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9月10号晚上,我发现了一颗非同寻常的SOHO彗星!

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福建ltycho 发表于 2007-9-13 15:13 | 显示全部楼层 来自: 中国–北京–北京 联通
哦,刚才没细看
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 楼主| 周波 发表于 2007-9-13 21:13 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网

Re: [comets-ml] C/1999 R1 = C/2003 R5 = 19?P

Hi all,

some updated information on the comet.

As of yet, there is no measured astrometry available for the comet. Karl Battams
promised to have it dealt with at high priority next week, so I am quite
confident that we will see the final confirmation of the identity soon. From a
comparison of available LASCO C3 images with the orbital elements, it seems as
if the comet is within only 4 hours of the predicted perihelion passage. This
seems to be quite close, even compared to long-known periodic comets.

Another interesting point is: Did the comet suffer from significant mass loss
since the last perihelion passage? As mentioned in the paper, the measured SOHO
brightness and evolution in 1999 and 2003 are very similar. This was confirmed
through private communication by people in France who are currently working on a
paper about SOHO non-Kreutz comet photometry. When looking at the 2007 passage,
the maximum brightness appears to be somewhere around 6.5 mag. This is about
what could be expected. So, it seems to be healthy.

Again, many thanks to everybody sending me congratulations on the list or
privately. It's quite a nice experience if such a venturesome prediction is
verified.

Regards,
Sebastian


>> Dear list,
>>
>> with pleasure I congratulate Sebastian for his successful prediction of the
>> identity of SOHO comets C/1999 R1 and C/2003 R5. His identification and
>> linkage was published in Astronomy & Astrophysics and a summary can be
>> accessed at
>> http://www.mpifr-bonn.mpg.de/sta ... Dateien/Page434.htm . The
>> paper is also available as an arXiv preprint.
>>
>> His original prediction for the perihelion passage in 2007 was Sep. 11.263
>> and the comet discovered yesterday by Bo Zhou seems to fit closely into this
>> prediction! What a fantastic achievement!
>>
>> I know that Sebastian has searched ground-based from his remote observatory
>> on Tahiti prior to perihelion but found nothing. He also published a revised
>> brightness prediction. The current perihelion passage may therefore be used
>> to set some lower/upper bounds for its brightness behaviour. I guess
>> Sebastian will give some details of the pre-perihelion searches he
>> conducted.
>>
>> Anyway, ONE SOHO-COMET LESS! The count has to be reduced by one.
>>
>> Again, a great acchievement and if I'd be responsible for the naming of
>> comets I'd call it SOHO-H鰊ig from now on!
>>
>> Cheers, Maik
>> --
>> If they give you ruled paper, write the other way. * Juan Ramon Jimenez
>> ________________________________________________________________________
>> maik@... http://www.comethunter.de
>> German Comet Section http://www.fg-kometen.de
>> http://groups.yahoo.com/group/comets-ml
>>
>>
>>
>>
>> Comet Observations List: http://groups.yahoo.com/group/CometObs/
>> Comet Images List: http://groups.yahoo.com/group/Comet-Images/
>>
>> NOTICE: Material quoted or re-posted from the Comets Mailing List should be
indicated
>> by:
>>
>> Comets Mailing List [date]
>> http://www.yahoogroups.com/group/comets-ml
>>
>> Yahoo! Groups Links
>>
>>
>>
>
>
>
> Comet Observations List: http://groups.yahoo.com/group/CometObs/
> Comet Images List: http://groups.yahoo.com/group/Comet-Images/
>
> NOTICE: Material quoted or re-posted from the Comets Mailing List should be
indicated by:
>
> Comets Mailing List [date]
> http://www.yahoogroups.com/group/comets-ml
>
> Yahoo! Groups Links
>
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 楼主| 周波 发表于 2007-9-13 21:37 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网
这颗彗星的最新C2和C3动画见:

http://www.mpifr-bonn.mpg.de/sta ... Dateien/Page434.htm
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 楼主| 周波 发表于 2007-9-14 13:23 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网

192?/P

RE: [sohohunter] Re: 192?/P


Parrish commented:

0618 722 438
0642 721 438
0742 719 438
0818 717 438
0842 716 438
0918 715 438
0942 714 438
1019 712 438
1042 709 438

"Strange that it seems to speed up? not sure if this a effect of
the sun but thats what I came up with."

