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- W2046616488 abstract "ISEE 1 magnetic field data for 1978‐1987 are examined to obtain the average distribution of the magnetotail current in the region . The whole data set is divided into three subsets according to different geomagnetic conditions, that is, AL −50 nT, −200 AL −50 nT, and AL −200 nT. Magnetic field values are averaged in each cell with a volume of 1 × 1 × 1 R E 3 , and the corresponding current densities are calculated from the average tail field. The radial distribution of the neutral sheet current for disturbed periods is characterized by intense currents near geostationary altitudes. In the midnight sector, it reaches as large as 140 mA/m, twice that for quiet periods. It is found that the neutral sheet current is maximized in the region −3 Y 6 R E , exhibiting clear dawn‐dusk asymmetry. There is no evident indication for the current disruption in the near‐Earth magnetotail, except for a 20 mA/m depression in the current intensity for disturbed periods near the midnight meridian within X −7 R E . Currents parallel to the average magnetic field are also derived. They are regarded as the average field‐aligned currents (FACs) in this paper. It is shown that irrespective of variable geomagnetic activity, large‐scale FACs are distributed in the conventional pattern, that is, region 1 and region 2 currents. The total intensity of FACs in the 2100‐0300 MLT sector is found to increase rapidly with increasing X in the region X −15 R E . This implies that the main source of FACs in the midnight sector is located in the near‐Earth magnetotail. A new model of the magnetotail current system for disturbed periods is proposed on the basis of our findings." @default.
- W2046616488 created "2016-06-24" @default.
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- W2046616488 date "1997-05-01" @default.
- W2046616488 modified "2023-10-14" @default.
- W2046616488 title "Statistical nature of the magnetotail current in the near-Earth region" @default.
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- W2046616488 doi "https://doi.org/10.1029/97ja00136" @default.
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