Long-distance propagation of 162 MHz shipping information links associated with sporadic E
- 1Space Exploration Sector, Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, United States of America
- 2Air Force Institute of Technology, Wright-Patterson AFB, OH 45433, United States of America
Correspondence: Alex T. Chartier (firstname.lastname@example.org)
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.
Automatic identification system (AIS) transponders are designed to provide vessel position, identification, and other information to other ships and to coastal authorities (e.g., International Maritime Organization, 2022). The system operates using very high-frequency (VHF) radio transmissions on two 25 kHz channels close to 162 MHz. AIS is required to be used on large ships, typically at the 12.5 W level. Many smaller vessels, including recreational boats, are also fitted with low-power (∼2 W) or passive AIS systems. The United States Coast Guard (USCG) operates a network of land-based AIS monitors and provided 3 d of data from stations in the eastern USA and Puerto Rico for this study (13–15 July 2021) along with satellite-received data used as an independent point of reference. The exact station locations are not disclosed by request of the data provider. Occasionally, signals are identified at long distances of 1000 km or more. This long-distance propagation is surprising since signals at 162 MHz would typically be expected to pass through the ionosphere to space rather than reflecting off and back to Earth as skywaves. VHF signals do propagate over the horizon as surface waves and through tropospheric ducting (Ames et al., 1955), but the distances are typically limited to a few hundred kilometers or less. We note that very long-distance propagation of VHF signals has been reported in amateur radio databases. For example, the “More Miles on VHF” database reports many long-distance links and attributes them to several different propagation modes, including both sporadic E and tropospheric ducting.
This study evaluates the possibility that extremely dense, low-altitude ionospheric layers (known as sporadic E) could provide a skywave propagation path that would explain the long-range USCG AIS observations. Sporadic E layers were first identified using ionosondes (e.g., Thomas and Smith, 1959). These layers are known to occur frequently, especially at midlatitudes during the daytime in summer (Wu et al., 2005; Chu et al., 2014; Arras and Wickert, 2018), with the cause believed to be a redistribution of existing plasma into thin, dense layers by wind shears (see reviews by Whitehead, 1970; Mathews, 1998; Haldoupis, 2011, for more details). The process may be aided by the presence of long-lived metallic ions deposited in the lower ionosphere by meteors (e.g., Maruyama et al., 2008). Recently, Yamazaki et al. (2022) presented convincing evidence linking sporadic E to zonal wind shears using ICON/MIGHTI interferometer wind profile data and COSMIC-2/RO retrieved electron density profiles. Deacon et al. (2022) have linked sporadic E to long-distance amateur radio propagation reports on frequencies up to 70 MHz, while amateur groups themselves routinely map sporadic E (e.g., Sampol, 2022). There are some observations of extremely high sporadic E critical frequency (foEs); for example Chandra and Rastogi (1975), Maeda and Heki (2014), and Shinagawa et al. (2021) observed and modeled foEs>20 MHz. However the phenomenon remains unpredictable, and its occurrence, intensity, and spatial extent are not well constrained observationally, in particular over the oceans.
The USCG AIS link dataset produced by stations in the eastern USA contains almost 29 million links over 3 d. Most of the received data (>99 %) are from ships within 300 km great-circle distance of the USCG stations. The data were processed taking care to remove any repeated signals as well as AIS signals emitted from search and rescue aircraft. A histogram of observed AIS link distances is shown in Fig. 1.
The ranges between a few hundred kilometers and ∼1000 km are likely caused by tropospheric refraction phenomena (e.g., ducting) and occur beyond the normal line of sight but are typically confined to paths within a few hundred kilometers of the coastline. As can be seen, there is a distinct population of links observed above around 1000 km great-circle distance, extending up to a maximum of 5453 km (6692 links >1000 km in total). A time series of these links is shown in Fig. 2, with a representative day–night boundary for Bar Harbor, ME, included for reference.
Almost all (6677) of the long-distance AIS links were detected on 13 and 14 July, with almost none seen at night or on 15 July. The maximum number of long-range links in a 15 min window was 655, between 18:45–19:00 UT on 14 July, and the second highest number was 421, between 14:15–14:30 UT on 13 July. Snapshots of these intervals are shown in Fig. 3.
These snapshots indicate the long-distance AIS propagation is related to a spatially confined phenomenon, intermittently present over an area of hundreds or thousands of kilometers during daytime hours.
Tropospheric ducting is estimated using meteorological reanalysis temperature, pressure, and humidity data. Here we computed ducting using the European Centre for Medium-Range Weather Forecasts (ECMWF) 5th Generation Reanalysis (ERA5) described by Hersbach et al. (2018). These data were processed to compute the maximum strength of all radio frequency (RF)/tropospheric ducts that appear at a single grid point and time. The maps of modified refractivity were derived from hourly forecast data using the full-resolution 137 level temperature and specific humidity data provided on a regular Gaussian grid, at hourly resolution. Ducting maps at 19:00 UT on 14 July and 14:00 UT on 13 July are shown in Fig. 4.
By showing the tropospheric ducting strength overlaid with the received position reports from land-based AIS receivers, one can see the correlations near shore of the tropospheric ducting that helps to extend the RF propagation range. It is also apparent that tropospheric ducting could not be responsible for the very long-range AIS receptions that are the main focus of this publication. To illustrate this, a time series of the median nonzero tropospheric duct strength is shown in Fig. 5.
