IMO天琴座流星雨分析报告出来了
没有中国报告 -------------------------------------
I M O S h o w e r C i r c u l a r
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LYRIDS 2004, VISUAL
Reports from only 21 observers have been received reporting
about the activity of the 2004 Lyrids. A first ZHR profile
was constructed from these data. The maximum time is near
April 22.0 and is a few hours earlier than the average max-
imum time of the last decade. The contributors are:
ADEHA Harshil Adesara (India; not used)
BANAN Ana Bankovic (Serbia)
CERAN Ana Cernok (Serbia)
GLIGE George W. Gliba (USA)
KACJA Javor Kac (Slovenia)
KOTMA Marija Kotur (Serbia)
KULRI Rishikesh Kulkarni (India; not used)
MASMI Mikhail Maslov (Russia)
MILIV Ivan Milic (Serbia)
MISKO Koen Miskotte (Netherlands)
MOLSI Sirko Molau (Germany)
PAWNI Nikhil Pawar (India; not used)
PUNNI Nilesh Puntambekar (India; not used)
SAVBR Branislav Savic (Serbia)
STOWE Welsey Stone (USA)
TAIRI Richard Taibi (USA)
VANMC Michel Vandeputte (Belgium)
VELKR Kristina Veljkovic (Serbia)
VELVA Valentin Velkov (Bulgaria)
WEITH Thomas Weiland (Austria)
YOUKI Kim Youmans (USA)
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Date (UT) Time Solarlong nINT nLYR ZHR
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Apr 20.06 01:26 30.261 2 8 5 +- 2
Apr 21.09 02:10 31.267 2 11 16 +- 5
Apr 22.01 00:14 32.164 5 45 21 +- 3
Apr 22.07 01:41 32.223 6 51 16 +- 2
Apr 22.29 06:58 32.438 9 54 10 +- 1
Apr 23.00 00:00 33.130 19 80 7 +- 1
Apr 23.97 23:17 34.075 4 9 4 +- 1
Apr 25.00 00:00 35.079 2 2 4 +- 2
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The ZHR was comuted by ZHR = nLYR*r^(6.5-LM)/(sin hR * Teff)
where r = 2.1, LM is the limiting magnitude, hR is the
radiant elevation and Teff is the effective observing time.
The data by the group from India delivered ZHRs which are
2-3 times higher than those of the other observers. They
have been excluded for this preliminary analysis.
Rainer Arlt
2004 Apr 27, 07:30 UT
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呵呵。。
因为我还没来得急将报告发出去。。所以。。
以往，我只是将观测结果寄给徐品新和朱进
因为我不懂英文，还不会用英文填写它们（IMO）的报告；又不知道IMO的具体发布报告网址……请二位帮帮我。谢谢！ www.imo.net
这里面有的。
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