1992
DOI: 10.1111/j.1365-246x.1992.tb04644.x
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A study of rocket measurements of ionospheric currents-III. Ionospheric currents at the magnetic dip equator

Abstract: The 31 daytime rocket flight results within 0" or 2" dip latitude provide a good study of several issues leading to the following findings. In this zone, 60 per cent or more of ionospheric current systems have two layers. The lower layer has a peak density of 7 f 4 A k m -' at an altitude of 1 0 6 f 2 k m , a half thickness at half peak of 5.7 f 0.7 km and an altitude extent of 34 f 9 km. The upper layer has a peak density of about 1 A km-' at an altitude of 136 f 8 km and an altitude extent of 19 f 5 km. In s… Show more

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Cited by 11 publications
(7 citation statements)
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“…The altitude of the peak current density of the upper current layer decreases with latitude from about 136 ± 8 km at the dip equator to about 120 km outside the EEJ zone. From their characteristics, the lower current layer is associated with the EEJ and the upper current layer is associated with the W Sq (Onwumechili 1992a,b). The W Sq is mainly a Pedersen current driven by the zonal component E y of the global Sq dynamo polarization electric field E .…”
Section: Discussionmentioning
confidence: 99%
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“…The altitude of the peak current density of the upper current layer decreases with latitude from about 136 ± 8 km at the dip equator to about 120 km outside the EEJ zone. From their characteristics, the lower current layer is associated with the EEJ and the upper current layer is associated with the W Sq (Onwumechili 1992a,b). The W Sq is mainly a Pedersen current driven by the zonal component E y of the global Sq dynamo polarization electric field E .…”
Section: Discussionmentioning
confidence: 99%
“…where SV stands for the sequential variability (Onwumechili 1992a), C stands for D, H and Z and c stands for d, h and z . Only consecutive days are used in obtaining the differences in eq.…”
Section: Datamentioning
confidence: 99%
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“…Also, the ground magnetic perturbations which are induced by the EEJ in the equatorial region have been observed regularly at several magnetic observatories since the 1920s [e.g., Bartels and Johnston, 1940;Egedal, 1947;Doumouya et al, 1998;Rastogi et al, 2004;Manoj et al, 2006]. In situ rocket measurements and ground and satellite-borne magnetometers have provided extensive information about the structure and characteristics of the EEJ [e.g., Onwumechili, 1992;Jadhav et al, 2002;Lühr et al, 2004;Lühr and Maus, 2006]. In addition, theoretical and empirical models have been built not only to examine physical features and to understand large-scale spatial variation in the EEJ, but to reveal its relations with other ionospheric phenomena [e.g., Richmond, 1973;Doumouya et al, 2003;Klimenko et al, 2007;Alken and Maus, 2007].…”
Section: Introductionmentioning
confidence: 99%