Suggestions(1)
Exact(3)
Ohya et al. 2007) indicated that GCR ionization is less intense under solar maximum conditions and the decrease of GCRs due to high solar activities may cause the decrease in the electron density in the D and lower E region of the ionosphere.
Statistically, for frequencies f ∼ 1 GHz (near current wireless bands), there can be a burst with amplitudes >103 solar flux units (SFU; 1 SFU = 10−22 W/m2) every few days during solar maximum conditions, and such burst levels can produce problems in contemporary wireless systems.
Its result is a binary image where white pixels indicate edge pixels selected by not only having their large value in Sobel filter response but also satisfying local maximum conditions and connectivity to the local maximum.
Similar(57)
The saturated optimal control force is determined from maximum condition and solving the forward backward stochastic differential equations (FBSDEs).
Using a relatively simple and approximate theoretical model calculation of an upward drift of the equatorial ionospheric plasma, based on the analytic solutions of the continuity equation for daytime solar maximum conditions, Oyekola and Akin Ojo (2008) have examined interrelationship between equatorial ionospheric F2-region parameters.
The trends of foF2 are larger in the winter hemisphere than in the summer hemisphere, for both solar minimum and maximum conditions.
The overall model error, that is the mean square root deviation of the model from the data over the representative month ranging from about 6 8% (hmF2), ∼13 38% (foF2) and ∼8 29% (hmF2), ∼ 12 44% (foF2), respectively for low and high flux year, but approximately comparable at ∼3 7% for M3000F2 during solar minimum and maximum conditions.
While the device was unable to generate the minimum and maximum conditions as close as the single condition device as shown in figure 3, the device did successfully generate distinct oxygenation zones with a gradient of oxygen tension separating each zone.
The plasma frequency calculated by IRI from E region to bottomside of the F region present latitudinal discontinuities during morning and evening times for both solar minimum and solar maximum conditions.
Average F2 layer peak altitude measured at Ibadan during December solstice (November February), June solstice (May August) and equinoxes (March April, September–October) for quiet time and sunspot maximum conditions.
Fig. 4. Comparison between IRI model-predictions and experimental observations for the height of the ionospheric F2-peak, h m F2 at Ibadan for March (upper left plot), June (upper right plot), September (lower left plot), and December (lower right plot) during quiet time and sunspot maximum conditions.
Write better and faster with AI suggestions while staying true to your unique style.
Since I tried Ludwig back in 2017, I have been constantly using it in both editing and translation. Ever since, I suggest it to my translators at ProSciEditing.

Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com