Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1039...40v&link_type=abstract
PARTICLE ACCELERATION AND TRANSPORT IN THE HELIOSPHERE AND BEYOND: 7th Annual International Astrophysics Conference. AIP Confer
Astronomy and Astrophysics
Astrophysics
1
Astronomical Observations, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Flares, Particle Acceleration, Corona, Magnetohydrodynamics And Plasmas, X-Ray Sources, X-Ray Bursts
Scientific paper
Our Sun is about 4.6 billion years old. Richard C. Carrington made the first flare observations in the 19th century, and we have thus observed solar flares for 10-8 part of its age.
Solar flares could be an important factor in the evolution of the solar system. I therefore attempt to paint an evolutionary picture of solar flares based on existing solar observations, original observations of young suns at the beginning of the main sequence and stellar flares. My primary focus will be on deriving the sizes of solar flare plasma loops when the Sun was young. I will also briefly discuss the implications of this picture to particle acceleration and transport in the heliosphere and beyond. ă
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