Hinode Euv Study Of Jets In The Sun’s South Polar Corona

Details Hinode Euv Study Of Jets In The Sun’s South Polar Corona Hinode Euv Study Of Jets In The Sun’s South Polar Corona

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.7201c&link_type=abstract

American Astronomical Society Meeting 210, #72.01; Bulletin of the American Astronomical Society, Vol. 39, p.178

Astronomy and Astrophysics

Astronomy

Scientific paper

Using the Hinode EUV Imaging Spectrometer coronal jets were observed on 20-JAN-2007 over a range of emission lines and corresponding plasma temperatures using the 40 arc sec wide slot images. In this preliminary analysis, jet plasma temperature and emissivity have been estimated while, based on assumptions about the jet morphology, electron density estimates are given and jet velocity measured. The evolution of the jets will be followed in a number of different EUV emission lines and jet energy input as a function of time will be assessed with reference to the magnetic field topologies involved.

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