It's just a perspective effect: direction of motion is changing
from being close to along the line of sight to transverse to it
as the comet curls around perihelion. --Rob
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 楼主| 周波 发表于 2007-9-16 09:21 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网
注意:
我这次发现的这颗SOHO彗星,应该是有“重要”意义的;
由于我本人不会英文,用翻译软件也看不太明白,因此,
还请会英文的朋友帮忙将上面的英文内容尽量多翻译些。
谢谢!
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 楼主| 周波 发表于 2007-9-17 11:15 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网

Latest News

Aug 17  Arkadiusz Kubczak reports a Kreutz group comet in real time C3 images
Aug 17  Shihong Yuan reports a Kreutz group comet in real time C3 images
Aug 18  Hua Su reports two Kreutz group comets in real time C3 images
Aug 20  Bo Zhou reports a Kreutz group comet in delayed C3 images from August 17
Aug 24  Gordon Garradd discovers faint comet 2007 Q1
Aug 26  Hua Su and Arkadiusz Kubczak report a Kreutz group comet in real time C3 images
Aug 28  Hua Su, Rainer Kracht and Shihong Yuan report a Kreutz group comet in real time C3 images
Aug 29  Shihong Yuan, John Sachs and Bo Zhou report a Kreutz group comet in real time C3 images
Aug 30  Alan Gilmore discovers faint periodic comet 2007 Q2
Aug 30  Faint comet 2007 Q3 discovered at Siding Spring
Sep 01  Hua Su reports a Kreutz group comet in real time C2 images
Sep 08  Hua Su reports a Kreutz group comet in real time C3 images
Sep 09  Bo Zhou reports a Kreutz group comet in real time C3 images
Sep 09  Steve Larson discovers faint periodic comet 2007 R1
Sep 10  Bo Zhou reports a Kracht group II comet in real time C2 images = 1999 R1 = 2003 R5
Sep 10  Masanori Uchina reports a Kreutz group comet in real time C3 images
Sep 12  A R Gibbs discovers faint periodic comet 2007 R2
Sep 13  Bo Zhou and Arkadiusz Kubczak report a Kreutz group comet in real time C3 images
Sep 14  Update
********************
http://www.ast.cam.ac.uk/~jds/
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 楼主| 周波 发表于 2007-9-18 02:26 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网

下面是国外同行在雅虎彗星邮件组上的发言(五)

Re: [comets-ml] C/1999 R1 = C/2003 R5 = 19?P


Dear Sebastian,

Sincerely congratulations for your great success! It is really one of
the most fantastic historical achievements! I hope an official IAUC or
MPEC will be issued soon.

I have written an article to introduce your prediction of this comet's
return in a Japanese magazine Hoshi-Navi issued on Sept. 5. I hope
some Japanese read it and came to be interested in this comet :-)

For further trials of observation of this comet, we would like to see
magnitude data of this comet.

Note, here is the light curve of this comet in 1999. But the magnitude
far from the perihelion was quite uncertain.

http://www.aerith.net/comet/catalog/1999R1/1999R1.html

Sebastian, would you show us the dates of your pre-prerihelion survey
with an upper limit of 17.5 mag?

Sebastian wrote that it was 6.5 mag at best in this return. Would you
tell us the time of the maximum brightness? The comet became brightest
about 0.17 days after the perihelion passage. Same behaviour also in
this return?

