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Abstract. We present the first observations from a new low-cost obliqueionosonde located in Antarctica. The transmitter is located at McMurdoStation, Ross Island, and the receiver at Amundsen–Scott Station, South Pole.The system was demonstrated successfully in March 2019, with the experimentyielding over 30 000 ionospheric echoes over a 2-week period. These dataindicate the presence of a stable E layer and a sporadic and variableF layer with dramatic spread F of sometimes more than 500 km (in units ofvirtual height). The most important ionospheric parameter, NmF2, validateswell against the Jang Bogo Vertical Incidence Pulsed Ionospheric (VIPIR) ionosonde (observing more than 1000 kmaway). GPS-derived TEC data from the Multi-Instrument Data Analysis Software(MIDAS) algorithm can be considerednecessary but insufficient to predict 7.2 MHz propagation between McMurdoand the South Pole, yielding a true positive in 40 % of cases and a truenegative in 73 % of cases. The success of this pilot experiment at a totalgrant cost of USD 116 000 and an equipment cost of ∼ USD 15 000 indicates that a large multi-static network could be built to provide unprecedented observational coverage of the Antarctic ionosphere.
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An Assessment of HF Radio Wave Propagation in Antarctica for a Radio Link Between McMurdo and South Pole Station
Abstract In this work, we analyze data collected by an HF transmitter/receiver radio link, operating as an oblique ionosonde between the McMurdo Station (transmitter) and South Pole Station (receiver) at 4.1, 5.1, 6.0, 6.4, and 7.2 MHz between 28 February and 14 March 2019. To help contextualize the link's data we have performed numerical raytrace simulations to help understand the observations. By considering both the data and simulations, we have identified both single‐ and two‐hop E‐ and F‐region propagation modes in the data, where the multi‐hop modes were observed in the hours around sunrise and sunset in the 4.1 and 5.1 MHz channels. This is an unexpected result given the accepted wisdom that multi‐hop modes, which require a ground scatter component, cannot be supported in Antarctica because of the highly absorptive ice covering much of the continent. Our results show that multi‐hop propagation modes can be supported in the region under specific ionospheric conditions—around sunrise and sunset—if the mode's ground scatter component is collocated with the Transantarctic Mountains. The mountains are located along the great‐circle path between the link's transmitter and receiver. However, the combination of favorable ionospheric and ground scattering conditions makes the detection of the multi‐hop mode a rare occurrence in the data set analyzed here. These findings are critical to data analysis efforts of any current or future oblique ionosonde systems operating in Antarctica and other regions such as the Arctic.
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- Award ID(s):
- 2032421
- PAR ID:
- 10544425
- Publisher / Repository:
- DOI PREFIX: 10.1029
- Date Published:
- Journal Name:
- Radio Science
- Volume:
- 59
- Issue:
- 10
- ISSN:
- 0048-6604
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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