Exact(2)
To estimate the EPB in life-cycle, the approach presented in Section 2 is available to obtain the ECC in establishing a new OTL.
Illustration of the different processing steps for EPB detection: (a) residual strength, (b) filtered residual strength, (c) filtered/rectified residual strength, (d) plasma density, (e) filtered plasma density, (f) Bubble Index and Bubble Probability, and (g) scatter plot of filtered residual strength and filtered plasma density for the widest EPB in panel (f).
Similar(58)
Furthermore, studies of day-to-day variability in EPB activity, in which the connection between EPBs and the lower atmosphere should be considered, are few.
The occurrence period of EPBs in TEC and OI 630.0 nm has found to be different.
Numerical modeling efforts to understand ESF and EPBs in the past 40 years were reviewed in this article.
An interesting approach is to resolve EPBs in a global ionospheric model.
Furthermore, the growth of EPBs in the models strongly depends on how initial seeding perturbations are added.
We will return to the difference between west-wall echoes and EPBs in 'Onset phase: ESF patches and primary EPBs' and 'Structure phase: clustering and EW asymmetry' sections.
We observed EPBs in images regularly during a limited period 19 30 to 02 30 LT and reach maximum probability of occurrence at 22 30 LT.
For that reason it may be useful to identify EPBs from in-situ magnetic observations and de-select EPBs in geomagnetic field modeling efforts, as has been done by Maus et al. (2007).
To explain the appearance of ESF in patches (and EPBs in clusters), some form of seeding must be assumed without understanding the causal physics.
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