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NEWS HOME INSTRUMENT MISSIONS DATA PUBLICATIONS CONTACTS INDEX
Summary


Rosetta/SREM summary plots

TC3 and S14 counters
Rosetta/SREM proton/electron environment

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Historical Plots

2004
JAN FEB MAR APR MAY JUN JUL AUG SEP OCT NOV DEC

2005
JAN FEB MAR APR MAY JUN JUL AUG SEP OCT NOV DEC

2006
JAN FEB MAR APR MAY JUN JUL AUG SEP OCT NOV DEC

2007
JAN FEB MAR APR MAY JUN JUL AUG SEP OCT NOV DEC

2008
JAN FEB MAR APR MAY JUN JUL AUG SEP OCT NOV DEC

2009
JAN FEB MAR APR MAY JUN JUL AUG SEP OCT NOV DEC

2010
JAN FEB MAR APR MAY JUN JUL AUG SEP OCT NOV DEC

2011
JAN FEB MAR APR MAY JUN JUL AUG SEP OCT NOV DEC

2012
JAN FEB MAR APR MAY JUN JUL AUG SEP OCT NOV DEC

2013
JAN FEB MAR APR MAY JUN JUL AUG SEP OCT NOV DEC

2014
JAN FEB MAR APR MAY JUN JUL AUG SEP OCT NOV DEC

2015
JAN FEB MAR APR MAY JUN JUL AUG SEP OCT NOV DEC

2016
JAN FEB MAR APR MAY JUN JUL AUG SEP OCT NOV DEC

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Legend

The Rosetta/SREM summary plots show the time course of the two SREM counters TC3 and S14.

Counter TC3 is sensitive to highly energetic protons and electrons and counter S14 is mainly sensitive to protons. The background level is caused by cosmic rays and is normally around 2 c/sec in TC3 and 0.2 c/sec in S14.

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