GEOTAIL observations of flow velocity and north-south magnetic field variations in the near and mid-distant tail associated with substorm onsets

• Published in: Geophysical research letters Vol. 26; no. 6; pp. 635 - 638
• Main Authors: Machida, S., Miyashita, Y., Ieda, A., Nishida, A., Mukai, T., Saito, Y., Kokubun, S.
• Format: Journal Article
• Language: English
• Published: Washington, DC Blackwell Publishing Ltd 15.03.1999; American Geophysical Union
• Subjects: Atmospheric movements; Earth, ocean, space; Exact sciences and technology; External geophysics; Geomagnetism; Magnetic fields; Physics of the magnetosphere; Plasma flow; Plasma motion, convection, circulation. Plasma instabilities; Plasma flow; Pi 2 micropulsation; Magnetospheric substorm; Plasmoid; Satellite observation; Magnetospheric tail; Flow velocity; Magnetic field
• ISSN: 0094-8276; 1944-8007
• DOI: 10.1029/1999GL900030

Temporal changes in the plasma flow and magnetic fields of the Earth's magnetotail in the region of −7.5 > X(RE) > −52.5 and −15 < Y(RE) < 15 in the GSM coordinates were studied by applying a superposed epoch analysis method to 263 substorm events observed by GEOTAIL spacecraft. The onset times of the substorms were determined with Pi‐2 pulsations at Kakioka station. It was found that the tailward flow associated with plasmoids started about 2 or 3 min before the Pi‐2 onsets, and the earthward flow became somewhat coherent 1 min before the onsets. The variation of the northward magnetic field component was investigated by obtaining the deviation of this component from that in the interval from 10.5 to 7.5 min before the Pi‐2 onsets. We found that the northward magnetic field increased at X ∼ −10RE and decreased at X ∼ −28RE simultaneously in the premidnight tail immediately after the onsets. These variations definetely correspond to the dipolarization and plasmoid formation, respectively.