Simultaneous Magnetographic and XUV Observations of a Coronal Jet

Details Simultaneous Magnetographic and XUV Observations of a Coronal Jet Simultaneous Magnetographic and XUV Observations of a Coronal Jet

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh41a14m&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH41A-14

Physics

7509 Corona, 7519 Flares

Scientific paper

On 03 November 2000, a jet of hot plasma appeared in the solar corona, and was observed by the Yohkoh Soft X-ray Telescope (SXT) and the TRACE coronal imager. The jet of magnetically channeled plasma, measuring over 280 megameters in length, serendipitously occurred within the high-resolution field of view of the SOHO Michelson Doppler Interferometer (MDI). We present the X-ray, extreme ultraviolet, and magnetographic observations, and attempt to draw conclusions about the evolution of the jet based upon the evolution of the magnetic field.

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