Best regards,

--
Seiichi Yoshida
comet@...
http://www.aerith.net/

**********************************
Re: [comets-ml] C/1999 R1 = C/2003 R5 = 19?P


Seiichi,

many thanks for your congratulations.

> For further trials of observation of this comet, we would like to see
> magnitude data of this comet.

Actually, Rainer Kracht did some preliminary photometric measurements which he
sent me some days ago. I hope he doesn't mind replicating them here in
abbreviated form:

11.34600 5.9 R
11.36266 5.6 R
11.40433 5.7 R
11.43067 5.5 R
11.44601 5.5 R
11.48767 5.5 R
11.52933 5.6 R
11.57101 5.7 R
11.59600 5.7 R
11.61267 5.8 R
11.63766 5.6 R
11.67933 5.8 R
11.69600 5.8 R
11.72101 6.0 R
11.73767 6.0 R

Unfortunately, I do not have any further information on the data, i.e.
catalogues used, calibration applied. I would guess, however, that they are not
calibrated, at least not against the sensistivity issues with the LASCO cameras.
Anyway, these values should indicate the actual brightness better than my
rough estimate.

Rainer made an interesting note: Apparently, the comet was not seen in the
STEREO-A data, although it should have been bright enough. While asteroids
(dominated by continuum light) are easily detected down to 10 mag, comets
(dominated by band emission) often escape detection in the STEREO-A COR2
instrument because their dominating spectral bands are not covered by the
filter. This indicates that 1999 R1 actually shows cometary activity, despite
not displaying a tail (and hardly a coma) in LASCO images.

Regards,
Sebastian

============================
http://tech.groups.yahoo.com/group/comets-ml/
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zhangmingth 发表于 2007-9-19 12:17 | 显示全部楼层 来自: 中国–湖北–武汉 电信
提示: 作者被禁止或删除 内容自动屏蔽
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 楼主| 周波 发表于 2007-9-19 21:24 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网

IAUC 8871 and 8872

Hi list,

IAUC 8871 and 8872 officially announce and confirm the identity of the SOHO
comet found by Bo Zhou on Sep. 10, 2007, with comets 1999 R1 and 2003 R5, as
predicted by Sebastian F. Hönig in 2005, and published in Astronomy and
Astrophysics <b>445</b>, 759 (2006). The linked orbit by B. G. Marsden,
based on only the C2 observations (with re-measured positions of the 1999,
and 2003 apparitions) indicate a perihelion date of Sep. 11.32, compared to
the prediction by H&ouml;nig of Sep. 11.26, which was thus only about 1.5
hours too early! M. Knight (University of Maryland), who has analysed the
brightness behaviour of this comet in all three apparitions remarks that the
lightcurves are more typical for a comet with several brightness peaks. The
evolution at all three apparitions is remarkably similar. It should also be
noted that the comet has not yet been detected in STEREO imagery, which is
typical for comets, where only bright ones are seen while minor planets can
be detected to a much fainter magnitude. The comet will most likely be
numbered 192P and the overall count of SOHO comets will be reduced by one.

Again congratulations to Sebastian!

Cheers, Maik
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 楼主| 周波 发表于 2007-9-23 02:57 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网

IAUC 8871

K. Battams, Naval Research Laboratory, informs us that B. Zhou
reported his detection of a member of the 'Kracht II comet group'
in SOHO-LASCO C2 data on Sept. 10; the object was immediately
confirmed by R. Kracht as showing 'Kracht-II' group motion.
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 楼主| 周波 发表于 2007-9-25 20:08 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网

Re: [comets-ml] C/1999 R1 = C/2003 R5 = 19?P

Re: [comets-ml] C/1999 R1 = C/2003 R5 = 19?P


Dear Sebastian and Rainer Kracht,

> Actually, Rainer Kracht did some preliminary photometric measurements which he
> sent me some days ago. I hope he doesn't mind replicating them here in
> abbreviated form:

Thank you very much for your informative measurements!

