  We use H$\alpha$ imaging spectroscopy taken via the Swedish 1-m Solar
Telescope (SST) to investigate the occurrence of fan-shaped jets at the solar
limb. We show evidence for near-simultaneous photospheric reconnection at a
sunspot edge leading to the jets appearance, with upward velocities of 30\ks,
and extensions up to 8~Mm. The brightening at the base of the jets appears
recurrent, with a periodicity matching that of the nearby sunspot penumbra,
implying running penumbral waves could be the driver of the jets. The jets'
constant extension velocity implies that a driver counteracting solar gravity
exists, possibly as a result of the recurrent reconnection erupting material
into the chromosphere. These jets also show signatures in higher temperature
lines captured from the Solar Dynamics Observatory (SDO), indicating a very hot
jet front, leaving behind optically thick cool plasma in its wake.
