The radio-observer occasionally creates a second meta.csv file. After that the file list looks like that:
20170804000000_HFN-R1_freq.csv
20170804000000_HFN-R1_meta.csv
20170804010000_HFN-R1_freq.csv
20170804010000_HFN-R1_meta.csv
20170804020000_HFN-R1_freq.csv
20170804020000_HFN-R1_meta.csv
20170804025608_HFN-R1_meta.csv
20170804030000_HFN-R1_freq.csv
20170804030000_HFN-R1_meta.csv
20170804040000_HFN-R1_freq.csv
20170804040000_HFN-R1_meta.csv
20170804050000_HFN-R1_freq.csv
20170804050000_HFN-R1_meta.csv
20170804060000_HFN-R1_freq.csv
20170804060000_HFN-R1_meta.csv
20170804070000_HFN-R1_freq.csv
20170804070000_HFN-R1_meta.csv
The second 20170804025608_HFN-R1_meta.csv created contains almost no data. Its contents look like that:
# file name; noise; peak f.; mag.; duration
20170804025509436_HFN-R1_snap.fits;2.49592;26535.6;3.413;0
Unfornutanelly the snapshot 20170804025509436_HFN-R1_snap.fits is not contained in previous original file 20170804020000_HFN-R1_meta.csv
This behavior could be related to station sensitivity increase, because the problem was observed first after receiver upgrade, resulting in increased meteor count detected per one snapshot interval.
The radio-observer occasionally creates a second meta.csv file. After that the file list looks like that:
20170804000000_HFN-R1_freq.csv
20170804000000_HFN-R1_meta.csv
20170804010000_HFN-R1_freq.csv
20170804010000_HFN-R1_meta.csv
20170804020000_HFN-R1_freq.csv
20170804020000_HFN-R1_meta.csv
20170804025608_HFN-R1_meta.csv
20170804030000_HFN-R1_freq.csv
20170804030000_HFN-R1_meta.csv
20170804040000_HFN-R1_freq.csv
20170804040000_HFN-R1_meta.csv
20170804050000_HFN-R1_freq.csv
20170804050000_HFN-R1_meta.csv
20170804060000_HFN-R1_freq.csv
20170804060000_HFN-R1_meta.csv
20170804070000_HFN-R1_freq.csv
20170804070000_HFN-R1_meta.csv
The second 20170804025608_HFN-R1_meta.csv created contains almost no data. Its contents look like that:
Unfornutanelly the snapshot 20170804025509436_HFN-R1_snap.fits is not contained in previous original file 20170804020000_HFN-R1_meta.csv
This behavior could be related to station sensitivity increase, because the problem was observed first after receiver upgrade, resulting in increased meteor count detected per one snapshot interval.