(meteorobs) Optimized filters for daytime fireball video capture?
Ed Majden
epmajden at shaw.ca
Mon May 25 16:38:22 EDT 2009
Hi Thomas:
There are several lines contributing to Fe lines across the spectral
range, not just a single line. Singling out a single line would
reduce the brightness considerably so would be no help. I would ask
Chris about how to make an occulting disk for the Sun. He says this
is easy to accomplish so I would be interested on how to do this to.
I wonder how he accounts for the daily change in rising of the Sun
and the altitude for various seasons. If this is done you would need
some sort of program to do this and also reset the occulting disk
East after the Sun sets, and driving it as the Sun rises in the East.
Ed
On 25-May-09, at 1:22 PM, Thomas Ashcraft wrote:
> Hi Ed and all,
>
>
> I wonder if it is possible to isolate the specific spectrographic
> wavelength for burning ( or ionizing?) nickel-iron?
>
> Thomas
>
>
>
> Ed Majden wrote:
>> Hi Thomas:
>> I'm not sure if filters would be that effective. A meteor spectrum
>> produces emissions from around 340.0 nm (Violet) to around 900.0 nm
>> ( near ir red end). Selecting a narrow region at the red end will
>> reduce the output of total radiation produced by a fireball. If you
>> go to my web site located at: http://members.shaw.ca/epmajden/
>> index.htm and look at a spectrum signature you will see what I mean.
>> You need to reduce the intensity of the Sun first. I have read
>> somewhere that a driven occulting disk that blocks out the Sun and
>> tracks it across the sky could be used but this would be complicated
>> to do I would think. A red filter could be used in conjunction with
>> this occulting disk to reduce light scatter. During daylight you may
>> see a dust trail but this is in the visible region so a filter may
>> not be effective.. I wonder if one of our professional meteor types
>> could comment on this.
>> Ed Majden - EMO meteor spectroscopy
>> Courtenay, B.C.
>> Canada
>>
>> On 25-May-09, at 8:13 AM, Thomas Ashcraft wrote:
>>
>>
>>
>
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