[PDF] Top 20 Solar wind reconstruction from magnetosheath data using an adjoint approach
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Solar wind reconstruction from magnetosheath data using an adjoint approach
... reconstructed solar wind parameters and the OMNI, as well as the THB solar wind data, are presented in ...The solar wind density of THB and OMNI show an off- set of about ... See full document
12
A variational approach to data assimilation in the solar wind
... Near-Earth solar wind speed (at L1) for 12 Carrington rotations spanning Oct 2010 to Oct ...observed solar wind speed in near-Earth space by the ACE ...generated using the MAS ensemble, ... See full document
69
A correlation study regarding the AE index and ACE solar wind data for Alfvénic intervals using wavelet decomposition and reconstruction
... real-time data from a spacecraft around L1 and verify the Alfvénicity through the technique employed by Belcher and Davis ...the data series would be fed in through the wavelet filtering and the AE ∗ ... See full document
10
Reconstruction of a large-scale reconnection exhaust structure in the solar wind
... MHD reconstruction maps of the bifurcated current sheet seen by ACE on 2 February 2002, during the interval of 00:12:12– 02:57:32 ...and Wind are ∼31 R E and ∼110 R E , respectively, in the ... See full document
16
Wind speed time series reconstruction using a hybrid neural genetic approach
... came from fossil fuels, making irreversible damage to the ...energy using clean methods, such as solar and wind energy, among ...others. Wind energy is one of the cleanest alternatives. ... See full document
10
Reconstruction of Helio-Latitudinal Structure of the Solar Wind Proton Speed and Density
... speed data derived from the IPS observations of STEL (Tokumaru, Kojima, and Fujiki, ...IPS data were deconvolved using the computer- assisted tomography method (CAT; Asai et ...breaks ... See full document
27
Astronomy. Astrophysics. Reconstruction of solar activity for the last millennium using 10 Be data
... first approach is based on mathematical extrapolation using the statistical properties of the SN record observed during the last 300 ...fragmentary data from naked-eye sunspot observations or ... See full document
7
Real-time wind-field reconstruction from LiDAR measurements using a dynamic wind model and state estimation.
... the wind energy indus- ...the wind, making it difficult to precisely determine wind magnitude and direction, owing to the so-called ‘cyclops’ ...information from typical LiDAR data, ... See full document
18
Probabilistic solar wind and geomagnetic forecasting using an analogue ensemble or "Similar Day" approach
... a solar-wind AnEn forecast, we use the OMNI series of near-Earth in-situ space- craft observations (King and Papitashvili, 2005) at one-hour ...the solar-rotation direction means that there are ... See full document
16
Selection of biogas, solar, and wind power plants’ locations: An MCDA approach
... multi-criteria approach to locating biogas, solar and wind power plants that significantly addresses the challenge of global warming caused by power ...biogas, solar and wind power ... See full document
27
Optimization of wind plant layouts using an adjoint approach
... of wind plant optimization ...optimization approach that combines sequential linear programming (SLP) with gradient-free genetic ...nite wind plants with turbines arranged in regular gridded tur- ... See full document
17
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 ... See full document
16
Solar wind vs magnetosheath turbulence and Alfv´en vortices
... lar wind and the Earth ...the magnetosheath turbulence is the presence of Alfv´en vortices at scales of the spectral ...observed magnetosheath spectrum in presence of the Alfv´en vortices can be ... See full document
14
Magnetosheath waves under very low solar wind dynamic pressure: Wind/Geotail observations
... because solar wind densities decreased to low values of or- der ...the magnetosheath, which may be isolated and studied by comparing them with a long segment of the same pass when MHD effects were ... See full document
17
ANGEO - Magnetopause stand-off distance in dependence on the magnetosheath and solar wind parameters
... the magnetosheath structure proposed in a recent paper from the authors is extended to estimate the magnetopause stand-o distance from solar wind ...the magnetosheath and ... See full document
9
Low frequency wave sources in the outer magnetosphere, magnetosheath, and near Earth solar wind
... the magnetosheath waves are gener- ated within a distance of 2000 km from the spacecraft con- figuration ...move from the shock towards the ...trend, from values indicating no significant ... See full document
12
Refractivity from Clutter by Variational Adjoint Approach
... variational adjoint approach for RFC measurement geometry. The adjoint model is derived from the parabolic equation method for a smooth, perfectly conducting surface and horizontal ... See full document
22
Mirror mode waves in Venus’s magnetosheath: solar minimum vs. solar maximum
... for solar minimum B ≈ 0.59 ± 0.36 (32 events) is higher than for solar maxi- mum with B ≈ ...for solar minimum as indicated by the given standard ...for solar minimum the en- ergization of the ... See full document
10
Using an Adjoint Approach to Eliminate Mesh Sensitivities in Computational Design
... performed using 64 Opteron processors. Here, the flow solver and its adjoint counterpart have each been run 1000 time steps, using the tightly coupled implementation of ...flowfield adjoint ... See full document
10
Helioseismic and neutrino data-driven reconstruction of solar properties
... the solar radius determined by performing sound speed inversions as described in Basu et ...in solar models is longer than the resolution achieved by using 30 radial points, as described in Section ... See full document
17
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