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Dátum: 2003-11-20 09:36:41
Feladó: Hevesi Zoltán
Tárgy: IMO Shower Circ.: Leonids 2003
>            -------------------------------------
>            I M O   S h o w e r   C i r c u l a r
>            -------------------------------------
>
>                     LEONIDS 2003, VISUAL
>
>
> The 2003 Leonid meteor shower has not yet provided distinct
> peaks of activity. A full week of moderate Leonid meteor
> rates has shown only one clear maximum; near 2003 Nov 19.4 UT
> with an uncertainty of roughly +-6 hours.
>
> This maximum coincides with the predicted times of about
> 06h30 - 08h00 UT for the encounter with the 15-revolution
> dust trail of parent comet 55P/Tempel-Tuttle. The dust
> was ejected from the comet near its perihelion passagein
> 1533.
>
> The material ejected in 1499 has produced enhanced rates
> on November 13, but no clear peak time can be derived from
> the data received so far.
>
> The ZHR gives the number of meteors as if the radiant would
> be in the zenith, and at an observer´s stellar limiting
> magnitude of +6.5. The latter condition implies strong
> extrapolations of observed meteor numbers, since the waning
> moon interfered with most of the observing periods.
>
> At this preliminary state, only the relative variations in
> the ZHR should be of interest. Absolute values must be
> discussed and fixed with the full dataset.
>
> --------------------------------------
> Date     Solarlong  nINT   nLEO    ZHR
> --------------------------------------
> Nov 12.80   229.93     1      0     (0)
> Nov 13.50   230.64     4     13     26
> Nov 13.72   230.86     7     12     21
> Nov 14.01   231.15     7      9     27
> Nov 14.77   231.92     1      2    (47)
> Nov 15.76   232.91    13     28     15
> Nov 16.24   233.40     1      4    (20)
> Nov 17.21   234.37     4      7      7
> Nov 18.52   235.69     6     18     13
> Nov 19.06   236.24     9     63     23
> Nov 19.14   236.32    10     51     39
> Nov 19.37   236.55    14     88     53
> Nov 19.90   237.09    14     35     39
> --------------------------------------
>
> A population index of r=2.3 was used to extrapolate to lm=+6.5.
> All solar longitudes refer to equinox J2000.0. nINT is the
> number of observing periods, nLEO the number of Leonid meteors.
>
> We would like to thank the following observers for their
> contributions to the above ZHR table:
>
> Alexandre Amorim, Joseph Assmus, Jure Atanackov, Aleksandar Atevik,
> Shushrut Bhanushali, Michael Boschat, Dustin Brown, Ed Cannon,
> Parag Deotare, Kshitija Deshpande, Lucio Furlanetto, Kearn Jones,
> Paul Jones, Javor Kac, Ashish Kuvelkar, Anna Levina, Michael Linnolt,
> Qiang Ma, Xiaoyun Ma, Paul Martsching, Mikhail Maslov, Alastair
> McBeath, Norman McLeod, Huan Meng, Yatin Patnekar, Nilesh Puntambekar,
> Tushar Purohit, Jurgen Rendtel, Rahul Sangole, Mikiya Sato, Tomoko
> Sato, Vladimir Slusarenko, Wesley Stone, Kazumi Terakubo, Richard
> Taibi, Michel Vandeputte, Jeremie Vaubaillon, Linjia Wang, Yi Wang,
> Guangjie Wu, Quanzhi Ye, Chao Zhang, Menglin Zhang, Zhousheng Zhang.
>
>
> Rainer Arlt, 2003 Nov 20, 09h UT
Vissza

  

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