The inter-relationships between magnetic helicity, magnetic reconnection, and dynamo eects are discussed. In laboratory experiments, where two plasmas are driven to merge, the helicity content of each plasma strongly aects the reconnection rate as well as the shape of the diusion region. Conversely, magnetic reconnection events also strongly aect the global helicity, resulting in ecient helicity cancellation (but not dissipation) during counter-helicity reconnection and a nite helicity increase or decrease (but less eciently than dissipation of magnetic energy) during co-helicity reconnection. Close relationships also exist between magnetic helicity and dynamo eects. The turbulent electromotive force along the mean magnetic eld (-eect), due to either electrostatic turbulence or the electron diamagnetic eect, transports mean-eld helicity across space without dissipation. This has been supported by direct measurements of helicity ux in a laboratory plasma. When the dynamo eect is driven by electromagnetic turbulence, helicity in the turbulent eld is converted to mean-eld helicity. In all cases, however, dynamo processes conserve total helicity except for a small battery eect, consistent with the observation that the helicity is approximately conserved during magnetic relaxation.