STEREO.html
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<title>STEREO ROR</title>
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<h3>IMPACT/MAG, IMPACT/SWEA and PLASTIC data from STEREO</h3>
</br>
Magnetometer data from the STEREO/IMPACT/MAG instruments are made
available by UCLA (Lead: C. T. Russell).<br/>
Electron data from the STEREO/IMPACT/SWEA instruments are made available
by CESR (Lead: J.-A. Sauvaud).<br/>
All STEREO IMPACT (PI: J. G. Luhmann) data and information may be found at <br/>
<a href="http://sprg.ssl.berkeley.edu/impact/">http://sprg.ssl.berkeley.edu/impact/</a>
<p>
Solar wind proton data from the STEREO/PLASTIC instruments are made
available by UNH (PI: A. B. Galvin).<br/>
All STEREO PLASTIC data and information may be found at <br/>
<a href="http://fiji.sr.unh.edu/">http://fiji.sr.unh.edu/</a>
<p>
We strongly recommend contacting/working directly with the instrument
leads regarding data interpretation and publication in order to be
informed of the latest nuances and accuracy updates of the dataset.
<p>
For SWEA electron measurements, calibrations have been done and permit
data usage for most scientific purposes. The usual long-term degradation
of the detectors has, however, not yet been accounted for. Thus the SWEA
data should not be used/interpreted in terms of absolute value.
<p>
It is also noted that, since commissioning, the SWEA instruments on both
STEREO spacecraft have registered difficulty to characterize the solar
wind at core electron energies. The nature of the degradations is such
that electron measurements below 45 eV cannot be used. Data products
used in AMDA have these lower energies removed. However, halo and higher
energy electrons are unaffected.
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