Nishitani, NozomuRuohoniemi, J. MichaelLester, MarkBaker, Joseph B. H.Koustov, Alexandre V.Shepherd, Simon G.Chisham, GarethHori, TomoakiThomas, Evan GrierMakarevich, Roman A.Marchaudon, AuréliePonomarenko, Pavlo V.Wild, James A.Milan, Stephen E.Bristow, William A.Devlin, JohnMiller, EthanGreenwald, Raymond A.Ogawa, TadahikoKikuchi, Takashi2019-03-252019-03-252019-03-18Progress in Earth and Planetary Science. 2019 Mar 18;6(1):27http://hdl.handle.net/10919/88520The Super Dual Auroral Radar Network (SuperDARN) is a network of high-frequency (HF) radars located in the high- and mid-latitude regions of both hemispheres that is operated under international cooperation. The network was originally designed for monitoring the dynamics of the ionosphere and upper atmosphere in the high-latitude regions. However, over the last approximately 15 years, SuperDARN has expanded into the mid-latitude regions. With radar coverage that now extends continuously from auroral to sub-auroral and mid-latitudes, a wide variety of new scientific findings have been obtained. In this paper, the background of mid-latitude SuperDARN is presented at first. Then, the accomplishments made with mid-latitude SuperDARN radars are reviewed in five specified scientific and technical areas: convection, ionospheric irregularities, HF propagation analysis, ion-neutral interactions, and magnetohydrodynamic (MHD) waves. Finally, the present status of mid-latitude SuperDARN is updated and directions for future research are discussed.application/pdfenCreative Commons Attribution 4.0 InternationalReview of the accomplishments of mid-latitude Super Dual Auroral Radar Network (SuperDARN) HF radarsArticle - Refereed2019-03-24The Author(s)Progress in Earth and Planetary Sciencehttps://doi.org/10.1186/s40645-019-0270-5