Dynamics of limb features from TRACE EUV observations

Details Dynamics of limb features from TRACE EUV observations Dynamics of limb features from TRACE EUV observations

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.505..619z&link_type=abstract

In: SOLMAG 2002. Proceedings of the Magnetic Coupling of the Solar Atmosphere Euroconference and IAU Colloquium 188, 11 - 15 Jun

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Limb Features, Spicules, Uv Radiation

Scientific paper

We present a preliminary study of spicule dynamics from TRACE UV observations in the 1216 (Ly-α), 1550 (C IV), 1600 and 1700 Å bands near the solar north pole. Spicules are visible beyond the in all bands, being stronger in the Ly-α and C IV bands, where some are seen crossing the limb. After reaching maximum height of up to 16000 km (40000 in exceptional cases), some of them fall back, others diffuse and a small number eject their material into the corona.

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