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(meteorobs) Observation July 6/7 2002



Hi everybody,

Here are a series of long-overdue meteor observation reports for the 
month of July...

The first night this month was held at Foymount on July 6/7, a dark 
sky site located almost 2 hours west of Ottawa.  Weather conditions 
were going to be very promising, and above-average transparency was 
predicted.  Unfortunately, smoke blowing south from the forest fires 
in northern Quebec caused some problems.  As I signed-on near local 
midnight, my limiting magnitude averaged 6.25 and the Milky Way was a 
far cry from the very dark nights I usually experience at this site. 
No doubt, there was still lots of smoke hanging in the atmosphere. 
The air also had a strong "burning wood" odor, and dust would 
occasionally cause tears in my eyes.  As the night went on, the smoke 
slowly thinned somewhat until my limiting magnitude reached 6.45.  In 
any case, it was enjoyable to be out again...

I observed for two and a half hours TEFF (effective time). In this 
time, I recorded a total of 15 meteors (including one July Pegasid 
and 14 sporadics).  I used a combination of plotting and cord 
alignment.

The highlight was a magnitude 0 blue sporadic that shot a swift 20 
degrees long path across the sky!

Pierre Martin
Ottawa, Ontario


DATE: July 6/7 2002
BEGIN: 0355 UT (2355 EDT)  END: 0709 UT (0309 EDT)
OBSERVER: Pierre Martin (MARPI)
LOCATION: Long: -77.304 West; Lat: 45.431 North  Elevation: 1800 ft
City & Province: Foymount, Ontario, CANADA
RECORDING METHOD: talking clock/tape recorder
-----------------------------------------------------------------------

OBSERVED SHOWERS:_______________________________________radiant position
		SAG (Sagittarids antihelion source)_____299 -20
		CAP (Alpha Capricornids)________________287 -17
		JPG (July Pegasids)_____________________338 +15
		TAQ (Tau Aquarids)______________________350 -09
		CET (Cetids)____________________________033 -08
		napx (sporadics from the north apex)____056 +21
		sapx (sporadics from the south apex)____056 -09
		SPO (random sporadics)
-----------------------------------------------------------------------

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

PERIOD(UT)__FIELD____Teff__LM____SPO_JPG_SAG_CAP_TAQ_CET_napx_sapx

0355-0456___1859+15__1.00__6.25__4___0___0___0___0___0____0____0
0456-0629___2014+15__1.00__6.35__5___1___0___0___0___0____1____0
0629-0709___2110+10__0.52__6.45__4___0___0___0___0___0____0____0

TOTALS:______________2.52________13__1___0___0___0___0____1____0 = 15

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 
(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

SPO: +0(1) 1(1) +2(1) +3(2) +4(5) +5(4) AVE: +3.5
JPG: +0(0) 1(0) +2(0) +3(1) +4(0) +5(0) AVE: +3.0

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:

None

Corresponding F value for this session is 1.00

------------------------

Dead time:
- 41.58 minutes for breaks.
- 1.16 min used for plots.

Breaks (UT): 0409 (30 sec), 0439 (20 sec), 0500-0513, 0525-0538, 
0600-0601, 0615-0620, 0641-0649, 0652 (45 sec)
---------------------------------------------------------------------








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