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(meteorobs) Observation June 25/26 2001



On June 25/26, I went to Casselman under clear skies and concentrated 
on June Bootids and Sagittarids by facing south-west. The very first 
meteor seen was a slow moving 1st magnitude low in the west over 20 
degrees, and had my hopes up. The plot showed the radiant alignment 
was too much of a miss (even assuming a diffuse radiant), so I called 
it a sporadic. The only other JBO candidate was also too badly 
aligned to the radiant.

Lots of sporadics were seen... 9 in the first hour alone! The best 
meteor was a sporadic from the north apex source at 6:13UT. It was a 
blue magn -1 that shot very swiftly high in the south-west, leaving 
behind a 2 sec train.

At 6:18UT, a satellite tumbling very quickly 80deg high in the east.

Pierre Martin
Ottawa, Ontario



DATE: June 25/26 2001
BEGIN: 4:25 UT (0:25 EDT)  END: 6:30 UT (2:30 EDT)
OBSERVER: Pierre Martin (MARPI)
LOCATION: Long: -75.063 West; Lat: 45.269 North  Elevation:100m
City & Province: Casselman, Ontario, CANADA
RECORDING METHOD: talking clock/tape recorder
-----------------------------------------------------------------------

OBSERVED SHOWERS: 3-letter code;    		 	radiant position
              	SAG (Sagittarids)			19h00 -20
		TOP (Theta Ophiuchids)			17h35 -17
		JBO (June Bootids)			15h00 +48
-----------------------------------------------------------------------

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

PERIOD(UT)   FIELD   	Teff   F     LM    SPO napx SAG TOP JBO
4:25-5:27    16h54 +20	1.00  1.00  6.26    9   0    1   1   0
5:27-6:30    16h54 +20	1.02  "	    6.32    5   2    1   1   0
--------------------------------------------------------------
TOTALS:              	2.02		    14  2    2   2   0  =  20
--------------------------------------------------------------
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). One hour = 1.00 teff. The fourth column 
(F) is for sky obstructions (clouds, buildings, ect). No obstructions 
= 1.00 but any obstructions will make this number slightly higher. 
The 5th 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 -1   0  +1  +2  +3  +4  +5	AVERAGE

SPO     1   0   2   2   4   5   2  	+3.35
SAG     0   0   0   1   0   1   0	+3.0
TOP     0   0   0   0   0   1   1	+4.5
---------------------------------
TOTALS: 1   0   2   3   4   7   3
---------------------------------
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 wi

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