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(meteorobs) pb of population index definition



Hello you all !

I have a simple question, dealing with a problem of population index determination :

In "Meteors showers and their observations", NAMN Guide, chapter 7, we find :
"r is a value indicating how many more times meteors of magnitude m+1 appear than meteors of magnitude m. [..] Example : m=4, r=3 => tree times as many meteors of magnitude 5 appear than meteors of magnitude 4".

I conclude : r = n(m+1) / n(m),
where n(m) is the number of meteors of magnitude m. I call this method method 1

On the other hand, in "The Perseid meteoroid stream : characterization odf recent ectivity from visual observations", Brown & Rendtel, Icarus, 124, 414-428, 1996, we can read :
"r=N(m+1)/N(m),
where N(m) is the TOTAL bumber of meteors of magnitude m OR LESS."
Whith this definition, we have :
N(m) = sum(n(m)), with m < smallest magnitude sawn
and r = N(m+1) / N(m)
I call this method method 2.

These 2 definitions are completely different and lead to different value of r.

Now, lets take a concreate example :

In "Comparison between Leonid meteor shower observation during 1998-200", PSS, 50, 379-384 (2002), table 2 : lets try to compute r just from the first line :
m      =   4.5    0.5    -3.2
n(m) =    33     10       10

value of r = 1.76

Now the question is : where does this value 1.76 come from ? Is it an average value ? I suppose yes, but averaging what ?
Method 1 leads to r = 33/10=3.3 and 10/10=1. average is 2.15
Method 2 leads to r = (33+10+10)/(10+10)= 2.65 and (10+10)/10 = 2. average is 2.33

So before I ask the author (who is perhaps here...), I would ike to be sure of what I am speaking of.
 
 

Last question : is it scientificly correct to compute an average value of r, if there is not so many meteors, and so a great scattering  in the values of r ? I ask this, because I would like to compute r from our video observations...

Thanks a lot for any answer, and clear skies !

Jeremie

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