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Hi,
Thanks, I initially wondered if this effect is what I have picked up in the more unusual spectra that show changes towards the end of flight.
…but perhaps not…I’ve been doing some crude velocity measurements and the separating part is travelling at more or less the same velocity (until burn out) as the pre separating meteor trail. So it looks like the meteoroid “sheds” some material, perhaps volatiles reaching a critical temperature and then taking some portion meteorid with it giving the little “puff” of stuff.
A spectrum would have been nice but it’s really nice to catch a new meteor ablation effect (unless anyone else has recorded it before…)
cheers,
Bill.
The fading meteors continue to be captured…
Got this last week. https://www.youtube.com/watch?v=YrxxiWbe40Q
First time I’ve seen this effect, most unusual.
cheers,
Bill.
Had some really nice results recently. Got this nicely detailed spectrum a few nights ago. This one has strong O lines at 557.7nm and 615.6nm as well as several Si+ lines indicating a fairly speedy meteor!
It is worth remembering that the colouration is wavelength stretched and false, the spectrum actually spans from ~370nm to 780nm so, rather sadly, you’d never see it look so nice…
cheers,
Bill.
Remarkable instruments, and, I suppose as an opto mechanical engineer myself I am highly biased but it demostrates clearly that whilst theoreticians may theorise, engineers make it happen! 😉
cheers,
Bill.
Hi,
Another interesting capture. Very complex with dispersion ~.5nm/pix. With the efforts of Alex and William of the Nemetode group it’s been tentatively identified as an October Camelopardalid.
The green magnesium line is very broad. Maybe seen as resolved if it hadn’t bloated as the terminal flare saturated.
Some broad similarities between this spectrum and the one in Post #41. Many Fe lines!
cheers,
Bill.
Hi,
Here’s the light curve from meteor 20160924_232416 (and a spectrum). Light curve shows the distinct shape as illustrated in previous postings. Now just need more spectra to see if what the compositional traits are (orbits would be nice to see of it’s fluffy cometary stuff…)
Here’s the capture image that shows the zero order image plus weak spectrum.
…and the smoothed light curve with the distinctive looking tail off like the other example.
…also the spectra again, just in case…
it’s all good stuff… 😉
cheers,
Bill.
Hi All,
Been getting some interesting results recently but the other night I got a spectrum on 3 cameras of the same meteor! Only two were useable and even these were quite noisy. Meteor was maybe mag 0 – -1. (This might be more properly placed on the “Fading meteor” thread but as its about spectra… 😉 )
HOWEVER, this (or these) are the first spectrum I’ve got from a “melting” meteor. This one, like to others just faded out.
The graphs are very similar (as one would expect) but a few differences creep in from different resolution and processing artifacts.
The first graph is from a system with a 830l/mm grating.
…and this from a 600l/mm grating.
Careful review of the video reveals many of the lines are real but it is interetsing to note a large fraction are artifacts. I don’t know if the spectrum actually tell us anything new yet, but it’s a step on the way.
Need to graph the light curve now for the other forum thread…
Cheers,
Bill.
Hi,
The Perseids have been a washout both metaphorically and literally. A ton of rain came down on Thursday night.
However ever the optimist I watched the skies closely and after 48 hours of cloud and rain there was a mysterious clearance for around 20 minutes last night. Rain stopped, wind dropped to near zero and the sky cleared. So I deployed my camera rigs as quickly as possible and I managed to capture a few meteors and one spectrum. Unfortunately the spectrum was contaminated by both scattered light and some in frame clouds. However if was well dispersed and showed some really nice detail at the red end.
The direction indicated it was a perseid fireball but the spectrum had the tell-tale emission at 557.7nm typical of high speed meteors. What was interesting about this one was the detail in the atmospheric bands. Perseids are high speed meteors and they carry a lot of energy. This energy is available for excitation as the meteors kinetic energy is transformed into heat.
Slight diversion… in 2002 astronomers at the VLT caught a spectrum by chance using the FORS1 spectrograph. After removing the redshifted lines of the supernova the remaining lines were of the atmospheric emissions of O, O2, N, N2.
As this was a highly accurate instrument the line measurements are invaluable for calibrating meteor spectrum. I thought it would be interesting to compare the results of a multi-million euro instrument against my 500 quid system…
VLT spectrum sections are in black. The modeling done by the astronomers indicates this is the profile of an emission of 4200K at a height of 95km.
As the devil is in the detail if you look closely at the model line (at around 755nm from O2) it is missing from the VLT observation but it is a distinct line in my spectrum. Another cool aspect is the “height” of the lines in the regions marked. Comparing the various scalings shows a very good ratio relation. So it would suggest that my real spectrum matches the modelling quite well. 4200K it is!
Not too terrible at all… 😉
cheers,
Bill.
Hi,
Thanks, Unfortunately the zero order fell outside my fov because David Anderson did catch it also. It was a really nice sporadic.
Here is Davids picture.
It would have been nice, I was very pleased with it for a first order spectrum. The dispersion was almost perfect at ~0.9nm/pix (a rare occurence with meteor spectroscopy!) and the effective resolution was ~1.9nm/pix fwhm on the blue/green irons lines. The multi station, multi technique data is slowly building up, we’ll get plenty more with the additional spectro stations now,
cheers,
Bill.
Hi,
After the long twilights it was back to the spectro action last night!
Fortune gave me a very bright spectrum this morning. Both good dispersion and good resolution.
Many iron lines with a strong sodium line so very probably a stony iron meteoroid. However doing a instrument flux correction shows the “true” brightness of the blue iron lines.
The video was quite interesting because the sodium line was very prominent on it’s own for a significant proportion of the meteors duration before the other lines lit up.
cheers,
Bill.
