Physics
Scientific paper
Dec 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...50..311g&link_type=abstract
Solar Physics, vol. 50, Nov.-Dec. 1976, p. 311-327.
Physics
27
Astronomical Photography, Magnetic Flux, Solar Corona, Solar X-Rays, Spectroheliographs, X Ray Spectra, Density Distribution, Error Analysis, Life (Durability), Solar Activity, Solar Cycles
Scientific paper
Observations of X-ray bright points (XBP) over a six-month interval in 1973 show significant variations in both the number density of XBP as a function of heliographic longitude and in the full-sun average number of XBP from one rotation to the next. The observed increases in XBP emergence are estimated to be equivalent to several large active regions emerging per day for several months. The number of XBP emerging at high latitudes varies in phase with the low-latitude variation and reaches a maximum approximately simultaneous with a major outbreak of active regions. The quantity of magnetic flux emerging in the form of XBP at high latitudes alone is estimated to be as large as the contribution from all active regions.
Golub Leon
Krieger Allen S.
Vaiana Giuseppe S.
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