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A Theory of Matter and Electricity by Birkhoff G.D.

By Birkhoff G.D.

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H. Schröter, Sol. Phys. M. E. M. G. , Astron. Astrophys. R. E. R. Wilson, Sol. Phys. J. Defouw, Astrophys. J. 209, 266 (1976) W. Deinzer, G. Hensler, M. Schuessler, E. Weisshaar, Astron. Astrophys. 139, 426 (1984a) W. Deinzer, G. Hensler, M. Schuessler, E. Weisshaar, Astron. Astrophys. P. Drake, Phys. P. Feynman, Progr. Low Temp. Phys. Chap. 2. N. Frazier, J. Stenflo, Sol. Phys. E. , Supercond. Sci. Technol. 14, 729 (2001) R. Howard, Astrophys. J. 130, 193 (1959) R. Howard, J. Stenflo, Sol. Phys.

7 shows an example of statistical studies performed with New Solar Telescope (NST) of Big Bear Solar Observatory. Observations were done with adaptive optics correction using TiO 7057 Å line with 10 s time cadence (Abramenko et al. 2010). 7 shows the probability distribution functions (PDFs) for the diameter, D, lifetime, LT, and maximum intensity, Imax , of bright points tracked during about 2 h period. 6 % of bright points live less than 120 s. The lifetime distribution function follows a log-normal approximation for all features with lifetime exceeding 100 s.

If line of force does not branch, then it cannot have a beginning or an end. Hence, it was postulated that there are three classes of nonbranching lines of force: (1) those that start at infinity and end at infinity; (2) those that remain in a bounded volume (closed or nonclosed) and (3) field lines that originate at infinity but are trapped within a finite volume. These early studies of various magnetic field configurations and their properties form the basis for the studies of magnetic field structures and their effects on various plasmas.

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