PC Plus HelpDesk - issue 221
This month, Paul Grosse gives you more insight into
some of the topics dealt with in HelpDesk
From the pages of HelpDesk, we look at:
- Transposed colour Infra red with Digital
Cameras;
- Novelty CDR finger bowl dish; and,
- Spam-bot honey pot.
From HelpDesk Extra, we look at: Spreadsheets:
- Basics
- Number Functions
- String Functions
- Conditional Expressions
- Double Entry Book
- Caesar and Horst Feistel
- Files
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HelpDesk
Transposed colour Infra red with Digital Cameras
| Most people have seen the far
infra red footage from police helicopters as
people are chased around in the dark. Whilst this
takes special lenses and sensors to see
wavelengths of light that are emitted by body
heat, your digital camera is actually sensitive
to near infra red. This is the
camera looking at the near infra red from a
garden incinerator.
Note the purple areas which are slightly
cooler than the red hot parts and to our eyes,
they are not hot enough to glow.
Molten glass also emits light at this
wavelength and if you shine your television
remote control (or infra red car fob) at the
camera, it will probably show similar results.
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| This is the eye's approximate
sensitivity to wavelengths of light. The visible
range roughly goes from 400nm (blue) to 700nm
(red) but it also extends below this to around
780nm. The CCD in your camera goes from around
400nm down to around 900nm. Interestingly, our
eyes are also sensitive to UV (wavelengths lower
than 400nm) but this is filtered out by the front
of our eyes. People who have had front of eye
operations can see UV and apparently, it looks a
sort of white. The part of the IR spectrum that
your camera can see between 700 and 900nm is also
represented as a very unsaturated purple (lower
levels of response from the green layer).
If you get an IR filter, you can use the
residual sensitivity of your eyes to see this.
All you need to do is to hold the filter up
against your eye so that you exclude all other
light and allow your eye to adjust to the reduced
level of light and then have a look around.
REMEMBER! THE AMOUNT OF LIGHT ENTERING YOUR
EYE IS STILL HIGH EVEN THOUGH YOU CANNOT SEE IT
VERY BRIGHTLY THEREFORE YOU CAN DAMAGE YOUR EYE
IF YOU LOOK AT SOMETHING THAT IS TOO BRIGHT SUCH
AS THE SUN. WITHOUT VISIBLE LIGHT ALLOWING YOUR
EYE TO REGULATE THE AMOUNT OF LIGHT ENTERING YOUR
EYE, YOU HAVE LOST ONE LEVEL OF PROTECTION SO BE
CAREFUL IF YOU DO THIS.
However, you can investigate the IR
sensitivity of your eyes at lower power levels
and do so reasonably objectively...
|
Looking at IR through your
filter using a diffraction grating (CD)
| If you want
to find out if the black filter you have
transmits NIR light that your eyes are
sensitive to as the 89b and 87 do, you
can test it very easily. First, get a CD
ROM and switch on a tungsten light (not a
fluorescent one as these do not emit a
continuous spectrum or in some cases,
even one that extends beyond red). Next,
adjusting the angle of the CD so that the
tracks split the light from the bulb into
the colours of the rainbow. Next, hold
the filter up to your eye so that you are
now looking through the filter at the
rainbow and you should see a deep red
band. Adjust the angle so that this band
falls half way over the edge of the CD
and hold it very still. Take away the
filter and you should now see that the
red you were looking at appears to have
gone - in fact it has been drowned out by
the visible part of the rainbow which
starts a little further on and which your
eyes are far more sensitive to. You were
looking at the IR part of the spectrum
that the filter passes and you have
confirmed it using a diffraction grating
(the CD ROM) in the same way that a
spectrophotometer would. You can also
note that this is proof that your eyes
are sensitive to infra red light. You can
use this method if you get hold of some
IR security spotlight film instead of a
Wratten filter.
