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<!DOCTYPE html PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html><head><meta http-equiv="Content-Type" content="text/html; charset=windows-1252">
<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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