  Neutrino physics is an experimentally driven field. So, we investigate the
different detection techniques available in the literature and study the
various neutrino oscillation experiments in a chronological manner. Our primary
focus is on the construction and detection mechanisms of each experiment.
Today, we know a lot about this mysterious ghostly particle by performing
different experiments at different times with different neutrino sources viz.
solar, atmospheric, reactor, accelerators and high energy astrophysical; and
they have contributed in the determination of neutrino parameters. Yet the
problems are far from over. We need to determine more precise values of the
already known parameters and unravel the completely unknown parameters. Some of
the unknowns are absolute masses of neutrino, types of neutrino, mass
hierarchy, octant degeneracy and existence of leptonic CP Phase(s). We analyse
the neutrino experiments into the past, present and the future (or proposed).
We include SNO, Kamiokande, K2K, MINOS, MINOS+, Chooz, NEMO and ICARUS in the
past; while Borexino, Double Chooz, Super-K, T2K, IceCube, KamLAND, NO$\nu$A,
RENO and Daya Bay in the present; and SNO+, Hyper-K, JUNO, RENO-50, INO, DUNE,
SuperNEMO, KM3NeT, P2O, LBNO and PINGU in the proposed experiments. We also
discuss the necessities of upgrading the present ones to those of the proposed
ones thereby summarizing the potentials of the future experiments. We conclude
this paper with the current status of the neutrinos.
