Open AccessGeomagnetic secular variation and secular acceleration in the Red Sea area
Author(s) -
Hall Stuart A.
Publication year - 1979
Publication title -
geophysical journal of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.302
H-Index - 168
eISSN - 1365-246X
pISSN - 0016-8009
DOI - 10.1111/j.1365-246x.1979.tb04795.x
Subject(s) - secular variation , earth's magnetic field , latitude , geomagnetic secular variation , geodesy , variation (astronomy) , geology , secular education , geomagnetic latitude , climatology , geomagnetic storm , geophysics , physics , magnetic field , astrophysics , law , quantum mechanics , political science
Summary. Estimates of the secular variation in the Red Sea over the period 1959 to 1972 have been obtained from an analysis of marine magnetic data. A total of 318 crossings of ships' tracks were used to determine the mean secular variation for the intervals 1959–72, 1959–65 and 1965–72. The mean secular variation 1959–72 shows a marked northward increase from approximately ‐10 nT/yr at 13°N to +27 nT/yr at 24°N. North of this, the data suggest a small decrease to + 25 nT/yr at 27° N. These values are consistent with the secular variation recorded at the nearby geomagnetic observatory at Helwan, Egypt, but less than those predicted by the 1965 IGRF for the same period. Comparison of the mean secular variations for 1959–65 and 1965–72 yields a rough estimate of the secular acceleration of ‐ 1.5 nT yr −2 . Analysis of the cross‐over information, corrected for the latitude dependence of the secular variation, shows a regular decrease in the secular change over the period 1959–72 at all latitudes of about ‐1 nTyr −2 . This secular acceleration makes a substantial contribution to the overall secular change in the Red Sea and as such must be included in the correction of magnetic data covering more than a few years.