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ENERGY SHEETS. “Energy transfer is most efficient when the reconnection process takes place at the dayside magnetopause, which occurs during periods when the interplanetary field points southward and is thus antiparallel to the intrinsic geomagnetic field.” https://link.springer.com/article/10.12942/lrsp-2007-1 View in LinkedIn

ENERGY FLUX. “In a quiescent situation, energy inflow is gradual, the energy is dissipated in the ionosphere, and magnetic flux opened at the dayside reconnection process is closed by a quasistatic reconnection process in the distant magnetotail at about 100–200 RE from the Earth.” https://link.springer.com/article/10.12942/lrsp-2007-1 View in LinkedIn

ENERGY FLUX. “In a quiescent situation, energy inflow is gradual, the energy is dissipated in the ionosphere, and magnetic flux opened at the dayside reconnection process is closed by a quasistatic reconnection process in the distant magnetotail at about 100–200 RE from the Earth.” https://link.springer.com/article/10.12942/lrsp-2007-1 View in LinkedIn

VAST ENERGY SOUP. “Energy, momentum, and plasma enter the magnetosphere both via magnetic reconnection at the magnetospheric boundaries in regions where the interplanetary and terrestrial fields are antiparallel and via viscous interactions along the boundary.” https://link.springer.com/article/10.12942/lrsp-2007-1 View in LinkedIn