HR: 1340h
AN: G43A-0913 [Abstracts]
TI: Influence of the Second-Order Ionospheric Delay on GNSS Geodetic Solutions
AU: * Palamartchouk, K
EM: kirill.palamartchouk@earth.ox.ac.uk
AF: University of Oxford, Parks road, Oxford, OX1 3PR, United Kingdom
AB:
The level of accuracy reached today by reference GNSS technology is in
great part a consequence of progress in modelling various contributions
to the observables. At the same time, advances in modelling of a single
effect will not necessarily lead to improvements in the final result if
there exist greater mismodelled contributions from other sources.
One of the effects, the importance of which has been recently
understood, is the ionospheric effect of second order. The commonly
accepted ionosphere-free linear phase combination eliminates the
plasma-induced phase delay in GNSS measurements in the approximation of
zero magnetic field. However, due to interaction of the GNSS carrier
wave, propagating in an ionospheric plasma, with the geomagnetic field a
small additional delay is introduced in the phase observable. The
magnitude of such a delay is of the order of~1~cm, and it depends on
the geographic coordinates of the observer, local time, season, and
solar activity.
We use International Reference Ionosphere (IRI2007) and International
Geomagnetic Reference Field (IGRF2005) models to create worldwide maps
of the second-order ionospheric delay and resulting geodetic
displacements for different time, seasons, and phases of solar activity
cycle. We show that, due to diurnal and seasonal variability of the
second-order ionospheric delay, there are apparent oscillations of
geocentre position. We demonstrate that the pattern of such oscillations
changes with the phase of solar activity cycle.
In applications to kinematic and sub-daily static positioning, we
demonstrate that due to high horizontal gradients of electron total
content during morning and evening hours, taking into account the
second-order ionospheric effect becomes meaningful not only for the
global, but also for regional networks. In the case of daily static
solutions accounting for the second-order ionospheric delay can help
improving the solution precision.
Based on the results presented we recommend introducing the modelling of
the second-order ionospheric delay in routine GNSS processing for global
geodetic networks, especially in view of the forthcoming solar activity
maximum.
DE: 1229 Reference systems
DE: 1241 Satellite geodesy: technical issues (6994, 7969)
DE: 6934 Ionospheric propagation (0689, 2487, 3285, 4275, 4455)
SC: Geodesy [G]
MN: 2007 Fall Meeting