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obvious that reaching the
final goals in the three years period was already
improbable. So I started to underline the importance of an alternative
Plan B
already during the
first ESSReS PhD committee meeting. After an intense dis-
cussion, all committee members shared the opinion that Plan B has to be set up
while I still try to push the initial
.
Luckily, Plan B was established quite quickly. Our partners from the Swedish
Institute of Space Physics gave us willingly access to their set of already measured
CO radiation data. This dataset was obtained with the same observation technique,
but scienti
Plan A
cally complementary to the one I was going to measure. This allowed
me to breakup the consecutive order of the
first two steps of my original plan: I
could gain experience with the retrieval before having
finished the work on my own
instrument. In the best case, I could combine both datasets in the analysis, otherwise
I would completely rely on the Plan B data.
But
firstly, I kept on pursuing Plan A for a while. After some more time, the
missing component was
finally delivered (2). However, the following tests indi-
cated that it did not work stable and it might take again several months for the
supplier to solve the problems. Of course, this kind of trouble has to be expected if
one tries to go beyond the limitations of state-of-the-art technique. But for me it was
very disappointing and I seriously felt the tension between the uncertainties of
scienti
ll formal requirements like the 3-year project
timeframe in this case. So, my optimism was damped again (3) until I really started
to work on Plan B, simultaneously (4).
Some months later, we had one more try with the re-engineered component (5),
but it became clear very quickly that the problem remained and that any solution
will come too late for my project. So, during the second committee meeting, we
decided that I will switch entirely to Plan B and thus skip the technical part
completely. While this was of course disappointing at that moment, I was lucky,
since the work on Plan B was already in progress and allowed for a seamless
transition into the next part of my project.
To keep it short, I started with refreshed motivation into the second phase (6),
but had to face new disappointments after a few months. I made progress in the
numerical data retrieval and got
c work and the need to ful
first results. But these results were not only
inconsistent with previous observations, moreover there were also inconsistencies
within my dataset itself. At this point it became highly questionable if the dataset is
applicable at all. So I spent several months (7) on
finding possible explanations in
every direction: de
ciencies of the retrieval technique, calibration problems of the
instrument, eventually a new atmospheric feature, or simply my own inability? So, I
had created dozens of pieces of a puzzle, but no idea how to put them together—if
if
they
fit together at all. After about two years of my PhD, apparently nothing was
achieved and I felt that it might be better to give up.
Luckily, I had another iron in the
fire. During my research in the months before,
I came across an interesting atmospheric model and I had the idea to replace the
missing technical part of my work with some modeling experiments. With the help
of my PhD committee members, I came into touch with the model developers at the
National Center for Atmospheric Research (NCAR) in Boulder, USA, and we
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