The SHARPP Instrument on the Solar Dynamics Observatory Mission

Details The SHARPP Instrument on the Solar Dynamics Observatory Mission The SHARPP Instrument on the Solar Dynamics Observatory Mission

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmsh52a0491h&link_type=abstract

American Geophysical Union, Fall Meeting 2002, abstract #SH52A-0491

Physics

7594 Instruments And Techniques

Scientific paper

The Solar Heliospheric Activity Research and Prediction Program (SHARPP) was selected by NASA for inclusion on the Solar Dynamics Observatory (SDO) mission. SDO is the first mission within the International Living With a Star program. SHARPP consists of a complement of seven EUV solar disk imagers collected into a package called the Atmospheric Imaging Assembly and a white light coronagraph called the KCOR. The AIA will observe the solar disk at seven wavelengths simultaneously with a cadence of about 10 seconds and a pixel size of about 0.7 arc seconds. The KCOR will observe the white light corona from 2-15 solar radii with a cadence of about 1 minute. The details of the science program and instrument configuration will be described.

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