Diagnostics of plasma jets in the solar corona

The paper discusses the diagnostics of plasma jets in solar corona with use data from modern space- and ground-based telescopes observing Sun extreme ultraviolet (EUV) micro- wave bands. We examine observational parameters EUV radio emission events associated jets, depending on mechanism formation, initiation conditions, evolution jets. opportunities provided by study which relies simultaneous observations different bands, are highlighted. For a number we have measured their primary parameters; this present preliminary results statistical processing obtained. Microwave several specific events, made instruments RATAN-600, SRH, Nobeyama Radioheliograph, considered detail. diagnostic capabilities these for studying coronal shown. To analyze three-dimensional structure magnetic field, used SDO/HMI data, allowed reconstruction field lower corona. information gained is compared at base according to RATAN-600 data. purpose methods developed determine physical mechanisms responsible generation, collimation, dynamics atmosphere.