I updated my light curve based on the Rainer Kracht's measurements.
Here is the curve:

http://www.aerith.net/comet/catalog/0192P/2007.html

My formula is:

m1 = 27.8 + 5 log d + 17.5 log r(t - 0.17)

which suggests that the maximum brightness was delayed after the
perihelion passage by 0.17 days. This is quite consistent with the
light curve in 1999.

http://www.aerith.net/comet/catalog/0192P/1999R1.html

The current brightness is slightly brighter than 1999 (only by 0.3
mag). But this will be due to the magnitude system or reference
catalog.

So in general, we can say the comet completely keeps the same
brightness.

Best regards,

--
Seiichi Yoshida
comet@...
http://www.aerith.net/
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 楼主| 周波 发表于 2007-9-26 08:55 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网

"Astronomers Spot New 'Halley-like' Comet"--P/2007 R5

Astronomers Spot New 'Halley-Like' Comet
By Ker Than, Staff Writer

posted: 25 September 2007 02:50 pm ET

The Solar and Heliospheric Observatory (SOHO) has spotted an unusual comet that flies around the sun at regular intervals.
Dubbed P/2007 R5 (SOHO), the object belongs to a rare class of comets called periodic comets. Only 190 of the thousands of known comets are periodic. The most famous periodic comet is Halley's Comet, which can be seen from Earth every 76 years and last passed close to the sun in 1986.
While many of SOHO's 1,350 detected comets are suspected of being periodic, this is the first one conclusively proven and declared as such. The new comet has a much smaller orbit than Halley, taking only about four years to travel once around the sun. It was first seen in September 1999, and then again in September 2003. In 2005, Ph.D. student Sebastian Hoenig at the Max-Planck-Institute for Radioastronomy in Bonn, Germany, speculated the two comets were actually the same object.
Hoenig's realization is similar to the one made by English astronomer Edmond Halley, who in 1682 connected a comet he saw to two previous comets observed in 1531 and 1607.
To test his idea, Hoenig calculated a combined orbit for the comet and predicted it would return on Sept. 11, 2007. The comet appeared right on schedule.
P/2007 R5 (SOHO) is estimated to be about 330 to 650 feet (100 to 200 meters) in diameter. Unlike most comets, it does not have a tail or a glowing halo, called a coma, of dust and gas around its head. But as it passed within about 5 billion miles (7.9 million kilometers) of the sun, the comet brightened by a factor of a million-a common behavior for a comet.
"It is quite possibly an extinct comet nucleus of some kind," said Karl Battams, who runs SOHO's comet discovery program. Extinct comets are those that have expelled most of their volatile ice, leaving little material to form a tail or coma.
P/2007 R5 (SOHO) is expected to return in September 2011. SOHO is a joint mission run by NASA and the European Space Agency (ESA).

********************
http://www.livescience.com/space ... 925_soho_comet.html


                               
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 楼主| 周波 发表于 2007-9-26 08:57 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网

                               
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 楼主| 周波 发表于 2007-9-26 09:14 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网

下面是国外同行和专家在雅虎彗星邮件组上的发言(六)

Solar Maximum Mission (SMM) Coronagraph/Polarimeter (C/P) Data Avail

Hi all,

Doug Biesecker -- remember him? -- forwarded me the following
information. It won't be of interest to most of you but I know Rainer
has enjoyed playing with this sort of stuff before...

