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(meteorobs) Observation October 8/9 2003



Here's my meteor report for the evening of October 8.  I went out to 
the Casselman site to verify for any Giacobinid activity despite the 
Full Moon.  I watched for almost four hours teff until just after local 
midnight.  Unfortunately, the Full Moon really hampered any meteor 
activity at all.  It took well over an hour to see my first meteor.  
The Giacobinids were completely silent, and a total of only four 
sporadics were recorded.  Near the end, I was glad to have had a good 
dose of coffee to keep me awake for such a slow evening!

Looking forward to higher rates with the Orionids.

Clear skies!

Pierre Martin
Ottawa, Ontario



DATE: October 8/9 2003
BEGIN: 0022 UT (2022 EDT)  END: 0410 UT (0010 EDT)
OBSERVER: Pierre Martin (MARPI)
LOCATION: Long: -75.063 West; Lat: 45.269 North  Elevation: 50m
City & Province: Casselman, Ontario, CANADA
RECORDING METHOD: talking clock/tape recorder, plotting
-----------------------------------------------------------------------

OBSERVED SHOWERS:_____________________________________radiant position
		GIA (Giacobinids)______________________________ 1750 +54		SPO (random 
sporadics)
-----------------------------------------------------------------------

OBSERVING PERIODS: 0 = none seen;  / = shower not observed

PERIOD(UT)__FIELD___Teff__LM_____GIA_SPO

0022-0124__1711+49__1.01__5.03____0___0
0124-0225__1848+48__1.01__4.80____0___2
0225-0325__1942+55__1.00__4.78____0___1
0325-0410__2119+58__0.75__4.75____0___1

TOTALS:_____________3.77__________0___4

The first column (Period UT) refers to observing periods broken down as 
close as possible to one hour of true observing, in Universal Time. The 
second column (Field) is the area in in the sky where I centered my 
field of view. The third column (TEFF) represents effective observing 
time (corrected for breaks or any time I did not spent looking at the 
sky). The fourth column (F) is a value for obstructions in the field of 
view such as clouds (1.00 = 100% clear skies). The next column (LM) is 
the average naked eye limitimg magnitude, determined by triangle star 
counts. All following columns indicate the number of meteors for each 
shower observed.
------------------------

MAGNITUDE DISTRIBUTIONS:

SHOWER
_____+2__+3__+4_____AVE

SPO___2___1___1____+2.75

Note: Magnitude scale is to determine the brightness of sky objects. 
Magnitude -8 is comparable to a quarter moon, magnitude -4 with the 
planet Venus, magnitude -1 with the brightest star Sirius, magnitude +2 
to +3 with most average naked eye stars and magnitude +6 to +7 are the 
faintest stars the naked eye can see under typical dark conditions. A 
meteor of at least magnitude -3 is considered a fireball.  The above 
table contains the magnitudes from all observed meteors, and the 
average (last column) for showers.
------------------------

SKY OBSCURED (FOV): none
------------------------

Dead time: 2.16 min (breaks).
Breaks (UT): 0:29 (60sec), 0:37 (40sec), 2:14 (30sec)
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