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Example of an Observer's Data By Pierre Martin On Thursday morning Oct 21 1999, I was out at Casselman to watch some decent
activity after moonset. Again tonight, I had to deal with variable clouds
(ranging from no more than 5% to 20% of my FOV while I was "on"). The first
half hour after beginning was clear, and only after that period I had to
start taking notes of the thin patchy clouds that moved slowly. Where it was
clear, the sky was magnitude 6.3. Despite the conditions, I managed to get
two successful hours of teff (actual observing time) until dawn. The first
hour produced 28 meteors. Of those, 19 were Orionids while the rest were
minor activity from both branch of the Taurids as well as some sporadics.
For the second hour, there was a sharp decline in overall activity (only 15
meteors). This decline is most likely due to the fact that many clouds
covered the south and I had to bring my FOV almost at the zenith where it
was still clear. Obviously, this meant looking at a much thinner part of the
atmosphere above me and so, less meteors were seen. There was two potential
Leo Minorids (LMI). The first is less reliable as I saw on the corner of my
eye, so I had to call it SPO. It was a brief but colorful magn. +2 streak
that moved just 2 degrees near the radiant located in Leo Minor. It left a
bright 1 sec train. Later on at night while on break (due to heavier
clouds), I casually spotted another swift LMI of magn.+3. The Taurids
complex produced just a few faint meteors. Another late Oct. Delta Aurigid
was seen. The Epsilon Geminids were not active. DATE: October 20/21 1999 ORI (Orionids) 06:24 +15OBSERVING PERIODS: 0 = none seen;
The first column (Period UT) refers to observing periods broken down as
close as possible to one hour periods, in Universal Time. The second column
(Field) is the area (E=east,W=west and so on) in the sky faced. The number
refers to the elevation in degrees where 0=horizon and 90=zenith. The third
column (F) is a value for sky obstructions (clouds, buildings). No
obstructions=1.00. Some obstructions will have this value slightly higher.
The fourth column (TEFF) represents the actual observing time (corrected for
breaks and any time not spent looking at the sky). One hour is 1.00 teff.
The 5th column (LM) is the average naked eye limitimg magnitude, determined
using triangle star count method. All following columns indicate the meteor
shower observed and their numbers seen.
Meteors of/or brighter than magnitude -3 are considered fireballs. | ||||||||||||||||||||||||||||||||||||||||||||||||
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