Using extragalactic radio source observations at OVRO-LWA to estimate ionospheric TEC gradients and scintillation

Esayas B Shume1, Gregg Hallinan2, Marin Anderson2, Ryan Monroe2 and Michael Eastwood2, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)California Institute of Technology, Pasadena, CA, United States
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