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| This is the
diffracted reflection of a
continuous spectrum source (a
tungsten light bulb) as seen with
a CD. The continuation of the red
into a blue is an artefact of
diffraction gratings in that this
spectrum blends into the next
(the primary (first) is the best
one for separation). |
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| This is a
fluorescent light. Note that it
is not continuous as it is an
emission spectrum of mercury and
another gas along with the
fluorescent coating on the inside
of the tube. The blue is at
404nm, turquoise at 436nm, green
at 546nm, yellow at 578nm and the
red is a series of peaks that
stretch into the IR due to the
noble gas - picked up here by the
IR sensitive camera (as the
purple smudge) although by eye, I
can only see the shortest of the
red peaks. |
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|
You can
see the effect of using an infra red filter just
by putting it over the lens of your camera. Click
on the image on the right to start it off or
click on this link
to go to it in the files directory. |
With the ability
to see into the near infra red region of the
spectrum and record it, we can take some
interesting photographs like the one of the lodge
on the right.This is a composite of two images
- effectively four layers - and we have thrown
away one of them. With the Wratten filter, we
have the range from 900nm up to around 750nm.
With the colour image, we have three bands -
nominally red (700 - 600nm), green (600 to 500nm)
and blue (500 to 400nm). If we transpose the IR,
R and G input bands to R, G and B output bands
using image editing software, we can reproduce
the Ektachrome colour transparency film.
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| If we break down the RGB and IR
images we end up with four layers that we can
play around with. The Ektachrome film works
like this but with some careful photography and a
little image manipulation, you can get similar
results...
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| A is the full spectrum of light
that can be broken up into bands (1, 2 and 3
normally by the camera and 4 using an infra red
filter such as the Wratten. The bands are built
up again into B to produce picture 5, the normal
photograph and C, each layer's sensitivity to IR,
producing the curiously coloured 6. This can vary
from CCD to CCD and the RGB producing dyes in the
CCD can have differing sensitivities to different
bands within the IR band. If you take a picture
with an IR filter and then turn up the colour
saturation, you will either see colour noise or
get different hues depending on what you have
photographed.
Normally, you would then normalise the colours
of the IR band and expand the contrast to produce
a grey-scale D, giving picture 7.
Next, the layers are brought together again -
discarding the blue and shifting everything else
up one so that we have three colours again in
picture 8.
Of course, you don't have to throw away the
blue, you can mix the layers or squash the hue
layer (or part of it) according to any recipe you
like so, without throwing away any layer you
could have...
|
| Layer-> |
R |
G |
B |
| Example |
| 1 |
I+R |
G |
B |
| 2 |
I |
R+G |
B |
| 3 |
I |
R |
G+B |
| 4 |
I |
R + G + B |
| 5 |
I + R + G |
B |
|
| ... and that's just keeping them
in order. You can either separate the layers and
treat them as individual entities or separate
them into HSL and squash or shift the hue layer
then introduce the IR layer - there are a number
of different ways of doing it. In Micrografx
Picture Publisher, one way is to take
the colour image and then shift the hue by 120
degrees (Map | Hue Shift), then go into Map |
Tone Balance, select the red channel and move the
'S' flag to the far right so that the image has
only all of the red information (formerly the
blue layer) removed.
Next, take your IR image that has been
corrected for tone balance, turned into grey
scale and back into RGB and then remove the green
and blue layers by going into Map | Tone Balance,
selecting the green and then blue channels and
with each, pulling the 's' flag to the far right.
After that, copy the now red image into the
clipboard and paste it into the now cyan coloured
image. Click on the white arrow and change 'Merge
Mode' to 'Additive'. Go back to the transform
arrow (black with the cross) and shift the red
image around until it is aligned with the cyan.
Then, click on Object | Combine | All Objects
With Base.
In The GIMP, you can separate
the three colour layers again and do it that way
or you can rotate the hue of the colour image
(Image | Colours | Colourmap Rotation...), click
on select all for both and then grab the colour
arrow on the 'To' colour map, on the inside of
the circular arrow and drag it around by 120
degrees (0.66 Radians/Pi or 2.09 radians).
