Time Variability of Active Region Loops Observed with the Coronal Diagnostic Spectrometer (Cds) on SOHO

Details Time Variability of Active Region Loops Observed with the Coronal Diagnostic Spectrometer (Cds) on SOHO Time Variability of Active Region Loops Observed with the Coronal Diagnostic Spectrometer (Cds) on SOHO

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998soph..182...73k&link_type=abstract

Solar Physics, v. 182, Issue 1, p. 73-95 (1998).

Physics

71

Scientific paper

Monochromatic images from the Coronal Diagnostic Spectrometer (CDS) of loops above active regions show clear evidence of rapid time variability. The rapidly changing conditions that we observe give a new conception of loop systems that has never before been seriously considered. Loop systems, particularly in emission lines formed at temperatures in the 1 5 × 105 K range, traditionally thought of as transition region temperatures, are seen to change significantly over a period of 1 hour. Loops may appear or disappear in certain emission lines, may show rapid variations in the distribution of the emission along their lengths, or may change shape or expand outward, all on time scales of 10 20 min. At other temperatures below 1.5 MK the variability appears less striking, but is still pronounced. At high temperatures, i.e., T ≥ 1.5 MK, conditions are normally much more stable. Examples exist, however, of loop systems showing violent changes in images at all temperatures up to Fe xvi formed at 2.7 MK. The structural variability is accompanied by high Doppler shifts, especially in the O v line. Corresponding velocities typically amount to 50 100 km s-1, but values as high as 300 km s-1 have been recorded. Animations with illustrative examples of loop variability have been prepared and are found on the enclosed CD-ROM. In addition we briefly discuss other structural and dynamical properties of active region loops, particularly those with temperatures below 1.5 MK. Theoretical models of loops cannot explain the present observations, but models that combine extreme fine structure, episodic heating and magneto-acoustic wave disturbances propagating in the loop legs seem promissing.

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