Physics
Scientific paper
Jan 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mwoc.conf...47p&link_type=abstract
Multi-Wavelength Observations of Coronal Structure and Dynamics -- Yohkoh 10th Anniversary Meeting. Proceedings of the conferenc
Physics
1
Scientific paper
Over the last decade the unprecedented uninterrupted, high resolution, coverage of the Sun has led to the discovery of many new types of small-scale phenomena, as well as a better understanding of phenomena such as X-ray bright points and coronal plumes. Due to the excellent range of telescopes aboard the many spacecraft currently viewing the Sun these small-scale phenomena have been observed in many different wavelengths. Much has been discovered over the past 10 years, but there are still many questions to be answered. What are the connections between all these different small-scale transient phenomenaNULL How are they createdNULL Do they contribute to the heating of the solar corona and if so how significant is their contributionNULL Are any of them the source of the fast solar windNULL I will be reviewing what has been discovered about both the new and well known dynamic quiet Sun phenomena from not only Yohkoh, but also SOHO and TRACE. In particular, I shall discuss the connections they appear to have to X-ray bright points and coronal plumes and will consider if any of them make a major contribution to the heating of the corona.
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