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(meteorobs) Observation 23/12/2003



Hi!

There was a little problem with my mail settings, so I'll repost the 
report now.

I'm a little late with my report, but some things have interfered with 
my Christmas plans this year that made everything go a little 
slower... still: here's my report.
I also checked for activity from the radiant in central Leo as 
suggested by Kim Youmans and found two plots on my map to be 
candidates, one of the Sporadics crosses Lynx and is a candidate for 
the source Robert Lunsford mentions in his recent meteor outlook, so 
too bad we do not have more plots of these possible sources yet.

Season's Greetings to all of you and clear skies


Daniel Gruen

----------

Day:23-24 Month:12 Year:2003
Begin: 20h58m   End:  1h18m

Location  long. E9d26'25"  latit. N48d51'57"

Site: Winnenden-Birkmannsweiler, near Stuttgart
Country: Germany

Observer: Daniel GRUEN   IMO code: GRUDA
Any questions? Mail me (daniel_gruen@webdot de)

Showers:
.-------------------------------------
|.Shw.|alpha|delta|veloc.|a.h|HR |eZHR|
|--------------------------*-------~--|
|.ANT.|.104d|.+23d|sl-med|53d|0.4|1.81|+
|.COM.|.179d|.+15d|42km/s|65d|0.9|3.19|
|.URS.|.215d|.+75d|33km/s|40d|1.3|6.75|
|.SPO.|.---.|.---.|.----.|.-.|5.2|.--.|
.-------------------------------------
these figures are taken from the current
AMS Meteor Activity Outlook by Robert Lunsford
* average radiant height (est.)
~ estimated with r=3.0, deltalm=0.0 and est. radiant height
+ how shall I label Antihelion meteors now?

Periods:
.---------------------------------------------------
|.Period....|Field....|Teff|.F.|.lm.|ANT|COM|URS|SPO|
|..(UT).....|RA..dot dec.|..h.|...|.m..|M|N|M|N|M|N|M|N|
|---------------------------------------------------|
|20:58-22:04|095d|+44d|1.04|1.0|4.99|P|0|P|1|P|1|P|3|
|---------------------------------------------------|
|23:53-01:18|143d|+52d|1.27|1.0|5.74|P|1|P|1|P|2|P|9|
.---------------------------------------------------

Magnitude Distribution:
.-----------------------------------------------------.
|Shower.|.-3|.-2|.-1|..0|.+1|.+2|.+3|.+4|.+5|avg.|.tot|
|-------|---|---|---|---|---|---|---|---|---|----|----|
|.ANT...|...|...|...|...|...|...|...|0.5|0.5|4.50|..1.|
|.COM...|...|...|1.0|...|...|...|1.0|...|...|1.00|..2.|Y
|.URS...|...|...|...|...|...|0.5|1.5|1.0|...|3.17|..3.|
|.SPO...|...|0.5|1.5|3.0|1.0|2.0|1.0|2.5|0.5|1.50|.12.|
.-----------------------------------------------------.
Y both meteors also fit Kim Youmans' Radiant (see comment)

Train Distribution:
.-----------------------------.
|dur.|5s|4s|3s|2s|1s|<*|no|tot|
|----|--|--|--|--|--|--|--|---|
|ANT.|..|..|..|..|..|..|.1|.1.|
|COM.|..|..|..|..|..|..|.2|.2.|
|ANT.|..|..|..|..|..|..|.3|.3.|
|ANT.|..|..|..|..|.1|.2|.9|12.|
.-----------------------------.
 * these trains persisted only for a few tenth of a second

Meteor Data:
(caution: I changed the order of the coordinates from
XBeg-YBeg-XEnd-YEnd to XBeg-XEnd-YBeg-YEnd)
.--------------------------------------------------------.
|No.|.Time|.Mag|Vel|Shw|Train|XBeg|XEnd|YBeg|YEnd|Map|Acc|
|---|-----|----|---|---|-----|----|----|----|----|---|---|
|518|21:12| 2.5|1-2|URS| --- | 170| 174| 161| 139| 4 | 3 |*
|519|21:22| 4.5|2-3|SPO| --- | 108| 084| 226| 248| 4 | 2 |
|520|21:26| 3.5| 2 |SPO| --- | 175| 179| 291| 308| 4 | 2 |
|521|21:45|-1.0| 2 |COM| --- | 114| 114| 181| 217| 2 | 3 |Y
|522|22:02| 4.0| 4 |SPO| --- | 253| 206| 113| 083| 2 | 2 |
|---|-----|----|---|---|-----|----|----|----|----|---|---|
|523|23:55|-0.5|4-5|SPO| <1s | 253| 224| 113| 084| 2 | 2 |
|524|00:08| 3.5| 3 |URS| --- | 168| 179| 151| 128| 2 | 1 |
|525|00:11| 1.0| 3 |SPO| --- | 131| 146| 024| 007| 2 | 3 |
|526|00:16| 3.5|4-5|SPO| --- | 095| 133| 172| 191| 2 | 1 |
|527|00:17| 0.0|3-4|SPO| <1s | 128| 115| 131| 156| 2 | 2 |
|528|00:19|-1.5|3-4|SPO| 1.0s| 141| 104| 078| 093| 2 | 3 |
|529|00:28| 2.0| 4 |SPO| --- | 058| 031| 259| 215| 4 | 2 |
|530|00:29| 4.5| 2 |ANT| --- | 208| 158| 096| 091| 2 | 1 |+
|531|00:57| 3.5| 2 |URS| --- | 116| 121| 101| 057| 2 | 2 |
|532|00:59| 3.0| 3 |COM| --- | 167| 200| 026| 035| 2 | 1 |Y
|533|01:05|-0.5| 2 |SPO| --- | 195| 203| 128| 125| 2 | 2 |~
|534|01:07| 0.0|2-3|SPO| --- | 090| 072| 129| 121| 2 | 1 |
|535|01:11| 2.0| 5 |SPO| --- | 119| 096| 151| 165| 2 | 2 |+ L
.--------------------------------------------------------.
enumeration starts in the 20/02/2003 session
all coordinates in mm from the lower left corner of the map
velocity scale:
1 - very slow; 2 - slow; 3 - medium; 4 - fast; 5 - very fast
* lines up with the URS radiant, but might be too slow and
  to short at this distance from the radiant
Y a candidate for Kim Youmans' radiant in central LEO
+ no perfect intersection with the ANT radiant, but all ANTs
  will be archived as Sporadics anyway I guess
~ strong yellow color
L backtrace crosses the constelleation of Lynx around 35 LYN,
  therefore a candidate for the Lynx activity mentioned by
  Robert Lunsford

Comments: Ursid rates were not a surprise, but still nice to
at least see something after two clouded nights. Kim Youmans
suggested a radiant in central Leo in his posts on the meteorobs
mailing list, so I checked my plots (to bad he didn't plot some
of his meteors) and found the two I noted as COM to be possibly
radiating from there.

Please note: d = degrees, all times in UT

This research has made use of the USNOFS Image and Catalogue Archive
operated by the United States Naval Observatory, Flagstaff Station
(http://www.nofs.navy.mil/data/fchpix/).

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