A Nearly Universal Solar Wind-Magnetosphere Coupling Function. Newell 1, thomas sotirelis 1, kan. Web pdf | we investigated whether one or a few coupling functions can represent best the interaction between the solar wind and the magnetosphere.
We investigated whether one or a few coupling functions can represent best the interaction between the solar wind and the. Web solar wind (sw) quantities, referred to as coupling parameters (cps), are often used in statistical studies devoted to the analysis of. Web quantitatively estimating the energy input from the solar wind into the magnetosphere on a global scale is still an observational challenge.
Quantitatively Estimating The Energy Input From The Solar Wind Into The Magnetosphere On A Global Scale Is Still An Observational Challenge.
Web it is shown that all widely used coupling functions about the solar wind magnetosphere interaction can be derived as particular cases of general expressions. This picture opens a new pathway to. Web the control function is found to be successful, statistically as good as the best “solar wind driver function” in the literature.
Solar Wind‐Magnetosphere Coupling Functions Have Now Been In Use.
These have been used for almost 50 years now,. It is shown that in addition to the interplanetary electric field, the solar wind. We investigated whether one or a few coupling functions can represent best the interaction between the solar wind and the.
Newell 1, Thomas Sotirelis 1, Kan.
Journal of geophysical research 112: Web pdf | we investigated whether one or a few coupling functions can represent best the interaction between the solar wind and the magnetosphere. Web solar wind (sw) quantities, referred to as coupling parameters (cps), are often used in statistical studies devoted to the analysis of.
Web Solar Wind—Magnetosphere Coupling Functions:
Web quantitatively estimating the energy input from the solar wind into the magnetosphere on a global scale is still an observational challenge.