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(meteorobs) More preliminary ZHR results (Europe too)
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To: meteorobs@latrade.com, Dutch Meteor Society -- Alex Scholten <a.scholten@dcs.cnt.antennadot nl>, Carl Johannink <cjohannink@compuserve.com>, Casper ter Kuile <pegasoft@cc.ruudot nl>, Erwin Ballegoij <ballegoy@worldaccessdot nl>, Guus Docters van Leeuwen <dl@THRijswijkdot nl>, Hans Betlem <betlem@strw.leidenunivdot nl>, Jaap van 't Leven <JVTleven@interdot nldot net>, Jos Nijland <jnb@worldonlinedot nl>, Klaas Jobse <cyclops@zeelandnetdot nl>, Marc de Lignie <mcdelign@pidot net>, Olga van Mil <pvmilnwk@boxdot nl>, Peter Jenniskens <peter@max.arc.nasadot gov>, Peter Bus <epbus@worldaccessdot nl>, Piet Koning <P.A.Koning@net.HCCdot nl>, Reinder Bouma <rjbouma@pidot net>, Robert Haas <delpsurf@pop3.cistrondot nl>, Eddy Echternach <zenit@astro.rugdot nl>, IMO news <imo-news@imodot net>, charlieh@hsmpk12a-55.Eng.Sun.COM, George Zay <GeoZay@aol.com>, Robert Lunsford <lunro.imo.usa@prodigy.com>, evanross@stad.dsldot nl
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Subject: (meteorobs) More preliminary ZHR results (Europe too)
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From: Marco Langbroek <marcolan@stad.dsldot nl>
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Date: Wed, 19 Nov 1997 17:47:51 +0100 (CET)
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Cc: marcolan@stad.dsldot nl
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Reply-To: meteorobs@latrade.com
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Sender: owner-meteorobs
Hello again,
Below some VERY preliminary ZHR-results from our Dutch observations, to
add to the preliminary ZHR for california I communicated earlier. Again:
please regard this as an indication of rate level only. It is based on
data from 3 observers: Carl Johannink, Koen Miskotte and me (=Marco
Langbroek).
In general, ZHR's were around ~50 for early november 17 as observed from
Northwest Europe. Unfortunately, our observing interval was short due to
clouds. The next night, 17/18, saw a ZHR that decreased clearly over the
night, from about ~40 to ~30. Coupled to the ZHR ~115 seen from
California (note: based on Bob's data only, so be carefull!), this agrees
excellently with a B~1 component peaking at around ZHR ~115 (annual +
outburst combined: outburst only ~100) above the western USA, with B
describing rate behaviour as in the next equation:
ZHR = ZHR_max * 10^-B|l-l_max| (See Astron. Astroph. 295 (1995), 206)
...with l= solar longitude
This means that a similar broad B ~1 (and bright) component as in
1994-1995-1996 has been present, this time with a peak ZHR near 100.
It is not clear whether a narrow peak was also present, as in 1996.
Perhaps Bob and some others saw the onset after 13:00 and the narrow peak
then might have peaked just after the end of the Californian time window,
over the western Pacific perhaps. But as George noted, 'storm'-rates have
not been seen by Californians themselves, judging from the reports and
Bob's data.
Below some ZHR's for the European intervals, as described above,
calculated for r=2.0 with gamma=1.4 and perception taken into account
(Carl: 1.0: Koen: 1.2; Marco: 1.4).
Nov 17
UT ZHR +-
1:30 50 8
Nov 18
UT ZHR +-
1:45 42 5
3:42 28 4
Add these to the values from Bob's observations from west USA send
earlier (ZHR's around 115, except for last hour which might have been
higher). The outburst was present for about one day, with Europe seeing
rates going up the one night and down the other, and the USA having the
privilege of the peak.
-Marco Langbroek
Dutch Meteor Society