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SOLAR CALCIUM PLAGE DATA
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Solar Calcium Data (All ftp)For many years, solar observatories have monitored the Sun in the calcium (Ca) K line wavelength by using a filter that allows only this wavelength's light through, calcium filtergrams, or spectroheliograms. Daily full disk calcium K232 images are reduced to provide calcium plage positions and areas or summed to produce a daily Ca K index. Ca K active regions can be seen moving across the solar disk, above the white light sunspot regions, and higher in the solar atmosphere (chromosphere).1a.) Daily Calcium Plage Areas from Mt. Wilson Observatory 1915-1984 -- Peter Foukal
1b.) San Fernando Observatory K-line facular data -- Gary Chapman
1c.) Daily calcium plage reduced data, including position, areas and intensities. Solar observatories contributing to this database include McMath Solar Observatory (1942-Sep 1979), Hale Observatory (Mt. Wilson Solar Observatory -- Oct 1979-Sep 1981), and Big Bear Solar Observatory (Oct 1981-Oct 1987)
2a. Daily summary data of the McMath/Hale/BigBear database 1942-1987 -- includes YYMMDD, number of plage regions, total corrected plage area, and Calcium plage index for that day.
2b. Big Bear Solar Observatory Calcium K Index
2c. Sacramento Peak Solar Observatory Daily Calcium K Index
3. SGD Table -- Solar-Geophysical Data Regions of Solar Activity Table 1969-1982 |
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