Impact of telescope height on the seeing
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Impact of telescope height on the seeing
Dear all,
Some time ago, I tried to measure the impact of the height of the telescope on the seeing. I compare the seeing at ground level and 1 m high.
Since I had only one SSM, the measurements at 0 m and 1 m where not simulaneous. Still some impacts are clearly visible:
Last August, Karine Chevalier carried out measurements at St Veran using two SSM. The seeing was measured simultaneously at 1 m and 1.5 m high, which is typical of telescope aperture heigths.
The ground at St Véran is made of rocks with no grass. The mesurements were made over a period of time of more than one hour.
Karine, whom I thank for, made the measurements and the data reduction. Here are the results :
This graphic gives the % of time below a given value of seeing :
The table is another way to present these results :
In a nutshell, it means that going from 1 m to 1.5 m high improves the seeing by about 0.35 arcsec, which is ... quite significant.
In high resolution imaging, we typically keep less than 5% of the frames. We can see on the table that the quantile 5% goes from 0.7 to 0.3 arcsec when the aperture of the instrument rises from 1 m to 1.5 m high.
So now, we all have to use tall tripods :-)
PS : of course, all of this depends on wind speed, ground nature, hour in the day, etc.
Best regards
Christian
Some time ago, I tried to measure the impact of the height of the telescope on the seeing. I compare the seeing at ground level and 1 m high.
Since I had only one SSM, the measurements at 0 m and 1 m where not simulaneous. Still some impacts are clearly visible:
Last August, Karine Chevalier carried out measurements at St Veran using two SSM. The seeing was measured simultaneously at 1 m and 1.5 m high, which is typical of telescope aperture heigths.
The ground at St Véran is made of rocks with no grass. The mesurements were made over a period of time of more than one hour.
Karine, whom I thank for, made the measurements and the data reduction. Here are the results :
This graphic gives the % of time below a given value of seeing :
The table is another way to present these results :
In a nutshell, it means that going from 1 m to 1.5 m high improves the seeing by about 0.35 arcsec, which is ... quite significant.
In high resolution imaging, we typically keep less than 5% of the frames. We can see on the table that the quantile 5% goes from 0.7 to 0.3 arcsec when the aperture of the instrument rises from 1 m to 1.5 m high.
So now, we all have to use tall tripods :-)
PS : of course, all of this depends on wind speed, ground nature, hour in the day, etc.
Best regards
Christian
Christian Viladrich
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Re: Impact of telescope height on the seeing
Very interesting Christian. I suppose height is relative to the ground on which the telescope rests, irrespective if the ground is at sea level or 2000 m a.s.l., am I right ? (anyway I would expect a generally better seeing at 2000 m...)
Raf
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Re: Impact of telescope height on the seeing
Yes indeed, this is the height relative to the ground.
Christian Viladrich
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Re: Impact of telescope height on the seeing
Great to know, Christian. Thank you for sharing this with all of us.
Franco
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Re: Impact of telescope height on the seeing
Interesting stuff, I imagine it is different for different thickness optics and different types of ground (field of soil & grass, compared to desert or straight rocks, sedimentary soil versus hot quartz sand, etc).
I keep my instruments up on a pier, fairly high up, and my decking in the observatory is over the soil.
I wonder if it would matter for those using tripods, if they put a thermal barrier (like covers used to block solar) on the ground under the telescope's aperture/mirror?
Very best,
I keep my instruments up on a pier, fairly high up, and my decking in the observatory is over the soil.
I wonder if it would matter for those using tripods, if they put a thermal barrier (like covers used to block solar) on the ground under the telescope's aperture/mirror?
Very best,
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Re: Impact of telescope height on the seeing
At home, I observe on a ground covered by grass, and I spray water on the grass during observation.
Christian Viladrich
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Re: Impact of telescope height on the seeing
Christian:
Very interesting information, my Mexico City home observatory is 2246 meters above mean sea level, the rural observatory is at 2265 meters above mean sea level.
