162
N. S. Philip
Fig. 8 Though transients are well defined, the inherent noise in the detector will be much larger
than the signal making it extremely difficult for their detection
Fig. 9 Though transients are well defined, the inherent noise in the detector will be much larger
than the signal making it extremely difficult for their detection
local weather stations accurately measure such events to mark those transients from
being misinterpreted as gravitational wave signals. A 30 minutes real data from 16
December 2015 was used to train the classifier to isolate lightning transients from
other types of transient events in the data. Two analyses were done on about 40
lighting events from the X- and Y-arms of the LIGO Livingston Observatories and
N. S. Philip
Fig. 8 Though transients are well defined, the inherent noise in the detector will be much larger
than the signal making it extremely difficult for their detection
Fig. 9 Though transients are well defined, the inherent noise in the detector will be much larger
than the signal making it extremely difficult for their detection
local weather stations accurately measure such events to mark those transients from
being misinterpreted as gravitational wave signals. A 30 minutes real data from 16
December 2015 was used to train the classifier to isolate lightning transients from
other types of transient events in the data. Two analyses were done on about 40
lighting events from the X- and Y-arms of the LIGO Livingston Observatories and