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Re: (meteorobs) Visual magnitude
> Sirko mentioned:
> >If I recall it correct I read somewhere, that the luminous trail of a
> >meteor has an actual diameter in the order of 1m. Don't ask me *where*
> >this information came from, I think it was a result of some photographic
> >investigation. It means that the apparent width of a meteor's trail should
> >be of the order of a few arc seconds.
My recollection was of a larger figure in the tens of metres, perhaps
given by Keith Hindley verbally or in an old BAA Meteor Section
Newsletter or perhaps in a paper by Baggeley. This figure might be
for bright visual meteors. It also surely depends on the velocity,
height, the meteoroid's `crumbliness', and other factors. A quick
trawl through some Czech papers just now turned up a few potential
papers, but it's too late at night here to wade through papers that
take a page just to list the meanings of the symbols used in the
equations. Can anyone provide a freindly reference?
> I'm surprised at the 1 arcminute width for trails. (Also, I wasn't sure how this
> resulted in apparent widths on the order of arcseconds, Sirko?) I perceive trail
> widths fairly clearly in two dimensions, especially for brighter meteors, and
> I'm pretty sure that images subtending 1 arcmin or less wouldn't give my eye
> this impression. Could I be witnessing some sort of optical "blooming" effect in
> my eye, rather than actual meteor trail width?
I think Sirko was talking about 1 metre (meter in American (-:) when
he wrote 1m. One arcminute approximately corresponds to about 30
metres in the meteor layer. So 1 metre subtends about 2 arcsec.
As far as widths go, the visual meteors seen telescopically appear to
have width, but I don't recall seeing anything appear wider than the
moon (31'/19.5x), and most are sub-arcminute. Some of this width is
attributable to the train, which you can see expanding and drifting
almost immediately following the meteor. Typical telescopic meteors
that I observe don't exhibit a pronounced width.
Malcolm
References: