Sentence examples for evolution of fluxes from inspiring English sources

As Ribas et al. (2005) give no power laws for the evolution of fluxes longward of 1200 Å, we used their equation (2) and the observational data given in their table 6 to estimate the flux evolution between 1200 1700 Å. Ribas et al. (2005) give observed emission line fluxes of six solar analogs (including the Sun), eight lines have wavelengths > 1200 Å.

In order to better understand the seasonal evolution of fluxes taking into account the changes observed in footprint areas between dry and wet seasons, monthly cumulated values of carbon fluxes (NEE, R and Gp) are presented in Figs. 11 and 12. Overall, along the year, the carbon flux dynamics were unsurprisingly submitted to a strong seasonal variability.

In order to better understand the seasonal evolution of fluxes taking into account the changes observed in footprint areas between dry and wet seasons, monthly cumulated values of carbon fluxes (NEE, R and Gp) are presented in Figs.  11 and 12. Overall, along the year, the carbon flux dynamics were unsurprisingly submitted to a strong seasonal variability.

The time evolution of flux and energy distribution of electrons and ions at the object surface were also obtained.

The evolution of flux and wall concentration over time is obtained for selected values of the polarisation and adsorption parameters involved, particularly in reference to protein ultrafiltration.

The evolution of flux control and selection on enzyme polymorphisms has been intensively studied in the glycolytic pathway of Drosophila[ 3, 6, 10, 11].

In this paper, we study the relation of flare productivity of active regions with their evolution of magnetic flux emergence, flux imbalance and free energy content.

Figure 9 Evolution of energy fluxes with the distance along the jet in models A (left panel) and B (right panel).

The temporal evolution of biogenic fluxes with meteorological conditions is calculated on line in the MesoNH C meso-scale atmospheric chemistry model.

If ˆφ is the entropy production, then the construction gives the non-steady evolution of thermodynamic fluxes to steady states distinguished by ˆφ and produces physically realistic finite velocity thermal and mass transport.

Fig. 3. Evolution of the fluxes at 1 AU in different wavelength regimes (X-ray: 1 20 Å, long dashes; SXR: 20 100 Å, dashed line; EUV: 100 920 Å, dash-dotted line; FUV: 920 1180 Å, dotted line; Ly-α: 1200 1300 Å, grey solid line; UV: 1300 1700 Å, grey dashed line with diamonds) normalized to the present solar values.