First, we show that if the pressure (associated to a weak Leray-Hopf solution of the Navier-Stokes equations) satisfies , then possesses higher integrability up to the first potential blow-up time . Our method is concise and is based upon energy estimates applied to powers of and the utilization of a `small exponent’. As a consequence, we show that if a weak Leray-Hopf solution first blows up at and satisfies the Type I condition $|v|{L^{\infty}{t}(0,T^; L^{3,\infty}(^3))}\leq M$\nabla v\in L^{2+O(\frac{1}{M})}(^3\times (\tfrac{1}{2}T^,T^*)).This is the first result of its kind, improving the integrability exponent of $\nabla v$ under the Type I assumption in the three-dimensional setting. Finally, we show that if $v:\mathbb{R}^3\times [-1,0]\rightarrow \mathbb{R}^3$ is a weak Leray-Hopf solution to the Navier-Stokes equations with $s_{n}\uparrow 0$ such that\sup_{n}|v(\cdot,s_{n})|_{L^{3,\infty}(^3)}\leq M $vO(M^{20})t=0$. Our method is direct and concise. It is based upon known -regularity, global bounds on a Navier-Stokes solution with initial data in and rescaling arguments. We do not require arguments based on backward uniqueness nor unique continuation results for parabolic operators.

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