Oscillations in the Coronal Green-Line Intensity Observed at Lominický Štít and Norikura Nearly Simultaneously.

Details Oscillations in the Coronal Green-Line Intensity Observed at Lominický Štít and Norikura Nearly Simultaneously. Oscillations in the Coronal Green-Line Intensity Observed at Lominický Štít and Norikura Nearly Simultaneously.

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003soph..213..269m&link_type=abstract

Solar Physics, v. 213, Issue 2, p. 269-290 (2003).

Physics

4

Scientific paper

We studied intensity oscillations of the coronal green line ([Fexiv] 530.3 nm) observed with two coronagraphs at Lomnický Štít and Norikura nearly simultaneously. In the spectroscopic data obtained at Norikura, we have detected and confirmed the earlier detection of 5-minute oscillations in photoelectric photometer observations made at Lomnický Štít. Quasi-periodic structures in the green-line intensity with a tangential speed up to 400 km s-1 have been detected for the first time. We briefly discuss the implications of these oscillations on the coronal heating mechanisms.

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