| 1983 |
Kamioka Underground Observatory was established. |
| 1983 Jul. |
Kamiokande experiment started observation. |
| 1985 |
Kamiokande denied the simplest GUT as a result of proton decay search. |
| 1987 Feb. |
Kamiokande succeeded in detecting neutrinos from a supernova explosion. |
| 1988 |
Kamiokande observed a solar neutrino deficit. |
| 1991 Dec. |
The construction of Super-Kamiokande (SK) was started. |
| 1994 Jan. |
The construction of a computer building was completed. |
| 1994 Jun. |
The excavation for the SK detector was finished. |
| 1995 Apr. |
Kamioka Observatory which belongs to the Institute for Cosmic Ray Research(ICRR), was established. |
| 1996 Apr. |
SK experiment started observation. |
| 1998 Jun. |
SK discovered the atmospheric neutrino oscillation. |
| 1999 Jun. |
The long baseline neutrino oscillation experiment; K2K started. |
| 2001 Jun. |
SK discovered the solar neutrino oscillation. |
| 2001 Jul. |
SK started replacement of several hundred nonfunctional PMTs. |
| 2001 Nov. |
After replacement work, half of the PMTs were destroyed by a chain reaction |
| 2002 Dec. |
The Nobel prize in Physics was awarded to Professor Koshiba as a consequence of the major scientific results obtained at Kamiokande. |
| 2002 Oct. |
SK started observation with about 5200 inner detector PMTs. |
| 2004 Jun. |
K2K experiment confirmed the neutrino oscillation. |
| 2004 Nov. |
K2K experiment was finished. |
| 2005 Oct. |
The new PMTs were almost ready, the full reconstruction work began. |
| 2006 Jul. |
SK started observation with full complement of PMTs. |
| 2008 Aug. |
The new hall for XMASS experiment was completed. |
| 2008 Sep. |
The new data acquisition system of SK was installed. |