E and F region electric fields over dip equator
Author(s) -
Prakash S.,
Muralikrishna P.
Publication year - 1981
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/ja086ia04p02095
Subject(s) - electric field , equatorial electrojet , drift velocity , midnight , magnetic dip , equator , physics , latitude , ionosphere , f region , electrojet , sunset , geology , declination , field (mathematics) , electron , geodesy , geophysics , magnetic field , astrophysics , earth's magnetic field , optics , astronomy , quantum mechanics , mathematics , pure mathematics
The horizontal east‐west drift velocity V E of ionisation irregularities in E region, and the vertical drift velocity V F of electrons in F region over Jicamarca (dip latitude ≃1°) are used to estimate the average diurnal variation of the east‐west components of the electric fields in these two regions. The F region field is estimated from V F by using the relationship derived earlier by Woodman. The E region field is estimated from V E by using a relationship different from the one used earlier by Balsley and Woodman and is derived by using more realistic electrojet and conductivity models. The E region electric field thus obtained is found to be weaker at least by a factor of 3 than that estimated by Balsley and Woodman. A comparative study shows that the east‐west electric field in the F region is, most of the time, stronger than that in the E region, and also that the ratio of the E region field to the F region field systematically increases from forenoon to afternoon hours, and from pre‐midnight to post‐midnight hours.
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom