The obtained results are an example of the capability of geomagnetic field fluctuations data to provide new insights about ionospheric dynamics and ionosphere magnetosphere coupling.
In conclusion, the obtained results are an example of the capability of geomagnetic field fluctuations data to generate new insights on the ionosphere magnetosphere coupling and, at the same time, to develop new applications using their changes in scaling features as a local indicator of the magnetosphere conditions.
In a subset of experiments, PCH analysis was also performed on the raw fluctuation data using Zen 2010, fitting to single component or two component PCH models [33] to obtain estimates of particle number (N) and brightness.
It is therefore very important to assimilate the GNSS-based fluctuation data into the existing theoretical model by means of new data calibration and to develop a new empirical or semi-empirical model based on GNSS TEC measurements of the ionospheric fluctuations and scintillation.
2dPCH was applied to the Ste11-GFP, Ste50-mCherry fluctuation data, and revealed the in vivo binding stoichiometry of the complexes (Figure 4).
The validity of the theory is confirmed experimentally by applying it to non-stationary road traffic noise level fluctuation data.
They used a free-falling Chameleon to collect pressure, potential temperature, conductivity, temperature gradient, horizontal velocity shears, and vertical velocity fluctuation data.
PCH could be used to evaluate molecular brightness (expressed as counts per second per molecule, cpsm) to estimate the stoichiometry (monomers, dimers, trimers, etc) [21], [22] of the diffusers from fluorescence fluctuation data.
The new analysis of the WMAP fluctuation data indicated that the universe is 13.73 billion years old with a precision of better than 1% and that the first stars formed only about 430 million years after the big bang.
Finally, right panel of Fig. 8 shows the results for the much smaller array of shot scale fluctuation data.
