High Resolution Observations of Spicules with Hinode/SOT

Details High Resolution Observations of Spicules with Hinode/SOT High Resolution Observations of Spicules with Hinode/SOT

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..397...27s&link_type=abstract

First Results From Hinode ASP Conference Series, Vol. 397, Proceedings of the conference held 20-24 August, 2007, at Trinity Col

Astronomy and Astrophysics

Astronomy

20

Scientific paper

High time cadence unprecedented images at the limb with Ca II H line filtergraph from the Solar Optical Telescope (SOT) aboard Hinode have revealed that a spicule consists of highly dynamic multi-threads (typically twin) as thin as a few tenths of an arcsecond, and shows prominent lateral movement or oscillation with rotation on its axis during its life. This multi-thread structure and lateral motion indicate that the spicules can be driven by magnetic reconnection at unresolved spatial scales at their footpoints.

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