Abstract
We present a study of the effects of atmospheric seeing on quantities derived from observations of solar polarized light – specifically, the vector magnetic flux and quantities derived from its magnitude and direction. Data from the Imaging Vector Magnetograph (‘IVM’) at the U. Hawaii/Mees Solar Observatory, are degraded by various degrees by applying a blur function to the ‘incoming light’, simulating a range of seeing conditions. A quantitative study of the resulting effects on derived quantities including total magnetic flux, vertical electric current density and magnetic shear angles, are discussed as a function of the imposed degradation. The generality of the seeing effects is explored by comparing the results from two different active regions; we find that the results are comparable for those quantities directly computed from the magnetic flux vector (e.g., summed, as in total flux) but less so for those quantities involving higher-order calculations (e.g., derivatives, as in vertical currents). We suggest that for temporal series data from any instrument, a method such as that which we outline here, be applied in order to model the uncertainties imposed on the data (in addition to instrumental uncertainties, etc.) due to seeing variations.
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References
Ambastha, A., Hagyard, M. J., and West, E. A.: 1993, Solar Phys. 148, 277.
Brandt, P. N., Mauter, H. A., and Smartt, R.: 1987, Astron. Astrophys. 188, 163.
Canfield, R. C., de La Beaujardière, J. F., Fan, Y., Leka, K. D., McClymont, A. N., Metcalf, T., Mickey, D. L., Wülser, J.-P., and Lites, B. W.: 1993, Astrophys. J. 411, 362.
Elmore, D. F., Lites, B., Tomczyk, S., Skumanich, A., Dunn, R. B., Schuenke, J. A., Streander, K. V., Leach, T. W., Chambellan, C. W., Hull, H. K., and Lacey, B. L.: 1992, SPIE 1746, 22.
Fontenla, J., Ambasta, A., Kalmán, B., and Csepura, G.: 1995, Astrophys. J. 440, 894.
Jefferies, J. and Mickey, D. L.: 1991, Astrophys. J. 372, 694.
Jefferies, J., Lites, B. W., and Skumanich, A.: 1989, Astrophys. J. 343, 920.
Klimchuk, J. A., Canfield, R. C., and Rhoads, J. E.: 1992, Astrophys. J. 385, 327.
LaBonte, B., Mickey, D. L., and Leka, K. D.: 1999, Solar Phys. 189, 1.
Lee J., Chae, J.-C., Yun, H. S., and Zirin, H.: 1997, Solar Phys. 171, 35.
Leka, K. D.: 1999, Solar Phys. 188, 21.
Leka, K. D. and Skumanich, A.: 1999, Solar Phys. 188, 3.
Lites, B. W.: 1987, Appl. Optics 26, 3838.
Mickey, D. L., Canfield, R., LaBonte, B. J., Leka, K. D., Waterson, M. F., and Weber, H. M.: 1996, Solar Phys. 168, 229.
Ricort, G. and Aime, C.: 1979, Astron. Astrophys. 76, 324.
Ricort, G., Borgnino, J., and Aime, C.: 1982, Solar Phys. 75, 377.
Rimmele, T., Kentischer, T., and Wiborg, P. H.: 1993, Real Time and Post Facto Solar Image Correction, Vol. 13 of NSO/Sacramento Peak Summer Workshops, pp. 24-31.
Roddier, F.: 1981, Progress in Optics XIX, 281.
Sańchez Almeida, J.: 1994, Astron. Astrophys. 292, 713.
Wang, J., Shi, Z., Wang, H., and Lu, Y.: 1996, Astrophys. J. 456, 861.
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Leka, K., Rangarajan, K. Effects of ‘Seeing’ on Vector Magnetograph Measurements. Sol Phys 203, 239–254 (2001). https://doi.org/10.1023/A:1013373424510
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DOI: https://doi.org/10.1023/A:1013373424510