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Noise evaluation
Time series recorded during the 96 hour break in transmission between tows
allowed background noise levels on the instruments to be obtained by applying
the same least squares fitting procedure as was used to extract data amplitudes.
Although there is an implicit assumption that the noise level remained constant
over the four days of the CSEM experiment, this approach allows direct comparison
with the data. Noise levels are plotted in Figure. 2
at frequencies chosen to cover the full range transmitted during the experiment.
The noise values determined for each receiver have been normalised by the
source dipole moment to provide estimates that can be compared directly
with the data amplitudes shown in later figures.
Sources of noise can be divided into two categories: external and instrumental.
External sources include electromagnetic fields from ionospheric and cultural
sources, and motionally induced fields caused by microseisms, water currents
and tectonic activity. Electric fields decay rapidly in the conductive seawater
layer, with the result that ionospheric noise at frequencies greater than
0.03 Hz is effectively screened by the water depths encountered on
the Reykjanes Ridge. Similarly, high frequency noise from cultural sources
is also removed from the spectrum. Between 0.1 Hz and 2 Hz the
dominant sources of external noise are microseisms generated by the non-linear
interference of sea surface gravity wave trains (Webb & Cox 1986). These
produce pressure fluctuations which can propagate to the seafloor even in
deep water, resulting in water and seafloor motions which generate electromagnetic
fields. In addition, tectonically generated seismic activity can cause ground
and water motions which also induce electromagnetic fields (Webb & Cox,
1982; Webb & Cox, 1986).
Noise generated in the instrument itself by the amplifiers and electrodes
is independent of the receiver dipole length and so signal to noise ratio
increases with increasing receiver dipole length. The ELFs were substantially
noisier than the LEMs due to their shorter receiver dipole length, although
the factor of 30 difference in antenna length suggests that the difference
between ELF and LEM noise levels should be larger if the observed values
were due only to instrumental noise. Kermit was nearly an order of magnitude
more noisy than the other ELF instruments because of contamination by noise
from an MT magnetometer deployed in tandem with the instrument. Quail, which
was re-deployed after releasing prematurely, was much noisier during its
second deployment than its first. This could be due either to an external
noise source associated with the change in location or to instrumental noise
introduced between deployments (it was modified to record MT as well as
CSEM data).
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field decomposition Up: Data
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Lucy MacGregor
Fri Aug 15 08:48:04 PDT 1997