The phrase "a strong evolution" is correct and usable in written English.
It can be used to describe a significant or impactful change or development in a particular context, such as technology, culture, or personal growth.
Example: "The company has undergone a strong evolution in its approach to sustainability, leading to more eco-friendly practices."
Alternatives: "a significant transformation" or "a profound change."
Distribution systems have undergone a strong evolution in the last few years.
The first elastic plastic regime corresponds to a strong evolution of the indented plastic zone.
Machining tests were conducted in the orthogonal cutting framework and showed a strong evolution of the cutting forces and the chip profiles with tool wear.
Both scission and recombination reactions, which strongly compete as a function of the exposure time, were found to cause a strong evolution of the molecular structure.
Furthermore, while the peak shifts showed that the powders are basically stress free, the SHKL showed a strong evolution of the peak width.
DMTA analysis shows for TPS composites a strong evolution of the main relaxation temperature, which can be linked to the existence of cellulose starch interactions resulting in a decrease of starch chain mobility.
In recent years, pneumococcal vaccination was a field in strong evolution.
Our study focuses on teachers from New Jersey, a State with relatively strong evolution standards and a well-educated citizenry (see subnormalnumbers.blogspot; http://subnormalnumbers.blogspot.kr/2010/04/acceptance-of-evolution-by-state.html).html
Based upon source distribution models assuming three different cosmological evolutionary scenarios (no evolution, weak evolution, and strong evolution), an extensive model for diffuse emission from infrared cirrus, and instrumental noise estimates, we present a comprehensive analysis for the determination of the confusion levels for deep far-infrared observations.
The luminosity function of these intermediate-redshift, luminous infrared galaxies (LIGs) supports an earlier finding of strong evolution [i.e. Φ z) ∝ (1 + z)6.5±3, assuming pure number density evolution] in the more local (z < 0.3) population of ultraluminous infrared galaxies (ULIGs) found at the faintest levels in the IRAS survey.
Cathodically all samples were conductive and showed a strong hydrogen evolution.
