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1 face magnetic fields, B approximately 10(15) gauss.
2 nos, and magnetic fields in excess of 10(13) Gauss.
3 m core field strength of approximately 10(7) gauss.
5 reconstituted with the human btk gene to a 1-gauss 60-Hz electromagnetic field (EMF) has been reporte
6 support the hypothesis that exposure to a 1-gauss 60-Hz EMF had a causal effect on protein-tyrosine
8 white dwarf in MV Lyrae of between 2 x 10(4) gauss and 1 x 10(5) gauss, too low to be detectable by o
10 magnetar-strength magnetic fields (of 10(15) gauss and above) and for powering the explosion of a rot
13 traints must be satisfied, namely the famous Gauss-Bonnet theorem, and an inequality stemming from th
15 in the electronic absorption spectra and < 8 gauss changes in the copper hyperfine coupling constants
16 scale has been detected to date (<2 x 10(21) Gauss-cubic centimeter), but here the discovery of multi
18 find that for surfaces with zero or positive Gauss curvature, a common feature of the response is the
19 uss in small external fields (less than 1000 gauss), enabling ferromagnetic control of local electron
22 ical with an overall EPR line width of 29-31 gauss (G) was generated by reaction of PGHS-2 with ethyl
23 uced tyrosyl radical from a functional 33-35-gauss (G) wide doublet/wide singlet to a 26-G narrow sin
24 uncation in the meriodonal direction through Gauss--Hermite quadrature projected onto a simple discre
25 sulting hyperfine fields are as high as 9000 gauss in small external fields (less than 1000 gauss), e
26 expressions are suggested to determine both Gauss (K) and Mean (H) curvatures as functions of invari
27 vection-diffusion equation coupled either to Gauss' law or Poisson's equation, depending on the choic
29 eeman shift approximately 4 x 10(-18) at 0.1 Gauss magnetic field, compared to approximately 10(-8) f
30 We show that the probability p(t) that a Gauss-Markov process will first exceed the boundary at t
32 find that field strengths larger than ~10(5) gauss may produce the observed depression, and in one ca
33 ultant modes are similar to truncated Bessel-Gauss modes that exhibit the ability to self-reconstruct
34 orbital angular momentum possessing Laguerre Gauss modes, are favourable as flying information carrie
36 le-splay (Gauss) modulus difference with the Gauss modulus of the L(o) phase being more negative than
37 n that of the L(d) phase and a saddle-splay (Gauss) modulus difference with the Gauss modulus of the
38 ion to the highest fields available, 600,000 gauss, more than a million times the Earth's magnetic fi
39 f the white dwarf is strong enough (at 10(6) gauss or more) to channel the accreted matter along fiel
43 d DPPC and DMPC bilayers are approximately 1 Gauss smaller (greater) than in the corresponding disper
45 rae of between 2 x 10(4) gauss and 1 x 10(5) gauss, too low to be detectable by other current methods
48 at g=2.012 with hyperfine splitting of 17.5 Gauss, which is consistent with nitrosoheme formation an
49 rface dipolar magnetic field of 4.9 x 10(13) gauss, which is higher than those of the vast majority o
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