If you want to squash all of the visible
colours into the G and B layers, you can do it
here just by going from 120 to 360 degrees as
your 'To'.
If you have rotated without squashing, your
old blue layer is now occupying your red layer
and you need to get rid of it. Right click on the
image and select Image | Colours | Levels. Select
the red channel and drag the white arrow to the
left so that the output range is 0 to 0. This
should make your image appear cyan. Click on OK.
Make sure that the red image is selected and
right click on it: "Select | All" then
right click again and "Edit | Copy".
In the 'Layers, channels and paths dialogue
box, make sure that it is displaying the cyan
image and then right click on the image.
Left click "Edit | Paste" and then
in the 'Layers ...' dialogue, change the mode to
'Addition'. Back on the image, move the red layer
around until it is aligned and then anchor it
(click on a part that has no floating image on it
or click on the anchor icon in the 'Layers ...'
dialogue.
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Channels (Layers in film
technology)...
900-700nm.
This is the IR layer taken using a Wratten 87
filter. Note how bright the foliage is, how dark
the path (tarmac) is and how clear the 'blue'
bits of the sky are.
If you click on the image, a larger version of
it (500 pixels wide) will open up in a new
browser or you can right-click on it and 'save
target as...' so that you can play around with it
yourself.
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700-600nm. The following
three images are the three layers of the colour
photograph.This one is the red layer. Note
that the leaves on the trees are quite dark in
comparison to the IR picture above.
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600-500nm. This is the
green layer. Note that the leaves on the trees
are brighter in this layer and also that the sky
is getting progressively lighter as we go through
the layers. |
500-400nm. This is the
blue layer. The sky is very bright and, no doubt,
if we carried on with the UV, it would be
brighter still. The brightness of the sky is due
to dust particles that interfere with the sun's
light, effectively filtering out the blue light
from the direct image (why the sun looks
yellowish) and adding that light (remember that
it is scattered and not absorbed) to the rest of
the sky. We have not got a yellow sun, we have
got a white sun that looks yellow when the blue
light is scattered.Look at the colours on the
tunnel mural and how they look in each layer.
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700-400nm. This is the colour
photograph that the camera takes, from which the
last three of the above separations was taken.You
can save this image so that you can play around
with it as well (it opens up to a larger version
of it).
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900-500nm. This is the
colour shifted photograph, using the IR, R and G
layers and putting them into the R, G and B
layers that we can see so that we can visualise
it.Note that because healthy foliage reflects
so much IR as well as green, that they get
shifted to R and B which is magenta. Sick foliage
does not reflect as much IR and so looks bluer
and in this way, you would be able to see a
camouflaged gun emplacement (the original use of
the Ektachrome film) or pinpoint that ill looking
apple tree in your 5,000 acre orchard before it
kills of a few dozen other trees around it.
If you play around with the two images (IR and
BGR) you will be able to see that some of the
grass through the tunnel is a different colour -
this is where it has been cut badly.
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Some Examples...
As you can see from the above
composite examples that grass is a nice magenta
and so are the trees. However, there are trees
that do not reflect as much green such as copper
beeches. In this shot, we see a number of
different types of tree and the orange ones are
the copper beech (deep red and IR make orange).
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This is the Orangery in
Markeaton Park in Derby. It is called that
because the buildings used to be used to grow
oranges, not because of the way its young grass
(this was taken in May) shows up in IR
composites.This grass is different to the
magenta rye grasses (hard-wearing, football pitch
type grasses) and is more of an ornamental grass
(as in 'keep off the grass' signs). This is proof
that it is a different type of grass.
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When I was researching
this for digital cameras, I went around, taking
shots of all types of things and chose this
because of the different types of trees in it.
However, there was an unanticipated result in
this.As you can see, the red filters on the
cars have come out as yellow, as you would
expect, and the colours of the cars are not the
same as in visible light. The red car, facing
away from us in the centre of the shot is
actually a fairly desaturated blue.
