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Much effort has been spent to develop methods to address these issues ([17] [21]; and references therein), including the use of different strains, selective growth conditions, fusion tags, co-expression with binding partners, and expression of independently folded structural domains.
In these conditions, fusion mediated by the H1 protein was increased 1.6-fold (p = 0.0199, t test) by N1, while H7-mediated fusion was increased 2.5-fold (p = 0.0068) and 2.2-fold (p = 0.058) by N4, in the absence and in the presence of TPCK-treated trypsin treatment, respectively.
Under these conditions, fusion proteins are exposed to proteases and could result in cleavage [ 7].
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Furthermore, the responsiveness of the protease specifically to InsP6 provides the user with complete control over the timing and conditions of fusion tag removal, while the autoprocessing nature of the CPD confers a high degree of specificity to fusion tag removal [4], [5].
More intense conditions cause fusion, and less intense conditions form rocks of the hornfels facies.
The validity of using this method under typical conditions in fusion plasmas is then discussed.
No matter the approach, the physicists reasoned that, as the plasma became denser, hotter, and longer-lasting, the conditions for fusion would eventually be met.
Furthermore, due to the extreme conditions in fusion reactors, diagnostic systems may be limited.
The notion is that experiments under the extreme conditions of fusion would allow bomb makers to study the physics of nuclear weapons without exploding them and check the accuracy of computer codes that calculate how well weapons will perform.
To test robustness under more realistic conditions, the fusion procedures were evaluated with and without post hoc bias correction of the ingredient QPEs.
The applications of our work range from geophysics (what is the chemistry of materials under pressure?), to materials performance (can we design materials that will perform under extreme conditions?), to fusion energy (can we create plasmas at high enough density and temperature to undergo nuclear burn?), to astrophysics (can we understand the physics of giant planets and stars?).
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CEO of Professional Science Editing for Scientists @ prosciediting.com