“High-latitude plasma convection from Cluster EDI: variances and solar wind correlations”
“The magnitude of convection standard deviations is of the same order as, or even larger than, the convection magnitude itself. Positive correlations of polar cap activity are found with |ByzIMF| and with Er,sw, in particular. The strict linear increase for small magnitudes of Er,sw starts to deviate toward a flattened increase above about 2 mV/m. There is also a weak positive correlation with Pdyn. At very small values of Pdyn, a secondary maximum appears, which is even more pronounced for the correlation with solar wind proton density. Evidence for enhanced nightside convection during high nightside activity is presented.”
“The magnitude of convection standard deviations is of the same order as, or even larger than, the convection magnitude itself. Positive correlations of polar cap activity are found with |ByzIMF| and with Er,sw, in particular. The strict linear increase for small magnitudes of Er,sw starts to deviate toward a flattened increase above about 2 mV/m. There is also a weak positive correlation with Pdyn. At very small values of Pdyn, a secondary maximum appears, which is even more pronounced for the correlation with solar wind proton density. Evidence for enhanced nightside convection during high nightside activity is presented.”
‘Low to Moderate values in the solar wind electric field are positively correlated to convection velocity.”
“A positive correlation between Ring current and convection velocity.”
http://web.ift.uib.no/Romfysikk/RESEARCH/PAPERS/forster07.pdf
“A positive correlation between Ring current and convection velocity.”
http://web.ift.uib.no/Romfysikk/RESEARCH/PAPERS/forster07.pdf
Low Energy ion escape from terrestrial Polar Regions.
http://www.dissertations.se/dissertation/3278324ef7/
http://www.dissertations.se/dissertation/3278324ef7/
No comments:
Post a Comment