  Ellerman Bombs (EBs) are thought to arise as a result of photospheric
magnetic reconnection. We use data from the Swedish 1-m Solar Telescope (SST),
to study EB events on the solar disk and at the limb. Both datasets show that
EBs are connected to the foot-points of forming chromospheric jets. The limb
observations show that a bright structure in the H$\alpha$ blue wing connects
to the EB initially fuelling it, leading to the ejection of material upwards.
The material moves along a loop structure where a newly formed jet is
subsequently observed in the red wing of H$\alpha$. In the disk dataset, an EB
initiates a jet which propagates away from the apparent reconnection site
within the EB flame. The EB then splits into two, with associated brightenings
in the inter-granular lanes (IGLs). Micro-jets are then observed, extending to
500 km with a lifetime of a few minutes. Observed velocities of the micro-jets
are approximately 5-10 km s$^{-1}$, while their chromospheric counterparts
range from 50-80 km s$^{-1}$. MURaM simulations of quiet Sun reconnection show
that micro-jets with similar properties to that of the observations follow the
line of reconnection in the photosphere, with associated H$\alpha$ brightening
at the location of increased temperature.
