scholarly journals Indices of equatorial electrojet and counter-electrojet in the Indian region: Evolution of the indices and their authenticity

1983 ◽  
Vol 92 (1) ◽  
pp. 45-55
Author(s):  
B N Bhargava ◽  
B R Arora ◽  
N S Sastri
1979 ◽  
Vol 31 (3) ◽  
pp. 311-340 ◽  
Author(s):  
R. T. MARRIOTT ◽  
A. D. RICHMOND ◽  
S. V. VENKATESWARAN

1994 ◽  
Vol 56 (1) ◽  
pp. 51-58 ◽  
Author(s):  
V.V. Somayajulu ◽  
K.S. Viswanathan ◽  
K.S.V. Subbarao ◽  
L. Cherian

2017 ◽  
Vol 35 (3) ◽  
pp. 535-545 ◽  
Author(s):  
A. Babatunde Rabiu ◽  
Olanike Olufunmilayo Folarin ◽  
Teiji Uozumi ◽  
Nurul Shazana Abdul Hamid ◽  
Akimasa Yoshikawa

Abstract. We examined the longitudinal variability of the equatorial electrojet (EEJ) and the occurrence of its counter electrojet (CEJ) using the available records of the horizontal component H of the geomagnetic field simultaneously recorded in the year 2009 (mean annual sunspot number Rz  =  3.1) along the magnetic equator in the South American, African, and Philippine sectors. Our results indicate that the EEJ undergoes variability from one longitudinal representative station to another, with the strongest EEJ of about 192.5 nT at the South American axis at Huancayo and a minimum peak of 40.7 nT at Ilorin in western Africa. Obtained longitudinal inequality in the EEJ was explicable in terms of the effects of local winds, dynamics of migratory tides, propagating diurnal tide, and meridional winds. The African stations of Ilorin and Addis Ababa registered the greatest % of CEJ occurrence. Huancayo in South America, with the strongest electrojet strength, was found to have the least occurrence of the CEJ. It is suggested that activities that support strong EEJ inhibits the occurrence of the CEJ. Percentage of occurrence of the CEJ varied with seasons across the longitudes. The order of seasonal variation of morning occurrence does not tally with the evening occurrence order at any station. A semiannual equinoctial maximum in percentage of morning occurrence of the CEJ was obtained at Huancayo and Addis Ababa. Only Addis Ababa recorded equal equinoctial maxima in percentage of evening occurrence of the CEJ. The seasonal distribution of the occurrences of the CEJ at different time regimes implies a seasonal variability of causative mechanisms responsible for the occurrence of the CEJ.


2018 ◽  
Vol 123 (8) ◽  
pp. 6821-6835 ◽  
Author(s):  
R. K. Archana ◽  
N. Phani Chandrasekhar ◽  
Kusumita Arora ◽  
Nandini Nagarajan

2019 ◽  
Vol 13 (3) ◽  
pp. 245-255
Author(s):  
Prashanthi Talari ◽  
Sampad Kumar Panda

Abstract The present paper investigates the alterations in ionospheric Total Electron Content (TEC) over a low latitude location Bangalore (Geographic latitude {12.9^{\circ }}\hspace{2.38387pt}\text{N} and longitude {77.6^{\circ }}\hspace{2.38387pt}\text{E}; Geomagnetic latitude 4.{5^{\circ }}\hspace{2.38387pt}\text{N}) in India, corresponding to the new Moon and full Moon days which are associated with abnormality in the eastward Equatorial Electrojet (EEJ) currents. It has been well established that even during certain geomagnetic quiet days, the EEJ current direction is reversed, resulting in a westward electrojet current called Counter Electrojet (CEJ) which is more prominent around the new Moon and full Moon days, favored by Sun–Moon–Earth alignments and lunar orbital characteristics. The Global Positioning System (GPS) derived TEC at Bangalore is investigated for full Moon and new Moon and their adjacent days during the period 2008–2015. The presence of CEJ during these days suggests the foremost role of driving EEJ current over the equator in the alterations of spatiotemporal distributions of TEC over the low latitude region. The deviations in quiet time TEC during new Moon and full Moon days are quantified in this study that may give a thrust towards modeling of lunar tidal effects in the flipped ionospheric parameter over the Indian region. The study would also support analysis of future solar eclipse effects on ionosphere those involve additional photoionization production/recombination processes corresponding to the passage of lunar shadow and cooling effects. Moreover, the results underpin modeling and mitigation of ionospheric error in the satellite-based positioning, navigation, and communication applications.


1983 ◽  
Vol 88 (A1) ◽  
pp. 253 ◽  
Author(s):  
Christian Hanuise ◽  
Christine Mazaudier ◽  
Paul Vila ◽  
Michel Blanc ◽  
Michel Crochet

2016 ◽  
Vol 125 (3) ◽  
pp. 669-675 ◽  
Author(s):  
H CHANDRA ◽  
R G RASTOGI ◽  
R K CHOUDHARY ◽  
SOM SHARMA

2017 ◽  
Vol 122 (2) ◽  
pp. 2185-2201 ◽  
Author(s):  
N. Phani Chandrasekhar ◽  
R. K. Archana ◽  
Nandini Nagarajan ◽  
Kusumita Arora

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