Determination of the solar minimum period between cycles 22 and 23 from the coronal index of solar activity

Details Determination of the solar minimum period between cycles 22 and 23 from the coronal index of solar activity Determination of the solar minimum period between cycles 22 and 23 from the coronal index of solar activity

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999soph..184..317a&link_type=abstract

Solar Physics, v. 184, Issue 2, p. 317-322 (1999).

Physics

7

Scientific paper

We present the coronal index of solar activity (CI) for 1997 and use the 1996 and 1997 data to examine the properties of the solar minimum between cycles22 and 23. To compute CI, we used only the intensities of the green corona from Lomnický Štít and Sacramento Peak coronal stations. Values of CI were low in the first half of 1997 with an increase from September toward the end of 1997. We determined the minimum in the green corona to be May 1996, which is in coincidence with the results from 2800MHz radio flux, the MgII index and the Wolf number.

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