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The SEVAN detector has several sets of scintillators to record the incoming cosmic rays of different origin. The topmost 5cm thick scintillators can record the galactic cosmic rays while the middle unit of 25 cm thickness is capable of recording the cosmic rays from the Sun. It has been recorded that 6hours before the thunderstorm in Delhi the topmost unit of SEVAN has detected a sharp rise in cosmic rays while the middle unit of same device has recorded a low cosmic ray intensity than the normal. The pressure sensor of SEVAN has shown sympathetic rise with the 5 cm cosmic ray sensor.