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Atmospheric and terrestrial turbulence.
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Taking the example of the plasma turbulence in the terrestrial magnetosheath, we show how the k-filtering technique constitutes the appropriate tool to make the best use of the 4-point measurements for this objective.
In the terrestrial case, various regions of the magnetosheath exhibit different properties of the waves and turbulence, depending on the position in relation to the bow shock and magnetopause.
Next, we give an overview of the concepts of waves, instabilities, chaos and turbulence in the planetary exoplanetary environment based on our present knowledge of the solar-terrestrial environment.
These include strong currents and/or wave activity that increase turbulence; the abundance of disease transmission vectors, including fish, divers and vessels; the distance from terrestrial sources of nutrient input; and the time period required to flush the surrounding waters.
Under the right conditions, this turbulence can also be associated with the presence of mesospheric thin layers (see "Solar-terrestrial effects on middle atmosphere chemistry").
The understanding of the wave activities and turbulence processes in the Venus magnetosheath will also enable us to predict the possible conditions in the terrestrial magnetosphere when the magnetic field is weak.
This turbulence.
There is turbulence ahead.
Some turbulence ahead indeed.
"That will create turbulence".
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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