Thursday Mar. 31, 2011
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The bulk of
today's notes follow. There were a couple of handouts (waveform
recorders and the frequency spectrum of lightning) that were briefly
discussed at the start of class that I'll add to the online notes
eventually.
We'll be discussing lightning protection in this class next
week. We'll look at how structures can be protected from
lightning strikes and how you can prevent transients on power lines and
signal cables from damaging sensitive electronics. Before doing
that we might ask how likely is it for a building or anobject to struck
by lightning. Today we are going to derive the "nearest neighbor"
probability distribution function. If lightning strikes are
randomly distributed over a particular region we'll be able to use the
nearest neighbor function to answer questions such as:
What is the most probable distance to the closest strike (the nearest
neighbor)?
What is the average distance to the closest strike?
What are the chances that the closest strike is inside a distance R of
a randomly chosen point on a map?
Before getting into the details of the nearest neighbor derivation it
might be a good idea to review some basic concepts.
A probability distribution is defined above. The
function must be normalized so that integrating the function over all
possible values of x (all possible outcomes) is 1.
The mean value of x is determined by multiplying x by its
probability distribution function and integrating over all values of x.
The cumulative probability
distribution function above gives you the
chance that x is less than or equal to some value xo. You could also compute the
probability that x is equal to or greater than xo.
Here's an example. We'll
figure out the probability distribution function for points on a line
segment of length L.
Multiplying f(x) times dx will tell you what the
chances are of
falling between x and x+dx. Note the odds of falling at a point x
are
zero because a single point has zero width. We need to normalize
the function f(x).
Now we can calculate the average
value of x.
Here's a second example, sort of a
2-dimensional version of what we looked at earlier.
We'll make use of this when we derive the nearest neighbor function.
What is the probability that a
randomly chosen point will fall between r and r + dr on a circle of
radius R. We assume the all points on the circle are equally
likely (that's why f(r) is set equal to a constant k). Sort of
like throwing darts at a dart board (with the
requirement that the dart must hit the dart board).
We need to normalize the distribution function.
So the probability that a dart
thrown at a dartboard will land between r and r + dr is
what if we were to throw N darts? As long as the throws are
really independent of each other, the chances of having a dart land
between r and r + dr would be N times the result above
We can also compute
the average r just like we did in the earlier problem
Now we're ready to derive the
nearest neighbor probability distribution function. The situation
is illustrated in the figure below.
We're asking what is the
probability that the nearest strike (nearest to the point in the center
of the circle) is between r and r + dr. This is not quite the
same as asking what the chances are of falling between r and r +
dr. Now we requiring that the nearest strike fall between r and r
+ dr. We don't want anything inside of r.
We'll assume a lightning strike density of Ng (strikes per km2 per
year) and we assume that the strikes are randomnly distributed.
So we can write w(r) as follows.
At (1) we are integrating w(r) from 0 to r to find out the
probability that the nearest neighbor is inside r. To find
the probability that the nearest neighbor isn't inside r we subtract
the integral from 1. That's (2) in the equation above. (3)
is the probability that a strike falls between r and r + dr. It's
really just the dart board question again. We're multiplying by
Ng because there are, on average, Ng strikes per km2 per year.
The area term in the denominator of the dart board expression is
really just built in to Ng. Ng is a density: strikes per square
kilometer.
How do you solve the equation above for w(r) when w(r) appears in
an integral? The first step is to differentiate the equation with
respect to r. Essentially all of the steps that follow were on a
class handout.
Leibnitz's rule shows you how to handle the term circled in
red. We're differentiating an integral with respect to r, but r
appears in one of the limits.
And now we're back to our derivation. Do you see what was done in
between the first and second lines above? We made use of an
earlier equation.
We just divide w(r) dr by term (3) above and use that to replace term
(2).
We have an expression for w(r) but
it contains an unknown constant k. But need still need to
normalize this equation.
The last equation (highlighted in yellow) is the nearest neighbor
distribution function.
This figure shows 24,790 cloud to ground strikes in a 51 km by
51 km area centered on the Main Gate at the U. of Az. These
strikes occurred between Jan. 1, 2000 and Sept. 23, 2002, a nearly 3
year period. One thing to notice is that the points appear to be
pretty uniformly distributed. We can use this data to estimate
the CG flash area strike density.
This figure shows how that is done. We multiply 24790 by
1/0.7 to correct for the 70% detection efficiency of the lightning
locating network. We then multiply by 1.45, the average number of
strike points per flash (see the next figure). We divide by the
51 km x 51 km area and divide by 3 years (there is very little
lightning between Sept. 23 and Dec. 31). On average there are 6.6
strikes per square kilometer per year in the Tucson area.
This is a portion of a figure handed out a few weeks ago (Thu., Mar.
3).
The left most figure is where the average 1.45 strike points per flash
value came from.