Abstract
Time-lapse photographs of the Hα chromospheric network were taken at 3-sec intervals with a\(\tfrac{1}{4}\)-Å filter centered at Hα + 0.65 Å, where the network appears as a system of dark mottles. A nearly continuous sequence of 62 hr duration was made possible by summertime operation of the telescope at Thule Air Base, Greenland, 10° above the Arctic Circle. A quiet region was followed across the center of the disc. The life history of the network, as determined by measurement of the cross-correlation of selected photographs taken at intervals ranging between 3 sec and 29 hr, shows a rather complicated behavior. Initially the correlation falls off quite rapidly, dropping from 0.97 at 3 sec to 0.60 at about 7 min. Thereafter, the decline becomes increasingly more gradual, reaching a value of 0.24 at 4 hr. From this point the correlation falls off quite slowly. A least-squares fit to that portion of the cross-correlation curve for time differences greater than 4 hr yields a mean (1/e) life of 25.0 ± 1.6 hr and a value for twice the half-life of 38.8 ± 4.0 hr. This rate of decline is believed to be characteristic of the lifetime of the chromospheric network. The rapid initial loss of correlation appears to be due to a redistribution of the features, seen in the red wing of the Hα line, along the network.
Similar content being viewed by others
References
Bahng, J. D. R. and Schwarzschild, M.: 1961,Astrophys. J. 134, 312.
Beckers, J. M.: 1963,Astrophys. J. 138, 648.
Beckers, J. M.: 1964, Thesis Utrecht; AFCRL Env. Res. Papers No. 49.
Bhavilai, R.: 1965,Monthly Notices Roy. Astron. Soc. 130, 411.
Bhavilai, R.: 1966, in K. O. Kiepenheuer:The Fine Structure of the Solar Atmosphere, Franz Steiner Verlag, Wiesbaden, p. 96.
Bruzek, A.: 1959,Z. Astrophys. 47, 191.
De Jager, C.: 1957,Bull. Astron. Inst. Neth. 13, 133.
De Jager, C.: 1959,Hdb. d. Phys. 52, 80–362.
Hart, A. B.: 1954,Monthly Notices Roy. Astron. Soc. 114, 17.
Hart, A. B.: 1956,Monthly Notices Roy. Astron. Soc. 116, 38.
Janssens, T. J.: 1970,Solar Phys. 11, 222.
Kiepenheuer, K. O.: 1957,Z. Astrophys. 42, 209.
Kiepenheuer, K. O.: 1960,Z. Astrophys. 49, 73.
Kovasznay, L. S. G.: 1949, Heat Transfer and Fluid Mechanics Institute, ASME, p. 211.
Leighton, R. B., Noyes, R. W., and Simon, G. W.: 1962,Astrophys. J. 135, 474.
Osterbrock, D.: 1961,Astrophys. J. 134, 347.
Simon, G. W. and Leighton, R. B.: 1964,Astrophys. J. 140, 1120.
Title, A. M.: 1966, Thesis Cal. Inst. of Technology.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Rogers, E.H. Lifetime of the Hα chromospheric network. Sol Phys 13, 57–77 (1970). https://doi.org/10.1007/BF00963942
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF00963942