Hi,
The remarkable spectrum of post #35 has become even more remarkable after attending a presentation by the meteor spectroscopy expert Jiri Borovicka at the International Meteor Conference in the Netherlands a few days ago. (A wonderful event I can recommend!)
The reason that I couldn’t identify many of the lines is that they are not atomic lines. Atomic lines are the only ones I have in the software databases I use but the lines visible are actually compounds! They are probably mostly emissions from oxides such as aluminum oxide. This makes it an even more unusal meteor.
Good stuff!
cheers,
Bill.
Hi,
The dim images MIGHT be being caused by the level sttings. Firstly let me disclaim by saying I’ve never used a 902H camera for meteor observing. However I have experienced a similar problem in a more professional capacity when I thought I ought to be seeing brighter images than I was.
Before proceeding does the 902H have a small adjuster screw any where? If so, as in my own case, have the camera on and in a fairly dim setting, ALC low, then slowly (and gently, these little pots aren’t meant to be tweaked too many times) adjust the control screw. The level control adjusts the feedback to the iris and if it’s not set properly even in dark dark conditions the iris may not fully open. (resulting in dim images). If this is the same on the 902H then at some point the iris will open fully irrespective of the illumination and you should see a much brighter image. Once you’ve found when it opens the iris take the pot to the end stop in the same direction. This should in effect keep the iris open under all conditions.
I’d use AGC low all the time if the above works, AGC high can be VERY noisy with a fully open IRIS.
Also I’d try “shutter” OFF first. This is related, usually, to the auto shutter settings. On some cameras this shutter really means the electronic exposure. OFF normally defaults to the longest exposure. To test this try it in day light and very quickly it will become apparent if this is the case as the image will saturate out because the shutter speed will not increase.
Hope this helps,
cheers,
Bill.
PS Also, some video capture cards seem to automatically produce fairly dim images. You may also need to adjust Brightness/Contrast/Gain on the video control panel. I had two dreadful Hauppauge boards that had this problem, every single power up they had to be adjusted. Thay are now in the bin! I’d try sorting the camera first though….
Hi,
I found a filter for 850nm (16nm fwhm) which happens to be very close to the emission wavelength of the Ca II IR triplet, however the image is much more bland at 850 due to less scattering and the fact that the telescope optics have less than half the resolution at this wavelength cf 390nm. (The Ca II IR triplet is used in spectrohelioscopes for photopolarimetry. The family of UV and IR transitions are quite interesting…)
Even a casual inspection reveals the limb just looks brighter, so doing the very same thing as before gave this graph…
Which indeed does have a slightly less steep gradient than the 350nm image. The edge has a brightness of around 56% of the centre.
This was all done with “auto everything” on, with the camera and software so I’m not sure how absolutely accurate the measurements are photometrically but it makes sense, which is kinda re-assuring… 😉
On doing a bit more digging, this continues for some ways until the very shortest radio wave wavelengths are reached when there is a transition to limb brightening!
cheers,
Bill.
Hi,
A lot of books describe the limb darkening but I’ve never seen it actually plotted. So I thought it might be fun to see what it looks like. Since the images were taken through a deep blue filter the darkening should be more here than at longer wavelengths. Since the shorter wavelengths scatter more. (Might be interesting to try this as different wavelengths to see if the theory matches the observations…)
At the edge the value of pixels is 37.5% of the centre.
Fascinating!
cheers,
Bill.
Hi,
The spot that I imaged on the limb a few days ago has turned out to be the classic sunspot…
Image is a stack of 100 images processed in Registax 6. Taken 15.47UT today 21/5/16. Hopefully get a few more shots tomorrow if the weather cooperates.
A bit of pixel counting yields a spot diameter of around 47600km, ~3.7 times the diameter of the Earth.
… the Earth would sit nicely within the umbra!
Cheers,
Bill.
Hi Andy,
Thanks, but its all in the image processing… 😉
I am quite please with how it’s performed though. Certainly planning on keeping it in place for a while.
The single spot image shows the Wilson effect quite nicely but I think I went a little overboard with the wavelet processing with the faculae image, it’s a bit “speckley”.
Although not as narrow as a proper Ca filter I am quite impressed that it can show the faculae well and possibly some of the super granulation of the chromospheric network.
It’s quite a paradox that I’ve got virtually nothing when I’ve actually tried it on the comets I’ve been able to see but it turns out to be great for solar observing!
cheers,
Bill.
Another sunny day!
So another test session with the 390nm filter…
Gorgeous faculae. (Note image is of w limb but rotated by 90 degrees.)
and a nice big spot coming round the limb…
cheers,
Bill.
Hi,
Wall to wall sunshine and 24C, I could hardly believe it!
Here are a couple of images I took in the evening.
after so many washouts over the years nice to finally see one end to end.
cheers,
Bill.
Hi,
Normally I don’t do the correction as theres not that much to be gained data wise at these resolutuions. However this time the size of the Mg line was immense.
I wanted to see if it would still be “higher” than the other metal lines in the blue after correction. Mostly this isn’t the case as a lot of the emissions from the meteors are in the blue but look faint due to the sensitivty issues discussed further back. I just divided the whole spectrum by a Vega spectrum and lo and behold the big Mg line was still the highest peaking line. This meteor may have looked pretty green if it had been seen visually.
cheers,
Bill.
Hi,
That’s a terrific piece of work. A dramatic demonstration of stellar spectroscopy.
You mention the long exposures, working at mag +13 what length were they? I’ve built several fairly crude spectroscopes over the years but I was drooling over the multitude of very neat commercial devices that were on show at the Astrofest! I’m tempted to put one on my C9.25….
cheers,
Bill.