So I don´t need a high pier. , but in the City the problem is air contamination, at the rural place I have a very even and clean seeing.
Best regards,
Eric.
Very interesting information, my Mexico City home observatory is 2246 meters above mean sea level, the rural observatory is at 2265 meters above mean sea level.
So I don´t need a high pier. , but in the City the problem is air contamination, at the rural place I have a very even and clean seeing.
Best regards,
Eric.
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Re: Impact of telescope height on the seeing
Very interesting! however I am barely tall enough to mount my telescope at 1m
Alexandra
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Re: Impact of telescope height on the seeing
Excellent clear results and presentation, thanks
Robert
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Re: Impact of telescope height on the seeing
Excellent and informative as always Christian!
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Re: Impact of telescope height on the seeing
We all know well about british grass lawns!
My SCT scopes are about 1,2 - 1,6m elevation (entrance aperture) above a grassy lawn level.
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Re: Impact of telescope height on the seeing
Great stuff Christian. My mount is over 2m in height but it is inside the dome...
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Re: Impact of telescope height on the seeing
Very interesting results and very well presented.
What do you feel might explain that much difference? Dust in the air layer just above the ground or perhaps some other form of scattering phenomenon? Thermal currents close to the ground?
Bruce G
What do you feel might explain that much difference? Dust in the air layer just above the ground or perhaps some other form of scattering phenomenon? Thermal currents close to the ground?
Bruce G
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Re: Impact of telescope height on the seeing
I'll give this a few more days here then move over to the library folks, I think is a useful thread for reference.
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Re: Impact of telescope height on the seeing
Hello Bruce,
We used two AiryLab SSM.
We also started a session with three SSM running at 1, 1.5 and 2 m high, but this session was quickly clouded.
The inhomogeneities of the air in the boundery layer depens on the wind speed, type and temperature of the ground.
I am planning to make some tests at home in order to check whether there is a general pattern or not.
We used two AiryLab SSM.
We also started a session with three SSM running at 1, 1.5 and 2 m high, but this session was quickly clouded.
The inhomogeneities of the air in the boundery layer depens on the wind speed, type and temperature of the ground.
I am planning to make some tests at home in order to check whether there is a general pattern or not.
Christian Viladrich
Co-author of "Planetary Astronomy"
http://planetary-astronomy.com/
Editor of "Solar Astronomy"
http://www.astronomiesolaire.com/
Co-author of "Planetary Astronomy"
http://planetary-astronomy.com/
Editor of "Solar Astronomy"
http://www.astronomiesolaire.com/
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Re: Impact of telescope height on the seeing
Those interested in this topic may wish to check out the following document:
THE EFFECT OF THE LOCAL ATMOSPHERIC ENVIRONMENT ON ASTRONOMICAL OBSERVATIONS
http://www.eso.org/gen-fac/pubs/astclim ... node1.html
In particular, note the following page
Surface layer seeing
http://www.eso.org/gen-fac/pubs/astclim ... ode75.html
This work is largely derived from the author's experience on the design and engineering of the ESO Very Large Telescope (VLT) observatory between 1984 and 1993. Thus, the focus is on large telescopes, not amateur, but the effect being studied is the same.
The Hypertext version is here: http://www.eso.org/gen-fac/pubs/astclim ... hesis.html
Note that the Hypertext version, while conveniently indexed, may be missing some figures
THE EFFECT OF THE LOCAL ATMOSPHERIC ENVIRONMENT ON ASTRONOMICAL OBSERVATIONS
http://www.eso.org/gen-fac/pubs/astclim ... node1.html
In particular, note the following page
Surface layer seeing
http://www.eso.org/gen-fac/pubs/astclim ... ode75.html
This work is largely derived from the author's experience on the design and engineering of the ESO Very Large Telescope (VLT) observatory between 1984 and 1993. Thus, the focus is on large telescopes, not amateur, but the effect being studied is the same.
The Hypertext version is here: http://www.eso.org/gen-fac/pubs/astclim ... hesis.html
Note that the Hypertext version, while conveniently indexed, may be missing some figures