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As the interface between the Sun's photosphere and corona, the chromosphereand transition region play a key role in the formation and acceleration of thesolar wind. Observations from the Interface Region Imaging Spectrograph revealthe prevalence of intermittent small-scale jets with speeds of 80-250 km/s fromthe narrow bright network lanes of this interface region. These jets havelifetimes of 20-80 seconds and widths of 300 km or less. They originate fromsmall-scale bright regions, often preceded by footpoint brightenings andaccompanied by transverse waves with ~20 km/s amplitudes. Many jets reachtemperatures of at least ~1 K and constitute an important element of thetransition region structures. They are likely an intermittent but persistentsource of mass and energy for the solar wind.

Prevalence of Small-scale Jets from the Networks of the Solar Transition Region and Chromosphere