Re: 03年象限仪流星
2003年1月4日拍摄，地点宁河七里海。用旋转快门拍的啊 看来是群内的 [计划失败] :?: 徐震：下次回帖子，别这么不负责，怎么总用表情符号啊。
有灌水嫌疑，是在关于你的帖子里你才说话，这样可不行。 原来你们也观测不成啊，我还以为是我们这里多云。
真惨！ 我在4号晚上1小时看到12颗，其中3颗群内，太少了，该不该发到IMO？ 可以发啊。。。。。。。。。。 天龙的报告分析结果出来了！！！！
-------------------------------------
I M O S h o w e r C i r c u l a r
-------------------------------------
QUADRANTIDS 2006, visual observations
Visual observations of the 2006 Quadrantids received
by the IMO before January 8 were used to provide a
rough estimate of the 2006 activity of the meteor shower.
A total of 303 Quadrantids seen during 34 hours of
effective observing time were reported by 21 observers.
The maximum of the shower was lower than usual, with
a ZHR of about 85 near January 3, 23h-24h or a solar
longitude of 283.39 degrees (J2000.0). The expected
maximum would have occurred at 18h20 UT on January 3.
Only a single observer from Japan was able to report
his data for that time (first line in below table)
with a ZHR clearly below 100, too.
The number of individual observing periods is very small.
The shape of the activity profile depends on the sampling
of these data. The below table is not 'hand-picked' but
still it is a selected one out of three different compu-
ter-generated samplings. The selection is arbitrary;
we can find out what happened only more additional data.
If you have not yet sent your report, please do so.
-----------------------------------------------------
Jan (UT) Solarlong Nint NQUA ZHR lm
-----------------------------------------------------
03 19h00 283.1864 1 12 60.6 +- 16.8 5.40
03 20h10 283.2356 3 9 36.9 +- 11.7 5.42
03 22h00 283.3137 9 25 54.6 +- 10.7 5.62
03 23h00 283.3609 11 71 67.2 +- 7.9 5.56
03 23h40 283.3898 3 24 85.4 +- 17.1 5.74
04 02h30 283.5075 4 6 42.3 +- 16.0 4.72
04 03h10 283.5374 3 15 36.6 +- 9.2 5.33
-----------------------------------------------------
We are grateful to
Pierre Bader (Germany),
Rohit Belapurkar (India),
Sushrut Bhanushali (India),
Charuta Deshpande (India),
William Godley (USA),
Lew Gramer (USA),
Shy Halatzi (Israel),
Manali Kulkarni (India),
Omkar Kulkarni (India),
Rhishikesh Kulkarni (India),
Jens Lacorne (France),
Alastair McBeath (UK),
Tushar Purohit (India),
Pulin Raje (India),
Aaditya Ramdas (India),
Trupti Ranka (India),
Jurgen Rendtel (Germany),
Rahul Sangole (India),
Amit Shukrun (Israel),
Shigeo Uchiyama (Japan), and
Michel Vandeputte (Belgium)
for their quick submission of the observing reports.
The Zenithal Hourly Rates (ZHR) were computed with an
assumed population index of r=2, and a simple radiant
elevation correction, 1/sin(hR). Solar longitudes
refer to equinox J2000.0.
Rainer Arlt, 2006 Jan 8, 14h UT
www.imo.net 好象比较适合中国地区啊，你翻译一下！ 你说什么 我说你把
-------------------------------------
I M O S h o w e r C i r c u l a r
-------------------------------------
QUADRANTIDS 2006, visual observations
Visual observations of the 2006 Quadrantids received
by the IMO before January 8 were used to provide a
rough estimate of the 2006 activity of the meteor shower.
A total of 303 Quadrantids seen during 34 hours of
effective observing time were reported by 21 observers.
The maximum of the shower was lower than usual, with
a ZHR of about 85 near January 3, 23h-24h or a solar
longitude of 283.39 degrees (J2000.0). The expected
maximum would have occurred at 18h20 UT on January 3.
Only a single observer from Japan was able to report
his data for that time (first line in below table)
with a ZHR clearly below 100, too.
The number of individual observing periods is very small.
The shape of the activity profile depends on the sampling
of these data. The below table is not 'hand-picked' but
still it is a selected one out of three different compu-
ter-generated samplings. The selection is arbitrary;
we can find out what happened only more additional data.
If you have not yet sent your report, please do so.
-----------------------------------------------------
Jan (UT) Solarlong Nint NQUA ZHR lm
-----------------------------------------------------
03 19h00 283.1864 1 12 60.6 +- 16.8 5.40
03 20h10 283.2356 3 9 36.9 +- 11.7 5.42
03 22h00 283.3137 9 25 54.6 +- 10.7 5.62
03 23h00 283.3609 11 71 67.2 +- 7.9 5.56
03 23h40 283.3898 3 24 85.4 +- 17.1 5.74
04 02h30 283.5075 4 6 42.3 +- 16.0 4.72
04 03h10 283.5374 3 15 36.6 +- 9.2 5.33
-----------------------------------------------------
We are grateful to
Pierre Bader (Germany),
Rohit Belapurkar (India),
Sushrut Bhanushali (India),
Charuta Deshpande (India),
William Godley (USA),
Lew Gramer (USA),
Shy Halatzi (Israel),
Manali Kulkarni (India),
Omkar Kulkarni (India),
Rhishikesh Kulkarni (India),
Jens Lacorne (France),
Alastair McBeath (UK),
Tushar Purohit (India),
Pulin Raje (India),
Aaditya Ramdas (India),
Trupti Ranka (India),
Jurgen Rendtel (Germany),
Rahul Sangole (India),
Amit Shukrun (Israel),
Shigeo Uchiyama (Japan), and
Michel Vandeputte (Belgium)
for their quick submission of the observing reports.
The Zenithal Hourly Rates (ZHR) were computed with an
assumed population index of r=2, and a simple radiant
elevation correction, 1/sin(hR). Solar longitudes
refer to equinox J2000.0.
Rainer Arlt, 2006 Jan 8, 14h UT
翻译一下！ 自己翻译去。。。。。我不管 ^^ 自己翻译去。。。。。我不管你欺负人！ :evil: 我太忙了。。。。。 :twisted: 忙完了就来翻译！