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Experimental NASA research models, based on observations from the Solar Terrestrial Relations Observatory (STEREO) and ESA/NASA's Solar and Heliospheric Observatory, show that the CME left the sun at speeds of around 900 miles per second, which is a fairly fast speed for CMEs.
Research objectives and content The main goal of this project is the development of an acceleration model for solar energetic particles, which is quantitatively consistent with the recent high energy observations provided by the ESA/NASA~s Solar and Heliospheric Observatory (SOHO) and the recently launched NASA~s Advanced Composition Explorer (ACE) missions.
European Solar and Heliospheric Observatory and Japan's Hinode spacecraft.
Contact with the Solar and Heliospheric Observatory -Soho - positioned between the Earth and the Sun, was lost on June 24 during a routine operation to alter its orbit.
Soho, which stands for Solar and Heliospheric Observatory, was launched in December, 1995.
1 billion satellite called the Solar and Heliospheric Observatory.
The Center uses the Pillar Axiom as a NAS device, consolidating information onto one system from the successful European Space Agency's Solar and Heliospheric Observatory (SOHO) launched in 1995 and Transition Region and Coronal Explorer (TRACE) launched in 1998.
Experimental NASA research models, based on observations from the Solar Terrestrial Relations Observatory (STEREO) and ESA/NASA's Solar and Heliospheric Observatory, indicate that both CMEs left the sun at around 400 miles per second, which is a fairly typical speed for CMEs.