Dayside field‐aligned current source regions

Abstract

[1] The source regions of region-0 (R0), region-1 (R1), and region-2 (R2) field-aligned currents (FACs) were statistically determined using DMSP particle precipitation and magnetometer data. Each FAC sheet originates from more than one region in the magnetosphere, depending on the latitude and the magnetic local time (MLT). R2 originates mostly from the central plasma sheet (CPS) and boundary plasma sheet (BPS) in the morning and from the CPS, BPS, and inner magnetosphere in the afternoon, all of which are on closed field lines. Near noon, some R2 may originate from the low-latitude boundary layer (LLBL), which is located near the magnetopause and can be open or closed. R1 mostly maps to the BPS, hence on closed field lines, in morning and afternoon, but near noon, it maps mostly to the LLBL. The LLBL source region can be found more frequently in the dawn-noon sector than in the noon-dusk sector. On the other hand, R0 is located mostly on open field lines and is associated mostly with mantle precipitation. However, the mantle precipitation has a dependency on the polarity of R0. Within up-flowing R0, sometimes an upward field-aligned electric field, which accelerates electron downward and retards ion precipitation, modifies mantle distribution to look more like those of polar rain or BPS. This electric field has the opposite polarity to the background electric field that maintains charge-quasi-neutrality and that limits some solar wind electrons from entering the magnetosphere in the mantle and polar rain regions. Implications to current generation mechanisms are discussed.

Double cusp encounter by Cluster: double cusp or motion of the cusp?

“…The IMF B z would move the cusp in the north-south direction (e.g. Carbary and Meng, 1986;Escoubet and Bosqued, 1989;Woch and Lundin, 1992;Newell and Meng, 1994;Sandholt et al, 1994;Zhou et al, 2000;Wing et al, 2001;Pitout et al, 2006a, b), while the IMF-B y would move the cusp in the east-west direction (e.g. Candidi et al, 1983;Crooker et al, 1987;Newell et al, 1989).…”

On the field‐aligned electric field in the polar cap

“…In fact, the ions look similar to those in the adjacent polar rain region. Taken together, the present study and Wing et al [2010] suggest that the Newell et al [1991aNewell et al [ , 1991bNewell et al [ , 1991c algorithm needs to be modified by taking into account FAC observations.…”

“…Thus, taking the upward electric field into account, we would have the expected pattern from low to high latitude as closed-open field lines. (This correction should also apply to the examples presented in Figures 1a, 1b, and 7 in Wing et al [2010].) Moreover, in the electron acceleration region, there is no significant ion precipitation.…”

“…Such structures are typically found slightly poleward of the dayside open-closed boundary. Two examples are presented (more examples can be found in Wing et al [2010]). Unfortunately, solar wind data are not available for these two events.…”

“…sheet [e.g., Iijima and Potemra, 1976;Wing et al, 2010]. The poleward boundary of the auroral oval is located at about magnetic latitude (MLAT)~À73.2°(18:30:12 UT).…”