Solar-B
is the follow-up mission to the very successful Japan/UK/US Yohkoh mission.
Using a combination of optical, EUV and X-ray instrumentation Solar-B will
study the interaction between the Sun's magnetic field and its corona to increase
our understanding of the causes of solar variability. It is due for launch
in 2005.
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Information about Solar-B EIS
Gallery 1 |
Included
in Solar-B's instrumentation is a 0.5m optical telescope, an EUV imaging specrometer
and an X-ray/EUV telescope.
Posters (MS PowerPoint) Download MSSL Solar-B EIS Poster (~2.2MB) |
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