Pre-Flight Measurements Necessary for a Correct Data Interpretation
Joachim Köppen DF3GJ Kiel/Strasbourg/Illkirch Summer 2004
Here is a list of items necessary for a reliable and sensible
interpretation of the data after the flight:
- pairing of LDRs of similar photometric properties:
Since the LDRs of each sensor array should have nearly the
same properties, i.e. the slope gamma of the sensivity
curve, one should select matching LDRs. Only then the readings
e.g. blue/red measure the colour independent of the brightness.
procedure clamp a test sensor under a light source. Measure
for each LDR the resistance under this light as well as with a
grey filter held in front of the sensor. The grey filter should be fairly
dark, say the resistance should increase by a factor of ten.
Determine for each LDR the ratio of the two resistances, and keep
a record of this. Select triplets (and one pair) of LDRs of nearly
the same resistance ratio.
The interpreting person must have the recorded data as well
as the grey filter.
- currents through each LDR: is needed to convert the
voltage readings into resistances.
procedure cover the entrance aperture of each sensor,
hold a current meter parallel to the LDR, and measure the current
flowing past the LDR.
Record the value for each sensor with
proper identification.
- overall photometric calibration : serves as an overall check
of the sensor-and-electrconics system.
procedure take readings of all the sensors, using an
arbitrary light source, such as a sheet of white paper held in front of
the sensors and lit by the sun or daylight. Hold a grey filter in front of
the sensors' apertures, and take another set of readings.
The interpreting person must have the recorded data as well
as the grey filter.
- overall colour calibration : ensures that the interpreting person
can link the data with real colours. Any local calibration with the colour
enlarger could be helpful, but as this cannot provide colour calibration
reproducible at other places:
procedure if possible, use the
sunlight on a cloudless day (the only natural standard light source
globally available). Hold the prepared coloured cards - or any other
homogeneously coloured cards - in front of each sensor array, so
that all three (two) sensors are equally illuminated. Record these
voltage readings for all arrays. If the sun cannot be used, use other
source (daylight, tungsten bulb), and provide
precise description of the source (cloud cover, weather conditons,
helpful details about the lamp).
The interpreting person must have the recorded data,
the colour cards, as well as samples of the colour filter material.
- if the above procedures cannot be done before flight,
one could attempt to do this after the flight. This requires that the
complete sensor-electronics payload is available for the analysis.
procedure return sensors+electronics to ISU Illkirch
- temperature of sensors: Since the LDRs' resistance may
depend on temperature - so far I have not ben able to get any data
on our devices - the calibration may differ from the lab and the
actual flight.
procedure To get an estimate about the importance, it would
be good to compare the resistances obtained with a single LDR at
room temperature and chilled for some time in a fridge ...
[I shall be able to do this late next week (after 15 July) - J.K.]
It is hoped that we can use one i-Button from
Jim Burke's experiment to sample the temperature in the vicinity
of the sensors. It is not expected that the temperature change during
flight will be important, but the difference from the lab conditions
might be.
Given this temperature information as well as the availability
of the sensors for the post-flight analysis, it would then be possible
to perform the correct calibrations under the ambient temperature
after flight.
| Top of the Page
| back to Main Page
| back to my Home Page
|