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Advanced effects in the solar wind driving

Different magnetospheric modes: solar wind driving and coupling efficiency

Different magnetospheric modes: solar wind driving and coupling efficiency

... The solar wind driving (dawn-dusk electric field and IMF B Z ) is the strongest for sawtooth events, the second strongest for the steady convections and the weakest over the periods of isolated ...

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-index solar wind driving function and its semiannual variations

-index solar wind driving function and its semiannual variations

... 2003) is ∼4 nT and consists of ∼2.1–2.3 nT of magneto- spheric/ionospheric part, 0.6–1.3 nT of heliospheric part (in- cluding 0.2–0.3 nT of R-M effect), 0.1–0.4 nT is due to the non-linear term. 90% confidence range of ...

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Solar wind velocity at solar maximum: A search for latitudinal effects

Solar wind velocity at solar maximum: A search for latitudinal effects

... the solar activity maxi- mum the solar wind appears as a highly variable flow at all ...latitudinal effects in the large-scale structure of the solar wind ...the wind ve- ...

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User s Manual Advanced Wind/Solar Hybrid Controller

User s Manual Advanced Wind/Solar Hybrid Controller

... specify wind turbine, the controller can achieve accurate speed control, namely, you can set the stop rotation ...the wind turbine exceeds this speed, the controller will stop the wind turbine ...

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Proton kinetic effects in vlasov and solar wind turbulence

Proton kinetic effects in vlasov and solar wind turbulence

... of solar wind turbulence, employing hybrid Vlasov–Maxwell (HVM) ...to solar wind sub-datasets. Moreover, both simulation and solar wind data suggest that temperature anisotropy ...

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Wind effects on roof-mounted solar photovoltaic arrays: CFD and wind-tunnel evaluation

Wind effects on roof-mounted solar photovoltaic arrays: CFD and wind-tunnel evaluation

... along wind static pressure ...for wind flow directed into the face of PV panel, into the face of the deflector and from the ...tiles; wind blew straight toward the wind deflectors; a straight ...

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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

... and Wind solar wind ...the solar wind dynamic pressure during northward interplanetary magnetic field conditions was related to the leading edge of the ...

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Effects of Solar and Wind Generation Integration on Feeder Hosting Capacity

Effects of Solar and Wind Generation Integration on Feeder Hosting Capacity

... One such example is for interconnection purposes since it is yet unclear who pays for the additional upgrades needed to interconnect to the system. The proposed framework may be used to determine the interconnection ...

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Advanced Wind/Solar Hybrid Controller. Model: WWS10A-48 Version 1.0

Advanced Wind/Solar Hybrid Controller. Model: WWS10A-48 Version 1.0

... by wind turbine and solar panels when total charge current of wind turbine and solar panels is lower than current limitting ...of wind turbine and solar panels exceeds current ...

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The distribution of solar wind speeds during solar minimum: calibration for numerical solar wind modeling constraints on the source of the slow solar wind

The distribution of solar wind speeds during solar minimum: calibration for numerical solar wind modeling constraints on the source of the slow solar wind

... the solar wind speed observed by Ulysses at a distance between ...fast wind at higher latitudes to slow highly variable wind speed at lower latitudes occur on days 400 and 453 at lati- tudes ...

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SuperDARN observations during geomagnetic storms, geomagnetically active times and enhanced solar wind driving

SuperDARN observations during geomagnetic storms, geomagnetically active times and enhanced solar wind driving

... phase, c: recovery phase, d: driven times, e: enhanced Sym-H index, irrespective of storm phase). Noon is to the top, and dusk to the left[r] ...

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SuperDARN observations during geomagnetic storms, geomagnetically active times and enhanced solar wind driving

SuperDARN observations during geomagnetic storms, geomagnetically active times and enhanced solar wind driving

... the solar wind driving decreases and Sym-H becomes less enhanced, the HMB and the FRB move to higher lat- itudes similar to at the start of the initial ...

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Wind and Solar Electricity:

Wind and Solar Electricity:

... from wind is close to cost competitive with electricity produced from natural gas—depending on natural gas prices, the availability of production tax credits, and other ...Moreover, wind becomes more cost ...

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Economic Effects of the Solar and Wind Energy Use

in Irrigation of Vegetable Cultures

Economic Effects of the Solar and Wind Energy Use in Irrigation of Vegetable Cultures

... robotized solar electrical generator has been tested (this time together with the mobile wind power generator) within the production of vegetables in the system which had included irrigation, since this ...

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Solar Activity, Solar Wind and Geomagnetic Signatures

Solar Activity, Solar Wind and Geomagnetic Signatures

... during solar cycles 20, 21, 22, and ...high solar wind stream; the QA is the effect of slow solar wind, and moderate and variable solar wind speeds are recorded during ...

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Deep Solar Activity Minimum 2007-2009: Solar Wind Properties and Major Effects on the Terrestrial Magnetosphere

Deep Solar Activity Minimum 2007-2009: Solar Wind Properties and Major Effects on the Terrestrial Magnetosphere

... i) an estimate of the cross-polar cap potential in its dependence on these interplanetary parameters (i.e. the dayside source of plasma convection in the magnetosphere), and ii) the shapes of the bow shock and ...

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Supermagnetosonic subsolar magnetosheath jets and their effects: from the solar wind to the ionospheric convection

Supermagnetosonic subsolar magnetosheath jets and their effects: from the solar wind to the ionospheric convection

... analysis of the jets showed that their properties are in agree- ment with the previous proposition (Hietala et al., 2009) that they are formed by ripples inherent to the quasi-parallel bow shock. We concluded that some ...

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Effects of solar wind density on auroral electrojets and brightness under influence of substorms

Effects of solar wind density on auroral electrojets and brightness under influence of substorms

... Abstract. Using the auroral electrojet indices and Polar Ul- traviolet Imager auroral images, we examined two fortuitous events during which the solar wind density had clear en- hancements while the other ...

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Effects of decreasing ionospheric pressure on the solar wind interaction with non magnetized planets

Effects of decreasing ionospheric pressure on the solar wind interaction with non magnetized planets

... The effects of decreased ionospheric pressure on the solar wind-interaction with non-magnetized planets have been investigated from numerical MHD ...dent solar wind dynamic pressure, ...

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Kinetic effects in the turbulent solar wind: capturing ion physics with a Vlasov code

Kinetic effects in the turbulent solar wind: capturing ion physics with a Vlasov code

... 2) In correspondence of these small scale structures, large temperature anisotropy with respect to the local magnetic field is recovered. 3) The temperature anisotropy plot from the [r] ...

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