Cheers,
~~Karl


---------------------------------------------------------------------------
Solar Maximum Mission (SMM) Coronagraph/Polarimeter (C/P) Data
Available Online
---------------------------------------------------------------------------

All Solar Maximum Mission (SMM) Coronagraph/Polarimeter (C/P) data are
now available from the SMM C/P web site at:

http://smm.hao.ucar.edu

These same data are also available from the Mauna Loa web page:
http://mlso.hao.ucar.edu
The Virtual Solar-Terrestrial Observatory:
http://vsto.hao.ucar.edu
and will soon be available at the Virtual Solar Observatory:
http://umbra.nascom.nasa.gov/vso

The SMM Coronagraph obtained images of the corona in white light and
halpha from March through September of 1980 before suffering an
electronics failure that rendered it inoperative. The instrument was
repaired by the Challenger Space Shuttle (STS-41C) in April 1984 and
obtained images between June 1984 and November 1989 when it re-entered
the Earth's atmosphere. The SMM coronagraph obtained ~240,000 images
of the corona during its operation.
The SMM C/P recorded quadrants of the sun (north-east-south-west) in a
square field-of-view extending around the entire corona between 1.6
and 4.1 solar radii and out to 6.0 solar radii along the diagonals
(corresponding to the solar equator). Images were obtained at a
spatial resolution of 12 arcseconds in the wideband 'green' filter
(500 to 535 nm). Three polaroid filters were used for polarization
analysis of the observed radiation. Between 1980 and December 1986,
many of the orbital data sequences included images taken in the
neutral line of hydrogen known as halpha (654.3 to 658.3 nm).

The SMM home page provides all SMM Coronagraph images in fits and jpeg
formats, along with daily movies, synoptic maps, CME catalogues,
calibration information and a few IDL tools for using the data. This
work was completed through NASA grant LWS03-0161-0051.

If you would like additional information about these data please
contact: mlso_data_requests [at] ucar.edu

*****************************************
Re: [sohohunter] Solar Maximum Mission (SMM) Coronagraph/Polarimeter (C/P) Data Available Online


On 25 Sep 2007, at 18:46, karlbattams wrote:

> Hi all,
>
> Doug Biesecker -- remember him? -- forwarded me the following
> information. It won't be of interest to most of you but I know Rainer
> has enjoyed playing with this sort of stuff before...
>
> Cheers,
> ~~Karl
>
>
> ---------------------------------------------------------------------------
> Solar Maximum Mission (SMM) Coronagraph/Polarimeter (C/P) Data
> Available Online
> ---------------------------------------------------------------------------
>
> All Solar Maximum Mission (SMM) Coronagraph/Polarimeter (C/P) data are
> now available from the SMM C/P web site at:
>
> http://smm.hao.ucar.edu
>
Great! these images are essential to search for precursors of the
SOHO Marsden and Kracht group comets. They should be there!

But among the ~254,000 images they are not easy to find.

Regards,
Rainer

********************
RE: [sohohunter] Solar Maximum Mission (SMM) Coronagraph/Polarimeter (C/P) Data Available Online


Hi Karl,

Just out of curiosity, I checked images from August 24-28, 1987, to
see if I could find P/1999 R1 (I'm not sure of the exact predicted time
of perihelion passage but it should be within +/- a day of August 26th.
Unfortunately, I don't think the sensor is sensitive enough to see
objects this dim. I can easily see Aldebaran in most of the ww images
from August 24th, and Mars cutting across the top left corner of
the ww image sequence on the 26th, but that's it for dates near
predicted perihelion passage. --Rob

-----Original Message-----
From:
sentto-6635867-2439-1190746011-matsonr=saic.com@...
[mailto:sentto-6635867-2439-1190746011-matsonr=saic.com@...
ahoo.com] On Behalf Of karlbattams
Sent: Tuesday, September 25, 2007 11:47 AM
To: sohohunter@yahoogroups.com
Subject: [sohohunter] Solar Maximum Mission (SMM)
Coronagraph/Polarimeter (C/P) Data Available Online

Hi all,

Doug Biesecker -- remember him? -- forwarded me the following
information. It won't be of interest to most of you but I know Rainer
has enjoyed playing with this sort of stuff before...

