Nocturnal variations of geomagnetic horizontal field at equatorial stations

The nocturnal variations of the horizontal component (H) of the geomagnetic field at equatorial stations Koror, Trivandrum, Addis-Ababa and Ibadan during any of the seasons of the period 1958-59 showed a steady decrease after sunset throughout the nighttime hours. However, at Huancayo a steady decrease after sunset to sunrise is seen only during the D-months. During the J and E months decrease is seen after sunset till about 22-23 hr and a slow and steady increase from midnight hours to sunrise. The nocturnal variations of H field at Huancayo show a remarkable similarity with the corresponding variations of the horizontal electric field in the ionosphere as determined by the Doppler shifts of backscatter echoes from the E and F layers over Jicamarca. Thus, genuine changes in the equatorial electric field and current in the ionosphere over the American sector during the nighttime hours are clearly indicated.

[1]  W. P. Olson The contribution of magnetospheric currents toSq , 1989 .

[2]  R. Stening,et al.  Night-time geomagnetic variations at low latitudes , 1987 .

[3]  T. Araki,et al.  Simulation of ionospheric currents and geomagnetic field variations of Sq for different solar activity , 1986 .

[4]  T. Araki,et al.  Electric conductivity of the ionosphere and nocturnal currents , 1985 .

[5]  S. Prakash,et al.  E and F region electric fields over dip equator , 1981 .

[6]  S. Malin,et al.  The Sq current system during the International Geophysical Year , 1977 .

[7]  J. D. Tarpley The ionospheric wind dynamo - I. Lunar tide , 1970 .

[8]  M. Schield Correction to paper by Milo A. Schield, ‘Pressure balance between solar wind and magnetosphere’ , 1969 .

[9]  M. Schield Pressure balance between solar wind and magnetosphere , 1969 .

[10]  D. Fairfield Average magnetic field configuration of the outer magnetosphere. , 1968 .

[11]  A. J. Chen,et al.  Plasma flow in the magnetosphere. , 1968 .

[12]  Donald J. Williams,et al.  Nightside magnetosphere configuration as obtained from trapped electrons at 1100 kilometers. , 1965 .

[13]  Sadami Matsushita,et al.  On the Geomagnetic Solar Quiet Daily Variation Field , 1965 .

[14]  G. Mead DEFORMATION OF THE GEOMAGNETIC FIELD BY THE SOLAR WIND , 1964 .

[15]  A. T. Price,et al.  New methods for the analysis of geomagnetic fields and their application to the sq field of 1932-3 , 1963, Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences.

[16]  W. D. Parkinson An analysis of the geomagnetic diurnal variation during the International Geophysical Year , 1977 .

[17]  K. Iyer,et al.  Quiet day variation of geomagnetic H-field at low latitudes. , 1976 .

[18]  K. N. Nair,et al.  Morphology of the geomagnetic field variations and a study of the interplanetary magnetic field fluctuations in relation to the daily variation of the geomagnetic field at low latitudes. , 1971 .

[19]  B. Balsley,et al.  Ionospheric drift velocity measurements at Jicamarca, Peru (July 1967-March 1970) , 1971 .

[20]  S. Chapman I. The solar and lunar diurnal variations of terrestrial magnetism , 1919 .