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24 Aug 2009: 3A(sin4 8, sin 24,) - 2(A - B)(sin28, sin 24,)}, of, = of. = ... A , B, F, 211, would not be related to the particle aspect ratio in 6he manner described for spheroids.

8 Dec 2014: Hence from eqn. (23) we have. λ2 (2z cosh B) λ (z2 z2) = 0=. ... To encode the magnetic field dependence we use B = h/kT as defined.

13 Dec 2018: f(x,y,y′) dx. [using a Taylor expansion to first order]. =. b. ... to travel from A to B, B. A. dl. c, (1.32).

1 Sep 2011: 2.2.2 The matrices B, B′, C. Setyν := D(hν )qν, ν < N; yN := D(hN1)qN,. ... By definition (2.2.9),. C := CNν := ADγ1ADγ2 ADγN ν A,B := Bν := ADδ1ADδ2 ADδν ,B′ := B′ν := D0BD0,.

16 Aug 2023: a (b c) = (a c)b (a b)c. (0.11e). Line integrals. ... Further examples. (i) As another example consider the equation (a b)c = d.

7 Apr 2017: M i t 25 T e x t a b b i l d u n g e n. ... die GELEIschen A b b i l d u n g e n fiber Paramevium-Ln'gssehnitte m i t d e m y o n WETZET, a n Flaehschnitten.

5 Jun 2013: above, i.e. compass-wise, in the northern hemisphere, corresponding to up-. ward B. ... waves. The background rotation and azimuthal magnetic field B point. toward the viewer.

17 Jun 2019: a = a(x;y;t); b = b(x;y;t) ; (2.4). when inserted into (2.2), expresses h(a; t) as another function. ... the general 2-dimensional Monge{Ampere equation. A B 2C D& E(&. 2. ) =

6 Oct 2014: or eAA′and the dual vector fields by a or AA′, where a,b,. = ... We choose a nulltetrad eAA. ′of TM, in which. g = εABεA′B′ eAA′eBB. ′=

29 Jul 2017: AB =.  0 11 0.  and A′B′ = 0 11 0. ... kernels of the span of the frame eA′B′C′D′. 30 CHAPTER 2.