Cheers,
~~Karl


------------------------------------------------------------------------
---
Solar Maximum Mission (SMM) Coronagraph/Polarimeter (C/P) Data
Available Online
------------------------------------------------------------------------
---

All Solar Maximum Mission (SMM) Coronagraph/Polarimeter (C/P) data are
now available from the SMM C/P web site at:

http://smm.hao.ucar.edu

These same data are also available from the Mauna Loa web page:
http://mlso.hao.ucar.edu
The Virtual Solar-Terrestrial Observatory:
http://vsto.hao.ucar.edu
and will soon be available at the Virtual Solar Observatory:
http://umbra.nascom.nasa.gov/vso

The SMM Coronagraph obtained images of the corona in white light and
halpha from March through September of 1980 before suffering an
electronics failure that rendered it inoperative. The instrument was
repaired by the Challenger Space Shuttle (STS-41C) in April 1984 and
obtained images between June 1984 and November 1989 when it re-entered
the Earth's atmosphere. The SMM coronagraph obtained ~240,000 images of
the corona during its operation.
The SMM C/P recorded quadrants of the sun (north-east-south-west) in a
square field-of-view extending around the entire corona between 1.6 and
4.1 solar radii and out to 6.0 solar radii along the diagonals
(corresponding to the solar equator). Images were obtained at a spatial
resolution of 12 arcseconds in the wideband 'green' filter (500 to 535
nm). Three polaroid filters were used for polarization analysis of the
observed radiation. Between 1980 and December 1986, many of the orbital
data sequences included images taken in the neutral line of hydrogen
known as halpha (654.3 to 658.3 nm).

The SMM home page provides all SMM Coronagraph images in fits and jpeg
formats, along with daily movies, synoptic maps, CME catalogues,
calibration information and a few IDL tools for using the data. This
work was completed through NASA grant LWS03-0161-0051.

If you would like additional information about these data please
contact: mlso_data_requests [at] ucar.edu

*************************************
RE: [sohohunter] Solar Maximum Mission (SMM) Coronagraph/Polarimeter (C/P) Data Available Online


On 25 Sep 2007, at 13:24, Matson, Robert D. wrote:

> Hi Karl,
>
> Just out of curiosity, I checked images from August 24-28, 1987, to
> see if I could find P/1999 R1 (I'm not sure of the exact predicted time
> of perihelion passage but it should be within +/- a day of August 26th.
> Unfortunately, I don't think the sensor is sensitive enough to see
> objects this dim. I can easily see Aldebaran in most of the ww images
> from August 24th, and Mars cutting across the top left corner of
> the ww image sequence on the 26th, but that's it for dates near
> predicted perihelion passage. --Rob
>

I have seen most of the gif images and have found three of Jupiters
moons and stars to mag 6. There should be enough sensitivity.

I think that P/1999 R1 was outside the small field of view in August
1987. The SMM FOV is smaller than the C2 FOV. The path of the comet
is outside of the C2 FOV in Mid-August.

Regards,
Rainer
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 楼主| 周波 发表于 2007-9-26 09:21 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网

下面是国外同行和专家在雅虎彗星邮件组上的发言(七)

Solar Maximum Mission (SMM) Coronagraph/Polarimeter (C/P) Data Avail

SMM sensitivity


Hi All,

Curious about the sensitivity of SMM, I searched forward a few more days
to check if rho Leonis (m +3.8) was visible on August 30, 1987 -- it
was.
So it's at least as sensitive as m4. --Rob

**********************************
SMM sensitivity at least +4.6


Just found chi Leonis (+4.6) in September 6, 1987 imagery (only 2
frames, but it's there). How bright do we think P/1999 R1 was on
its three known perihelion passages? With some fits file processing,
it may be possible to pull it out of the SMM images... --Rob

*************************
[Fwd: Re: [sohohunter] P/1999 R1 in 1987]

> Then, it fades rather
> quickly, approximately 0.5-1mag per hour.

Well, this was too pessimistic (didn't remember correctly). From a quick check
with the light curve, I find that 1 mag decreas in brightness corresponds to
~0.35 days (= 8 hours).