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However, whilst in
visible light, the car looks as though it has a
fairly uniform paint finish (you cannot tell any
difference between parts of it) in IR, a
different story is revealed.The driver's door
shows up brighter in IR and whilst the same blue
as the rest of the car in visible light, it is
completely different in IR. If you had a red car
that needed the driver's door respraying and it
came back from the paint-shop looking like this,
you would send it back.
Sometimes, flaws like this can show up in
sodium light which has a number of bands very
close together in the yellow region (there are
actually many although most spectrophotometers
will show only two - if you remove the Doppler
shift from the gas using a saturation/absorption
method with a tunable laser, you can see the
other transitions as well).
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So, we have seen how shifting the
colours along by one can effectively bring things
that are merely very hot into the extremely hot
range and also make the world around us look
weird. So, what does this do to our already
colourful sunsets? There's only one way to find
out...This is a normal sunset as most people
would expect it to look.
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This is the same sunset, taken a few
seconds later using the Wratten 87 filter |
This is the IR-R-G > R-G-B
composite. You know from your own experience that
as the sun gets closer to the horizon, the
overall light balance shifts towards the red.Here,
we have shifted it back again by shoving the
arbitrary layers up around 100nm or so. This is
more like the middle of the day than a sunset.
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Novelty CDR dish
This
is one thing that you can do if your burning activities
go amiss - one step further on from just using them as
coasters. It is based on the widely publicised activity
that many children did with vinyl records in the 1960s
and 70s using a flower pot and an oven - there is nothing
new here, it is just brought up-to-date in the age of the
CD.
First of all, if you are going to try this, make sure
that you both own the oven and that you are the one that
uses it for cooking - if you decide to try this, you do
so entirely at your own risk.
Having made sure that the kitchen windows and door are
open and that any doors into the rest of the house are
closed, set the oven to gas mark 6. Put a clean, dry
plant pot with a small base (2.5 to 3cm) upside down on a
clean baking tray. Place the CDR on it and when the oven
as got up to temperature, place the baking tray, complete
with plant pot and CDR, on a shelf in the middle of the
oven. Leave it there for five minutes and then check it.
It should have started to droop by then and if your oven
is set a little on the hot side, you might find that it
is already done. If not, leave it for a few more minutes.
Once it is ready, take it out of the oven and let it
cool down, noting how long it took for your oven. Once it
has become rigid enough, you can put it under a cold tap
if you want to. Don't put the plant pot in the water or
you might crack it.
You might notice the smell of hot plastic but remember
that you should have the kitchen well ventilated and that
you are not even melting the plastic, let alone burning
it so the smell you have is similar to the one in the
pressing plant where local exhaust ventilation is all
that is used (a plastic injection moulding plant that I
worked on for a while didn't even have that).
With your new, novelty dish with some kitchen towel in
the bottom you can put some peanuts in and it will be the
talking point of the LAN party.
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Spam-bot honey pot
Spammers have to get their spam out through somewhere
and with known open mail relays being isolated, they have
to comply with the rules for other relays. This usually
involves making sure that a certain proportion of mails
are not bounced and if someone is monitoring the amount
of bounces, sending something that is not spam is the
only way to ensure it. This is why we get mails that are
either empty or have some piece of (formerly) genuine
text in which the spam filters will not be able to filter
out: send 20,000,000 mails of which 10,000,000 contain no
spam and you automatically have a 50% non-bounce success
rate with the mail relay.
Of, course, this depends upon the mail addresses all
being real ones. If the list has been poisoned with false
email addresses, they will all bounce, reducing the
proportion regardless of the nature of the content. So,
how can we poison the email lists? We know that email
address list compilers use spiders to work their way
around the Internet, looking for mailto: strings in web
pages or even joe (at) bloggs (dot) com is not clever
enough nowadays. So, all we have to do is provide them
with a web page or twenty, filled with bogus email
addresses.