As can be seen in Fig. 5, tropospheric ducting peaks on 15 July 2021, when almost no long-distance AIS links were observed. Therefore a different explanation is needed for the >1000 km propagation observed on 162 MHz that were shown in Fig. 2.
Data from ground-based Digisondes and from Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC-2) radio occultations are used to identify the cause of the observed long-distance AIS links. Figure 6 shows Digisonde peak sporadic E plasma frequency (foEs) from Millstone Hill, MA; Wallops Island, VA; and Ramey, Puerto Rico.
The Digisonde foEs values saturate (i.e., they reach the maximum observable value of 10 MHz at Millstone and Wallops or 6.5 MHz at Ramey) during the daytime at Wallops and Ramey on 13 July and at Wallops and Millstone on 14 July. The data do not saturate at any station either at night or at any time on 15 July. This is consistent with the trend seen in the long-distance AIS link data.
Spatial maps of sporadic E are produced by combining COSMIC-2 RO data with Digisonde measurements, using the S4-based approach described by Yu et al. (2020). These maps are produced at 3 h cadence to increase the number of local observations in the region. Maps corresponding to the two maximum AIS link times are shown in Fig. 7.
Given the spatial and temporal limitations of the data coverage, the sporadic E maps show remarkably good agreement with the AIS long-distance link data shown in Fig. 3. While the COSMIC-2 RO data are useful in identifying the presence or absence of sporadic E (Carmona et al., 2022), predicting foEs magnitudes from RO data is more difficult (Gooch et al., 2020). This is especially true of strong sporadic E layers that tend to saturate the S4 amplitude scintillation (Stambovsky et al., 2021; Yu et al., 2020). Therefore, we have higher confidence in the foEs estimates near Digisondes than in the locations driven strictly by RO data.
The analysis indicates that long-distance 162 MHz AIS links observed in the western Atlantic region on 13 and 14 July 2021 are associated with sporadic E layers. This is remarkable given that signals at such high frequency are typically expected to pass through the ionosphere. The available vertical-incidence ionosonde data in the region saturate at or below 10 MHz, so it is not possible to determine the true value of foEs during these periods.
If we assume a layer height of 100 km and take the shortest AIS paths within the anomalous distribution at around 1200 km (see Fig. 1), we can estimate an angle of incidence ∼9.5∘ (neglecting refraction and curvature). In this case the secant law (see Han, 1970, for details) implies MHz or 9×1012 electrons m−3. This is almost an order of magnitude larger than is typically expected, though there have been observations of foEs>20 MHz (Chandra and Rastogi, 1975; Maeda and Heki, 2014).
There are several challenges inherent in using AIS data to identify long-distance propagation. In some cases the system is subject to spoofing, either of the signals themselves or the GNSS signals they rely upon. There are also occasional transmission errors that still pass the checksum. Therefore accurate determination of long-distance propagation requires the identification of multiple unique vessels over similar geometries. To avoid random errors, it is useful to observe multiple reports from a given ship over a few minutes; to observe consistency between the reported position, time, speed, and course; and to cross-reference with other information, such as ports of call. We have applied these techniques in filtering the AIS data, but the removal of erroneous data remains an open challenge.
In summary, long-distance AIS links appear to be a promising means of observing dense sporadic E layers. The data have several advantages, notably high power, high density of users and high cadence due to internationally mandated usage, and coverage over the oceans. The USCG dataset used here is not routinely available, but the protocol is public and transponders are widespread on ships and ground stations. Therefore much of the infrastructure is already in place to develop a worldwide monitoring network. This study indicates skywave propagation due to sporadic E layers is possible at higher frequencies than we were able to find previously reported in the literature, though we have not performed an exhaustive search.
Data analysis code is available here: https://doi.org/10.5281/zenodo.7278089 (Chartier, 2022b).
Digisonde data can be retrieved from http://giro.uml.edu/didbase/scaled.php (Global Ionosphere Radio Observatory, 2022). COSMIC-2 data are available from https://doi.org/10.5065/t353-c093 (UCAR COSMIC Program, 2019), while the sporadic E maps for our study are available at https://doi.org/10.5281/zenodo.6977022 (Emmons, 2022). Tropospheric ducting files are at https://doi.org/10.5281/zenodo.7140002 (Hanley and Chartier, 2022). The AIS data used here are not accessible to the public or research community, but it may be possible to obtain them from USCG by request. We note that public repositories of other VHF radio link data exist that may be useful for independent validation of these findings (e.g. https://www.wsprnet.org/drupal/, last access: 3 November 2022; https://pskreporter.info/pskmap.html, last access: 3 November 2022; https://mmmonvhf.de/odx.php, last access: 3 November 2022).
The full set of our >1000 km AIS links can be viewed at https://www.youtube.com/watch?v=AcNzM03zZP8 (Chartier, 2022a).
ATC wrote the paper, produced Figs. 1–6, and submitted the paper. TRH performed the AIS data analysis and first raised the possibility that these long-distance links were related to ionospheric phenomena. DJE performed the ionosonde–GNSS sporadic E analysis and produced Fig. 7.
The contact author has declared that none of the authors has any competing interests.
Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
Alex T. Chartier acknowledges support of NASA (grant no. 80NSSC21K1557).
This research has been supported by the National Aeronautics and Space Administration (grant no. 80NSSC21K1557)
This paper was edited by Jorge Luis Chau and reviewed by two anonymous referees.
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