During the second half of 2020, I serendipitously captured six meteors on my telescope’s 17 x 11 arcminute video field of view while observing potential asteroid occultation events. I used the method described in There’s a Meteor in My Image to determine the radiant for each meteor. Here they are.
Each frame is an exposure of 0.13s (meteor is at left side of field)
A sporadic meteor is any meteor that does not come from a known radiant.
Each frame is an exposure of 0.13s ; possibly a Perseid (meteor from upper right to lower left)
Each frame is an exposure of 0.27s ; possibly a Perseid (meteor from upper right to lower left)
Each frame is an exposure of 0.13s ; (meteor at upper right)
Each frame is an exposure of 0.27s (meteor at upper right)
Each frame is an exposure of 0.13s ; (meteor along upper part of field)
None of these meteors were particularly bright, unfortunately, so you may want to use the full-screen button at the lower-right-hand corner of each video to see them well.
References
International Meteor Organization, 2o2o Meteor Shower Calendar, Jürgen Rendtel, ed. https://www.imo.net/files/meteor-shower/cal2020.pdf.