If you have a website, but do not use
that IP address for mail services, you can have a few
pages of dedicated email links that are all false. You
can stop genuine search engine spiders from looking at
them by using the robots.txt file - something that a
spam-bot might use to point it in the right direction.
When the spam-bots spider your web pages, they will pick
up on all of these addresses and think that they have hit
gold. All you need to do is have a convincing looking set
of pages that look like they are a directory of company
employees or customers that the spam-bot can see.
Obtaining name lists
How do we make one of these? First of all, we need
some names. There are various lists of first names and
last names on the Internet that you can download - just
type 'first names list' and get the results. Some of
these have the frequency next to them so that instead of
the same unlikely name popping up with the same frequency
as common names ('John' appearing the same number of
times as 'Shula'), you can use the frequencies to change
their probabilities of being selected.
If you get a combined list of boy's and girl's names,
you can copy the table into a spreadsheet which will put
them into columns for you. You will then be able to
highlight the columns you want for each list (male/female
name + frequency) and paste it into a text editor, then
saving it as a text file.
Using the list
Next, you need to write a program that will use these
names to create email addresses.
With frequencies
If you have a list with the frequencies (these are
usually census data with the empirical frequency next to
each name), you can write a program that will first of
all, load up the names into an array (this can be done
with male and female names in the same array if you want
equal distribution) of the form [string][longinteger],
add up the frequency totals and then choose random
numbers between 1 and the total (or 0 and the total-1 if
you are doing it that way). Next, start at the second
long integer value and add the previous long integer to
it, storing the result in the second long integer array
element. Thus...
Before...
John 5467
Fred 4629
Chris 3761
...and after...
John 5467
Fred 10096
Chris 13857
So, if the last number was 120,000, choose a number
between 1 (for the first of the first name) and 120,000.
If our random number is 12,642, this represents 'Chris'
in our example because the end of the Freds is at 10096
and the end of the Chrises is at 13857. You can speed up
a search of a thousand names by using successive
approximation where you start in the middle and if it is
higher, you go to the middle of the upper half and so on.
As these numbers are skewed, you might find that you can
get quicker results if you choose a different starting
point for each iteration if the computer time is that
important to you.
Without frequencies
You just need to load up the names into an array and
then choose them. If they were compiled by frequency (ie,
is not an alphabetical list), you can skew the
probabilities by using a function of the random number.
Next...
We now have a list of names that we can pluck proper
sounding names from. Next, we need to make them into
email addresses.
Email addresses come in a number of formats when used
by corporations which include:
- [firstname].[lastname]@company.com -
joe.bloggs@company.com
- [lastname].[firstname]@company.com -
bloggs.joe@company.com
- [firstinitial].[lastname]@company.com -
jbloggs@company.com
- [firstname][numberbetween1and999]@company.com -
joe341@company.com
These can be with or without the dot in the username
part of the address. As for a company name, you can
register a free domain name on a permanent basis (ie not
temporary) and point it at your firewall (note that at
the beginning, I said that you should use an address that
does not use mail services - this is because your
firewall will reject the mail traffic but the domain name
will turn out correct. To get around this, the spammers
will have to check that a mail server exists at that
address which, no doubt will be the next battle in the
war.
Finally...
We need to turn these into a web page.
So, in your program, configure it to...
load up the name files # ie check that it is going to work
write an html header # top of the page including
# <head> and so on, leading into the body
# with the top of the page
generate a reasonable number of mailto: links
write the footer # possibly with links to other
# honeypot pages
tidy up.
If you add a line to your robots.txt file that says
that spiders shouldn't look there, then, if they use
that, the will go straight there. If you want them to get
there anyway, you can put an invisible link on your page
(small white text on a white background) and then word it
so that anybody who stumbles across there by mistake
knows not to use them.
