Tsurutani, B.T.; Dasgupta, B.; Galvan, C.; Neugebauer, M.; Lakhina, G.S.; Arballo, J.K.; Winterhalter, D.; Goldstein, B.E.; Buti, B.
(2002)
[1] Solar wind protons detected within Magnetic Holes (MHs) and Magnetic Decreases (MDs) are found to be preferentially heated perpendicular to equation image0. The MHs/MDs are associated with the phase-steepened edges of ...