𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Sunspot cycle variations of ensemble-averaged active regions

✍ Scribed by John K. Lawrence


Publisher
Springer
Year
1987
Tongue
English
Weight
375 KB
Volume
110
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

✦ Synopsis


We examine published sunspot and calcium plage areas for 1620 solar active regions between 1974 and 1985. With these data we study the properties of ensemble-averaged active regions. The average sunspot area per region, the average plage to sunspot area ratio, and the average plage intensity of regions all vary significantly with the sunspot cycle and in correlation with one another. The average plage area per region varies significantly but is uncorrelated with the sunspot cycle and with the other quantities. While the plage and sunspot areas and the plage intensities of individual active regions observed over a two-year period are strongly correlated, the relationship among these quantities appears to change over an 11-yr period. These results suggest the existence of some energetic connection between active region sunspot areas and plage intensities. Further, if energy balance between sunspot luminosity deficits and facular luminosity excesses holds, then standard models relating these quantities to sunspot and plage areas will have to be modified. Overall energy balance can neither be established nor ruled out.


πŸ“œ SIMILAR VOLUMES


Longitudinal and temporal variations of
✍ Antonio Sanchez-Ibarra πŸ“‚ Article πŸ“… 1990 πŸ› Springer 🌐 English βš– 383 KB

The relationship between sunspot activity in heliographic longitude and coronal holes 1s investigated for the period corresponding to Cycle 21 (Carrington rotations 1623-1779). The major result is that, based on HeT 10830 ~ data, a strong inverse association is found between the longitudinal positio

Limb-darkening and solar cycle variation
✍ F. Albregtsen; P. B. JorΓ₯s; P. Maltby πŸ“‚ Article πŸ“… 1984 πŸ› Springer 🌐 English βš– 677 KB

New observations of the umbral limb-darkening are presented. We find a real and significant decrease in the umbra/photosphere intensity ratio towards the limb. This result contrasts the findings of previous authors and we believe this to be the first time such a decrease is reported. Our conclusion

On the average rate of growth in sunspot
✍ Robert M. Wilson πŸ“‚ Article πŸ“… 1990 πŸ› Springer 🌐 English βš– 411 KB

The average rate of growth during the ascending portion of the sunspot cycle, defined here as the difference in smoothed sunspot number values between elapsed time (in months) t and sunspot minimum divided by t, is shown to correlate (r > 0.78) with the size of the sunspot cycle, especially for t >

Solar irradiance variations from photome
✍ G. A. Chapman; A. D. Meyer πŸ“‚ Article πŸ“… 1986 πŸ› Springer 🌐 English βš– 442 KB

The Extreme Limb Photometer (ELP) has been used to measure the irradiance fluctuation of the Sun due to selected active regions. Forty-five active regions that were completely scanned at various disk positions are included in the analysis. The contribution of these active regions to a global solar i