Hope this helps,

Sebastian
================
http://tech.groups.yahoo.com/group/sohohunter/messages/2438?l=1
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 楼主| 周波 发表于 2007-9-26 09:27 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网

下面是国外同行和专家在雅虎彗星邮件组上的发言(八)

Solar Maximum Mission (SMM) Coronagraph/Polarimeter (C/P) Data Avail
*********************************************************
P/1999 R1 in 1987


Hi Rainer,

> I have seen most of the gif images and have found three of Jupiters
> moons and stars to mag 6. There should be enough sensitivity.

Well, that's promising -- and indeed I've now managed to find a
5th magnitude star.

> I think that P/1999 R1 was outside the small field of view in
> August 1987. The SMM FOV is smaller than the C2 FOV. The path of
> the comet is outside of the C2 FOV in Mid-August.

I show it a little more than 3-1/2 solar diameters away at perihelion
on 8/26/1987, which as you point out is definitely outside the FOV
of SMM. I'm not sure how quickly this comet fades after perihelion,
but if it could hold on for 5 more hours, it pulls to within two solar
diameters. --Rob
*********************
Re: [sohohunter] P/1999 R1 in 1987


On 25 Sep 2007, at 14:39, Matson, Robert D. wrote:

> Hi Rainer,
>
> > I have seen most of the gif images and have found three of Jupiters
> > moons and stars to mag 6. There should be enough sensitivity.
>
> Well, that's promising -- and indeed I've now managed to find a
> 5th magnitude star.
>
> > I think that P/1999 R1 was outside the small field of view in
> > August 1987. The SMM FOV is smaller than the C2 FOV. The path of
> > the comet is outside of the C2 FOV in Mid-August.
>
> I show it a little more than 3-1/2 solar diameters away at perihelion
> on 8/26/1987, which as you point out is definitely outside the FOV
> of SMM. I'm not sure how quickly this comet fades after perihelion,
> but if it could hold on for 5 more hours, it pulls to within two solar
> diameters. --Rob
>
>
Actually, the perihelion time of P/1999 R1 in 1987 was even more
unfavourable: integrating the orbit from MPEC 2007-S16 to 1987
with SOLEX, I find T = 1987 August 17 (not late August).

I have made a page with my early SMM experiences;
http://www.rkracht.de/smm/smmcp.htm

Rainer
***************
Re: [sohohunter] P/1999 R1 in 1987


Hi Rob,

> of SMM. I'm not sure how quickly this comet fades after perihelion,
> but if it could hold on for 5 more hours, it pulls to within two solar
> diameters. --Rob

The peak brightness is approximately 4 hours after perihelion (note: perihelion
is not equal to the max. elongation!). Then, it fades rather quickly,
approximately 0.5-1mag per hour.

Cheers,
Sebastian
**********
[Fwd: Re: [sohohunter] P/1999 R1 in 1987]

> Then, it fades rather
> quickly, approximately 0.5-1mag per hour.

Well, this was too pessimistic (didn't remember correctly). From a quick check
with the light curve, I find that 1 mag decreas in brightness corresponds to
~0.35 days (= 8 hours).

Hope this helps,

Sebastian
***************
RE: [sohohunter] P/1999 R1 in 1987


Hi Rainer,

> Actually, the perihelion time of P/1999 R1 in 1987 was even more
> unfavourable: integrating the orbit from MPEC 2007-S16 to 1987 with
> SOLEX, I find T = 1987 August 17 (not late August).

Even so, the portion after perihelion does intersect the field of view.
However, I did not find it -- at least in my scanning of the jpegs from
8/12 to the end of the month. (I was able to easily see stars of +5.3
and +5.4, so I would think I could have pulled out +6 if it was in the
FOV.) If I had a fairly confident perihelion date with some error bars,
I'd be willing to dig into the fits files to see if I could go a bit
deeper with additional processing.

