Ionospheric trough

From Glossary of Meteorology



ionospheric trough

A portion of the F-region, centered on the magnetic dip equator, in which electron densities are anomalously low with peaks at 15°–20° latitude on both sides.

The equatorial trough appears during daytime and is absent at night. It is attributed to diffusion of ionospheric plasma down the magnetic field lines from the magnetic equator as the F-region rises in response to an eastward electric field generated by dynamo action in the lower ionosphere. One or more troughs in electron density are also found at high latitudes and are magnetically linked to the plasmapause located at a radial distance of several earth radii in the outer magnetosphere.


Copyright 2024 American Meteorological Society (AMS). For permission to reuse any portion of this work, please contact permissions@ametsoc.org. Any use of material in this work that is determined to be “fair use” under Section 107 of the U.S. Copyright Act (17 U.S. Code § 107) or that satisfies the conditions specified in Section 108 of the U.S.Copyright Act (17 USC § 108) does not require AMS’s permission. Republication, systematic reproduction, posting in electronic form, such as on a website or in a searchable database, or other uses of this material, except as exempted by the above statement, require written permission or a license from AMS. Additional details are provided in the AMS Copyright Policy statement.