Auroral Plasma Acceleration Above Martian Magnetic Anomalies
Coates, A. J.; Kallio, E.; Fedorov, A.; Koskinen, H.; Barabash, S.; Lundin, R.; Holmström, M.; Yamauchi, M.; Sauvaud, J. -A.; Sharber, J. R.; Kozyra, J.; Hsieh, K. C.; Grande, M.; Orsini, S.; Wurz, P.; Woch, J.; Asamura, K.; Winningham, D.; Frahm, R.; Nilsson, H.; Luhmann, J.; Fraenz, M.; Hayakawa, H.; Curtis, C.; Brain, D.; Brandt, P.; Mckenna-Lawler, S.; Soobiah, Y.
Sweden, United States, France, Japan, United Kingdom, Finland, Germany, Ireland, Italy, Switzerland
Abstract
Aurora is caused by the precipitation of energetic particles into a planetary atmosphere, the light intensity being roughly proportional to the precipitating particle energy flux. From auroral research in the terrestrial magnetosphere it is known that bright auroral displays, discrete aurora, result from an enhanced energy deposition caused by downward accelerated electrons. The process is commonly referred to as the auroral acceleration process. Discrete aurora is the visual manifestation of the structuring inherent in a highly magnetized plasma. A strong magnetic field limits the transverse (to the magnetic field) mobility of charged particles, effectively guiding the particle energy flux along magnetic field lines.