to install and ...Whilst the Cessna uses ... See full document

37

Blowing jets as a circulation flow control to enhancement the lift of wing or generated power of wind turbine

Blowing jets as a circulation flow control to enhancement the lift of wing or generated power of wind turbine

... investigate the aerodynamic performance of a wind turbine rotor equipped with circulation control technology (blowing ...jet). The highly beneficial impact to lift-to-drag (L/D) ratio from ... See full document

17

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