Scientific Objectives
The three main scientific objectives of SOHO are:
- Investigation of the outer layer of the Sun, which consists of the chromosphere, transition region, and the corona. CDS, EIT, LASCO, SUMER, SWAN, and UVCS are used for this solar atmosphere remote sensing.
- Making observations of solar wind and associated phenomena in the vicinity of L1. CELIAS and CEPAC are used for "in situ" solar wind observations.
- Probing the interior structure of the Sun. GOLF, MDI, and VIRGO are used for helioseismology.
Read more about this topic: Solar And Heliospheric Observatory
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“The scientific mind is atrophied, and suffers under inherited cerebral weakness, when it comes in contact with the eternal woman—Astarte, Isis, Demeter, Aphrodite, and the last and greatest deity of all, the Virgin.”
—Henry Brooks Adams (1838–1918)
“Along the journey we commonly forget its goal. Almost every vocation is chosen and entered upon as a means to a purpose but is ultimately continued as a final purpose in itself. Forgetting our objectives is the most frequent stupidity in which we indulge ourselves.”
—Friedrich Nietzsche (1844–1900)