We redetermine magnitudes of the meteors by adjusting a meteor lasting time to be consistent with the naked-eye observations.
Jeong Han Kim, Jong-Kyun Chung, Yong Ha Kim, Young-In Won, Moo-Young Chun, Hong-SuhYim 2003, 'All-Sky Observation of the 2001 Leonid Meteor Storm: 1. Meteor Magnitude Distribution',Journal of Astronomy and Space Scienceshttp://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2003/v20n4/OJOOBS_2003_v20n4_283.pdf. Retrieved from DOAJ CC BY 4.0 (https://creativecommons.org/licenses/by-sa/4.0/legalcode)