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With the advance of observational techniques and the expansion of the field of view of the existing observation network, as well as the development of modeling/numerical simulation algorithms, we hope to enhance the understanding of the ionosphere, ranging from the high to mid/low latitude, and its relation to the dynamics of the geospace and upper atmosphere.
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The fact that higher transmittances are related to lower sheet resistances is in line with the existing observations.
We were not able to discriminate between these two mechanisms based on the existing observations.
This evaluation and the OE's observations and evaluations of the individual CREATE implementations (outlined below) were compiled by the OE in a 127-page final report and provided to the PIs (Hurley, 2009) For evaluation of CREATE faculty implementers on individual campuses, the OE modified two existing observation protocols to adapt them specifically for the CREATE classroom.
When compared to existing observation data, the global-mean OLR in the simulations is around 240 250 W m−2, which is relatively larger than the observed OLR at around 235 W m−2, [obtained from daily-mean-interpolated OLR data from the National Oceanic and Atmospheric Association satellite (Liebmann and Smith 1996)].
They are also small enough to elude routine detection by existing observation systems.
Furthermore, existing observation networks have poor coverage in some regions (for example, over large bodies of water such as the Pacific Ocean), which introduces uncertainty into the true initial state of the atmosphere.
Furthermore, existing observation networks have limited spatial and temporal resolution (for example, over large bodies of water such as the Pacific Ocean), which introduces uncertainty into the true initial state of the atmosphere.
"But given the existing observations, there is a lambda".
The combined effect of these two factors is that the hypotheses whose 2D projections best fit to the existing observations obtain higher likelihood values, taking into account both that the area of the intersection is large, and that the boxes are aligned in the two dimensions of the plane.
The existing observations and simulations show that the physical mechanisms for the WSA and northern MSNA formation could be attributed to the equatorward neutral wind, E × B drift, photoionization, and downward diffusion from the plasmasphere (Burns et al. 2008; Lin et al. 2009, 2010; Liu et al. 2010; de Larquier et al. 2011; Chen et al. 2011).
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com