magnet

The Project MAGNET mission 
provided a wealth of airborne-magnetometer data
spanning the globe (Coleman, 1992). 
This dataset represents a single track of horizontal field
intensities (a very small subset of the full collection!).

datasets

Produces power spectral density estimates through iterative
refinement of the optimal number of sine-tapers at each frequency. This
optimization procedure is based on the method of Riedel and Sidorenko
(1995), which minimizes the Mean Square Error (sum of variance and bias)
at each frequency, but modified for computational stability. The same
procedure can now be used to calculate the cross spectrum (multivariate
analyses).

Andrew Barbour

Adaptive, Sine-Multitaper Power Spectral Density and Cross
Spectrum Estimation

Jonathan Kennel

magnet function

A dataframe with 2048 observations on the following 4 variables.
<dl>
<dt><code>km</code></dt>
<dd>Relative along-track distance, in kilometers. The first observation is at zero kilometers.</dd><dt><code>raw</code></dt>
<dd>Raw intensities, in nanotesla.</dd><dt><code>clean</code></dt>
<dd>Edited raw intensities, in nanotesla</dd><dt><code>mdiff</code></dt>
<dd>The difference between <code>clean</code> and <code>raw</code> intensities, in nanotesla.</dd>
</dl>

Format

A single line of Project MAGNET horizontal field intensity — magnet

A dataframe with 2048 observations on the following 4 variables.
<dl>
<dt><code>km</code></dt>
<dd>Relative along-track distance, in kilometers. The first observation is at zero kilometers.</dd>

<dt><code>raw</code></dt>
<dd>Raw intensities, in nanotesla.</dd>

<dt><code>clean</code></dt>
<dd>Edited raw intensities, in nanotesla</dd>

<dt><code>mdiff</code></dt>
<dd>The difference between <code>clean</code> and <code>raw</code> intensities, in nanotesla.</dd>


</dl>

magnet: A single line of Project MAGNET horizontal field intensity

Description

Arguments

Format

Details

Raw and Clean Sets

References

See Also

Examples