Abstract
Abstract. Sporadic E layers form in the daytime midlatitude ionosphere as a
result of wind shears in the mesosphere–lower-thermosphere compressing
metallic ions of meteoric origin into dense, narrow sheets extending over
hundreds or thousands of kilometers spatially. These layers are poorly
observed, being too narrow to be properly resolved by incoherent scatter
radar or path-integrated total electron content measurements. Sporadic E
layer peak densities can be resolved by ionosondes and by rocket-borne
Langmuir probes, but these techniques have major limitations in terms of
spatial and temporal coverage, and (for many ionosondes) maximum density
resolution. As a result, the density, occurrence, and spatial extent of
sporadic E layers are not well constrained by observations. The maximum
density of sporadic E is widely believed to be around 5–10×1011 electrons m−3 NmEs (equivalent to 6–9 MHz foEs), though
there are a few isolated reports of layers extending beyond 20 MHz (Chandra
and Rastogi, 1975; Maeda and Heki, 2014). Here, we identify sporadic E
layers using a huge database of 29 million 162 MHz automatic identification system (AIS) shipping transmissions collected over 3 d by a United
States Coast Guard (USCG) terrestrial monitoring network in the eastern
United States and Puerto Rico. Within this dataset, most (>99 %) links are explained by line-of-sight, surface-wave, and tropospheric
propagation, but a small population cannot be explained by these mechanisms.
In total, 6677 signals were identified from ships located over 1000 km from
the ground stations between 13 and 14 July 2021, and almost no long-distance
links were received at night or at any time on 15 July. This coincides with
intense (saturated) sporadic E in collocated ionosondes and in satellite
radio occultation data. The density of these layers might exceed 27 MHz
foEs or 9×1012 electrons m−3 NmEs. AIS transmissions
potentially provide an excellent means of identifying dense sporadic E
layers globally.
Funder
National Aeronautics and Space Administration
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