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Agapitoi filoi,

 

Thn alli vdomada 8a exoume thn emfanisi ths vroxis metewrwn me to onoma Leontides.

Anamenetai na einai ena apo ta megalutera astronomika 8eamata (merikes xiliades thn wra..!) kai isws anepanalipto gia ta epomena xronia (kati analogo upologizetai to ...2099!)

Dustuxws h Eurwpi den eunoeitai idiaitera alla sigoura 8a doume simantiki drastiriotita.

 

Gia perissoteres plirofories: http://www.skypub.com/sights/skyevents/0111skyevents.shtml http://science.nasa.gov/headlines/y2001/ast08nov_1.htm?list556196 http://space.com/scienceastronomy/astronomy/leonids_citytimes-1.html http://see.msfc.nasa.gov/see/Leonid_Forecast_2001.html http://www.amsmeteors.org/lunsford/

 

Gia to pws 8a ta paratirisete: http://www.skypub.com/sights/meteors/meteorwatch.html http://www.space.com/scienceastronomy/astronomy/leonid_watching_011106-1.htm

 

Kai eidika sites me 8ema ta metewra: http://www.imo.net/ http://www.amsmeteors.org/ http://www.namnmeteors.org/ http://www.meteorobs.org/

 

Grhgorhs

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Agapitoi filoi,

 

Hdh tin emfanisi tous oi prwtes Leontides tin kanane! Proetoimasteite me zesta rouxa kai upomoni, kai vgeite meta ta mesanuxta gia na tis paratirisete.

Idiaitera ta 3hmerwmata tis 18 Noemvriou anamenetai to megalutero 8eama. Vevaia auto einai kapoia provlepsi pou mporei na pesei kai e3w kai na exoume tin proigoumeni h tin epomeni e3eairetika megali drasthriotita. Kalo loipon 8a itan na parakolou8isete kai alles meres alla an den mporeite oi prwtes proines wres tis 18 noemvriou einai mallon oi kaluteres!

Elpizw mono na eunoeisei o kairos kai na e3afanistoun kapoia sunnefa pou exei edw h A8ina...

 

Kales paratiriseis,

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Agapitoi filoi,

 

Dustuxws o apologismos den itan dunatos gia tin Athina kathws to vradi 17/18 o ouranos itan sunexws synnefiasmenos !! (kanena apo ta proigoumena vradia den eixe toso asximes sunthikes!). Mono kata tis 6 to prwi katharise kapws kai se 25 peripou lepta katafera na katagrapsw 10 metewra, kuriws lampra.

 

Parakatw einai mia prwti sunoliki analusi tis drastiriotitas pou parousiasan oi Leontides (forwarded apo tin IMO)

 

Grigoris,

 

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

International Meteor Organization

Meteor Shower Circular

 

2 0 0 1 L E O N I D S

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

 

This year's Leonids were marked from excellent lunar conditions. The weather

was also very friendly to most of the observers around the world.

 

The strongest peak observed is around 18h20min UT which was suitably

situated for the observers in East Asia and Australia. The rates during this

peak reached more then 2800 meteors per hour. This is well below the

theoretically predicted peak levels which were around 5000 according to

Lyytinen/Nissinen/van Flaudern or 8000 in Asher/McNaught's model.

 

As far as the first peak, observed from America, is concerned rates were

between 1000 and 1500 meteors per hour. However there is still not enough

data reported from it especially about the time after 11 UT.

 

The first activity profile is derived from the observations of 38 observers.

It is aimed to give a general view of the observed shower and no conclusions

can be made on this stage. The following detail analysis will tell us more

about the shower and the dust trail models.

 

Data of the following observers is included in the preliminary profile. The

countries in brackets show the place where observations were carried out,

not necessarily his home land :

Albert Kong (USA), Andreas Buchman (Germany), Andrzej Skoczewski (Poland),

Antonio Martinez (Venezuela), Brian Shulist (Canada), Camila Bacher (USA),

Carles Pineda Ferre (Spain), Detlef Koschny(Australia), Francisco A.

Rodriguez Ramirez (Spain), Gaurav Rathod (India), Ina Rendtel (Germany),

James Bedient (USA), Jaydeep Belapure (India), Joe Zemder (Australia), Josep

M. Trigo-Rodriguez (Spain), Joseph Zammit (Malta), Kamil Hornoch (Pland),

Ken Hodonsky (USA), Kim Youmans (USA), Marion Rudolph (Germany),Mark Davis

(USA), Martin Galea De Giovanni (Malta), Mayuresh Girish Prabhune (India),

Michael Doyle (USA), Miguel A. Serra (Spain), Mike Linnolt (USA), Rafael

Haag (Brazil), Rainer Arlt (Korea), Robert Lunsford (USA), Shigeo Uchiyama

Japan), Sirko Molau (Korea), Tom Roelandts (China), Tomislav Jurkic

(Croatia), Umberto MulХ Stagno (Tunis), Valentin Velkov (Bulgaria), Werner

Hamelinck (China), Xiaorong Wang (China), Zhou Xingming (China)

 

 

_____________________________________

Date Time Sollong Nint Nobs ZHR +/-

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

18 0100 235.732 23 8 52 4

18 0300 235.816 22 9 80 3

18 0500 235.900 21 8 95 5

18 0630 235.963 11 5 160 10

18 0730 236.005 15 7 200 10

18 0815 236.036 13 5 150 10

18 0845 236.057 15 5 270 15

18 0915 236.078 18 6 430 20

18 0945 236.099 12 6 570 20

18 1015 236.121 17 6 790 25

18 1045 236.142 20 5 1000 25

18 1130 236.173 8 2 400 40

18 1300 236.236 12 2 370 25

18 1430 236.299 9 1 320 20

18 1530 236.341 16 3 490 30

18 1630 236.383 16 3 780 40

18 1700 236.404 16 4 1100 50

18 1730 236.425 18 4 1550 50

18 1800 236.446 20 5 2320 60

18 1820 236.460 28 7 2850 60

18 1840 236.474 32 7 2430 50

18 1900 236.488 21 6 1580 50

18 1920 236.509 18 5 1160 40

18 1940 236.516 17 5 1020 40

18 2000 236.530 17 7 800 30

18 2030 236.551 13 5 470 20

18 2120 236.587 16 5 150 10

18 2220 236.629 7 4 130 10

______________________________________

 

Calculations are made for population index r=2.0. Nint is the number of

intervals observing intervals in a certain period. Nobs is the number of

different observers in it.

 

Many thanks to all the observers that have contributed their data. Also to

the favorable weather conditions whish are not so typical for this part of

the year.

 

Clear Skies,

Vladimir Krumov

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