Exact(11)
The statistic performance of power regression equation to calculate the PAR for each latitude is shown in Table 9.
Regression analyses between the PAR and the monthly average of daily global solar radiation are carried out for each latitude.
It is found that for each latitude the O 1S) nightglow emission rate appears to increase with increasing solar F10.7 cm flux, following a linear relationship.
In Table 3, we compile the column abundance of the aerosol for each latitude for each set of simulations in this section.
Since we are not performing rigorous radiative transfer calculations at this time, we would have had to have arbitrarily determined the penetration depth of photons for each latitude.
Fig. 21 Left: The total column abundance in the microphysical model domain (40 80 km) for each latitude and coagulation condition simulated here.
Similar(49)
We did not expect that our simple flux models would account for all variability across each latitude band.
The outward drift of winter air creates a sharp temperature anomaly in eastern and northeastern Asia, where the climate is colder than the characteristic global average for each given latitude.
Fig. 15 Contour plot of particle size distributions for the nominal photochemistry simulation, as functions of radius and altitude, for each simulated latitude profile.
Figures 13 and 14 show the average of Pearson coefficients calculated for Swarm A and C, and Pearson coefficients calculated for Swarm B, by considering all the three IRI topside options IRI-20011, IRI-2001corr, NeQuick), respectively, for morning and evening sectors, and for each magnetic latitude band.
Average of Pearson coefficients calculated for Swarm A and C (left panels), and Pearson coefficients calculated for Swarm B (right panels), for each magnetic latitude band (from top to bottom: NP, NM, EQ, SM, and SP), by considering all the three IRI topside models IRI-20011, IRI-2001corr, IRI-NeQuick), for morning and evening sectors.
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