Titlebook: Infrared Solar Physics; Proceedings of the 1 D. M. Rabin,J. T. Jefferies,C. Lindsey Conference proceedings 1994 Springer Science+Business M

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V. Levkovsky,P. Papushev,R. Salakhutdinovnannte „joint production function“ („jpf“) als . Mehrgüter-Produktionsfunktion das geeignete Konzept. Diese „jpf“ wurde bisher jedoch nur in einem statisch-deterministischen Zusammenhang betrachtet. Damit stellt sich nun die Aufgabe, eine stochastische „jpf“ zu formulieren sowie unter produktionsthe

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Formation of the Solar 10830 Å Line upper chromosphere. The computed 10830 Å line is shown for the four atmospheric models and for three values of the coronal illumination. The calculated off-limb 10830 intensity distribution shows a minimum in the low chromosphere and a maximum at roughly 2000 km above the photosphere, in general ag

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Variability of the Solar He I 10830 Å Tripletvariation is similar to that of other activity indices but with some interesting small differences. Since images are available, it has been possible to decompose the full disk index into components due to plages, filaments, coronal holes and background. At all times during the cycle, most of the sig

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Conference proceedings 199492. Aimed at active workers andgraduate students in solar physics, this volume provides the firstcomprehensive view of a rapidly expanding discipline that gives us anew perspective on the sun..Measurements across the wide infrared spectral range -- here, from 1mum to 1 mm -- can probe the solar atmo

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