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HelpDesk Extra
Spreadsheets
Basics
The cells are all given a letter and a number to
reference them. A1 is in the top left and, depending upon
the size of your program (version or memory dependent)
the bottom right could be Z255, BA8191, ZZ65535 or
whatever. Interestingly, spreadsheets work by storing
cell contents in a database rather than storing the whole
sheet as an array. This means that if you have 2 cells
occupied, it should not take up a significantly different
amount of memory whether they are in A1 and B2 or in A1
and ZZ21436 (or anywhere in the vicinity of ZZ9 Plural Z
Alpha for that matter)
Spreadsheets need to know what type of input they are
looking at so that they know how to render it and how to
process it.
How programs recognise user input
(input starts with...) Examples
in blue |
| Program |
Number |
String |
Function |
Cell
reference |
| Abacus 2.3 |
1234567890
3.6 |
"
"Hello |
letters
sum(A12:G19) |
cell address
B9 |
| Lotus 1-2-3 |
1234567890
49.42 |
letters
Total |
@
@COUNT(B1..B11) |
+
+A23 |
| OOo Calc |
1234567890
327 |
letters
Accounts |
=
=SUM(A1:F19) |
=
=BJ19 |
since Abacus on the Sinclair QL, the
emphasis has changed so that users now can just type text
implicitly, having to use a special character to use a
function. In OOo Calc, only the beginning of the cell
entry needs the '=' so if you had
=IF(VLOOKUP(E3;D8:F31;3)>7;SUM(A9:A26);K15), only the
first function needs it.
Number Functions
There are many number functions and, excluding the
statistical functions, they are as listed below...
ABS, ACOS, ACOSH, ACOT, ACOTH, ASIN, ASINH, ATAN,
ATAN2, ATANH, CEILING, COMBIN, COMBINA, CONVERT, COS,
COSH, COT, COTH, COUNTBLANK, COUNTIF, DEGREES, EVEN, EXP,
FACT, FLOOR, GCD, GCD_ADD, INT, ISEVEN, ISODD, LCM,
LCM_ADD, LN, LOG, LOG10, MOD, MROUND, MULTINOMIAL, ODD,
PI, POWER, PRODUCT, QUOTIENT, RADIANS, RAND, RANDBETWEEN,
ROUND, ROUNDDOWN, ROUNDUP, SERIESSUM, SIGN, SIN, SINH,
SQRT, SQRTPI, SUBTOTAL, SUM, SUMIF, SUMSQ, TAN, TANH,
TRUNC.
Many of them are self-explanatory and for those that
are not, there is the help, either on the spreadsheet
itself or as the extra help files that come with the
program.
String Functions
The string (text) functions are pretty similar to
those that you will find in any high-level programming
language They are...
ARABIC, BASE, CHAR, CLEAN, CODE, CONCATENATE, DECIMAL,
DOLLAR, EXACT, FIND, FIXED, LEFT, LEN, LOWER, MID,
PROPER, REPLACE, REPT, RIGHT, ROMAN, SEARCH, SUBSTITUTE,
T, TEXT, TRIM, UPPER, VALUE.
Conditional Expressions
Conditional expressions (ie IF) allow you to use the
output of an expression that can be evaluated in logical
terms (whether something is equal to something else (or
greater than, less than and so on) and giving the
contents of that cell accordingly. These can also be
nested and mixed with other functions allowing things
like =IF(VLOOKUP(E3;D8:F31;3)>7;SUM(A9:A26);K15).
Double Entry Book
The double entry book spreadsheet that is in the
magazine can be found for Lotus 1-2-3 97, MS Excel and
OOo Calc in the files directory which you can enter by
clicking here.
In this version, the months have been typed in manually
but if you want to try out the method described in the
magazine and then change the language, you can see what
happens.
Caesar and Horst Feistel
This is about ROT13 (one of the text (string)
functions). ROT 13 is a Caesar cipher where each letter
is displaced by an offset - in this case 13. A Feistel
network shifts bits around to encrypt data. There is more
about Horst Feistel on the Internet
Files
You can find the files for this month's work in the
files directory which you can enter by clicking here.
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