> I have made a page with my early SMM experiences;
> http://www.rkracht.de/smm/smmcp.htm

Very nice! A little web-searching reveals that SMM has been credited
with 10 sungrazing comet discoveries. The first, SMM-1, is quite bright
and clearly visible in the last two ss images of 10/5/1997. Even
brighter is SMM-2, visible in the last three ss images of 10/17/1997.
Both of these were Kreutz comets.

--Rob
*****************
RE: [sohohunter] P/1999 R1 in 1987


On 25 Sep 2007, at 15:38, Matson, Robert D. wrote:

> Hi Rainer,
>
> > Actually, the perihelion time of P/1999 R1 in 1987 was even more
> > unfavourable: integrating the orbit from MPEC 2007-S16 to 1987 with
> > SOLEX, I find T = 1987 August 17 (not late August).
>
> Even so, the portion after perihelion does intersect the field of view.
> However, I did not find it -- at least in my scanning of the jpegs from
> 8/12 to the end of the month. (I was able to easily see stars of +5.3
> and +5.4, so I would think I could have pulled out +6 if it was in the
> FOV.) If I had a fairly confident perihelion date with some error bars,
> I'd be willing to dig into the fits files to see if I could go a bit
> deeper with additional processing.
>
> > I have made a page with my early SMM experiences;
> > http://www.rkracht.de/smm/smmcp.htm
>
> Very nice! A little web-searching reveals that SMM has been credited
> with 10 sungrazing comet discoveries. The first, SMM-1, is quite bright
> and clearly visible in the last two ss images of 10/5/1997. Even
> brighter is SMM-2, visible in the last three ss images of 10/17/1997.
> Both of these were Kreutz comets.
>
> --Rob
>
I have added the first four SMM (Kreutz) comets to the page.

Rainer
*************
Re: [sohohunter] P/1999 R1 in 1987


Rob,

> Even so, the portion after perihelion does intersect the field of view.
> However, I did not find it -- at least in my scanning of the jpegs from
> 8/12 to the end of the month. (I was able to easily see stars of +5.3
> and +5.4, so I would think I could have pulled out +6 if it was in the
> FOV.) If I had a fairly confident perihelion date with some error bars,
> I'd be willing to dig into the fits files to see if I could go a bit
> deeper with additional processing.

You might try the following:

TP = 1987 Aug. 22.61
q = 0.0596
e = 0.97642
i = 13.47
Peri = 40.14
Node = 8.60
a = 2.52927
P = 4.02

Sebastian
***************
Re: [sohohunter] P/1999 R1 in 1987


Ah, it's too late. I should go to bed...

> TP = 1987 Aug. 22.61

Should read: TP = 1987 Aug. 21.75

Sebastian
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小龙·哈勃 发表于 2007-9-26 15:45 | 显示全部楼层 来自: 中国–广东–广州–番禺区 电信
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 楼主| 周波 发表于 2007-9-26 18:16 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网

谢谢!要是能再用中文说上两句就好了。

奇怪!都半个多月时间了,这个专家(KB)怎么还不在报告页上发“正式”公告呀!
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小龙·哈勃 发表于 2007-9-26 22:17 | 显示全部楼层 来自: 中国–广东–广州–番禺区 电信
Notes for editors:

The credit for discovery and recovery of the object goes to Terry Lovejoy (Australia, 1999), Kazimieras Cernis (Lithuania, 2003) and Bo Zhou (China, 2007).
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 楼主| 周波 发表于 2007-9-27 00:53 | 显示全部楼层 来自: 中国–陕西–咸阳 广电网

P/2007 R5 (SOHO)

Hi all,

according to the linked orbit by S. Nakano at

http://www.oaa.gr.jp/~oaacs/nk/nk1537.htm

this comet will approach Earth in

2035 at 0.27 AU
2038 at 0.19 AU
2043 at 0.30 AU

Maybe then earthbound observation will finally be successful.

30 years to go...

Cheers, Maik
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