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Titel |
Systematic Residual Ionospheric Errors in Radio Occultation Data and a Potential Way to Minimize them |
VerfasserIn |
Julia Danzer, Barbara Scherllin-Pirscher, Ulrich Foelsche |
Konferenz |
EGU General Assembly 2013
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Medientyp |
Artikel
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Sprache |
Englisch
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Digitales Dokument |
PDF |
Erschienen |
In: GRA - Volume 15 (2013) |
Datensatznummer |
250075833
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Zusammenfassung |
Radio Occultation (RO) sensing is used to probe the Earth’s atmosphere in order to obtain
information about its physical properties. With a main interest in the parameters of the neutral
atmosphere, there is the need to perform a correction of the ionospheric contribution to the
bending angle. Since this correction is an approximation to first order, there exists an
ionospheric residual, which can be expected to be larger when the ionization is high (day
versus night, high versus low solar activity). The ionospheric residual systematically affects
the accuracy of the atmospheric parameters at low altitudes, at high altitudes (above
25 km to 30 km) it even is an important error source. In climate applications this
could lead to a time dependent bias which induces wrong trends in atmospheric
parameters at high altitudes. The first goal of our work was to study and characterize this
systematic residual error. In a second step we developed a simple correction method,
based purely on observational data, to reduce this residual for large ensembles of
RO profiles. In order to tackle this problem we analyzed the bending angle bias of
CHAMP and COSMIC RO data from 2001 to 2011. We could observe that the
night time bending angle bias stays constant over the whole period of 11 years,
while the day time bias increases from low to high solar activity. As a result, the
difference between night and day time bias increases from about -0.05μrad to
-0.4μrad. This behavior paves the way to correct the solar cycle dependent bias
of day time RO profiles. In order to test the newly developed correction method
we performed a simulation study, which allowed to separate the influence of the
ionosphere and the neutral atmosphere. Also in the simulated data we observed a similar
increase in the bias in times from low to high solar activity. In this model world we
performed the climatological ionospheric correction of the bending angle data, by using
the bending angle bias characteristics of a solar cycle as a correction factor. After
the climatological ionospheric correction the bias of the simulated data improved
significantly, not only in the bending angle but also in the retrieved temperature profiles. |
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