Sentence examples for unresolved field from inspiring English sources

The unresolved field (tilde {B}_{r}) at small length-scales being correlated over decades, is also correlated in time (Gillet et al. 2015).

The formal separation between resolved and unresolved field is obtained by wavelet threshold filtering that is inherent to the adaptive wavelet collocation numerical method.

Finally, a quantitative criterion assessing the nature of the unresolved field based on the strain-rate ratio of mean and unresolved fields is examined.

To go further, we could reduce the importance of SV model errors by co-estimating the unresolved field at degrees n>14 (and its associated uncertainties) together with the field at large length-scales, following Aubert (2014) who performed such a co-estimation using the cross-covariances between Gauss coefficients obtained from the forward integration of a geodynamo simulation.

Although the issue remains unresolved, the field as a whole continues to grow in sophistication.

We propose a new subgrid scale model (RSEM), which is based on estimation of the unresolved velocity field.

Accounting for time-correlated model errors (subgrid processes associated with the unresolved magnetic field) is made possible thanks to the use of an augmented state ensemble Kalman filter algorithm.

In the present study, spatially unresolved magnetic fields in solar flares are investigated by analyzing the fine structure of Zeeman splitting in two FeI lines.

Close correlation (r = 0.77 ± 0.06) was found between (a) and (b) effects indicating the reality of very strong (≈8 kG) unresolved magnetic fields.

In order to search spectral evidences of very strong spatially unresolved magnetic fields, the Stokes I ± V and V profiles of the Fe I 6301.5 and 6302.5 Å lines are studied in detail.

We consider in (5) temporally correlated SV model errors arising from the interaction of the flow with temporally correlated, but unresolved, small-scale field from degrees 14 to 30.