Frissell, Nathaniel A.Kaeppler, Stephen R.Sanchez, Diego F.Perry, Gareth W.Engelke, William D.Erickson, Philip J.Coster, Anthea J.Ruohoniemi, J. MichaelBaker, Joseph B. H.West, Mary Lou2022-07-122022-07-122022-03-160094-8276e2022GL097879http://hdl.handle.net/10919/111219We demonstrate a novel method for observing Large Scale Traveling Ionospheric Disturbances (LSTIDs) using high frequency (HF) amateur radio reporting networks, including the Reverse Beacon Network (RBN), Weak Signal Propagation Reporter Network (WSPRNet), and PSKReporter. LSTIDs are quasi-periodic variations in ionospheric densities with horizontal wavelengths >1,000 km and periods between 30 and 180 min. On Nov 3, 2017, LSTID signatures were observed simultaneously over the continental United States in amateur radio, SuperDARN HF radar, and GNSS Total Electron Content with a period of similar to 2.5 hr, propagation azimuth of similar to 163 degrees, horizontal wavelength of similar to 1680 km, and phase speed of similar to 1,200 km hr(-1). SuperMAG SME index enhancements and Poker Flat Incoherent Scatter Radar measurements suggest the LSTIDs were driven by auroral electrojet intensifications and Joule heating. This novel measurement technique has applications in future scientific studies and for assessing the impact of LSTIDs on HF communications.application/pdfenCreative Commons Attribution-NonCommercial-NoDerivatives 4.0 InternationalLSTIDTraveling ionospheric Disturbancemidlatitude ionosphereamateur radioSuperDARNGNSS TECArticle - Refereedhttps://doi.org/10.1029/2022GL0978794951944-8007