Neutron-induced reactions on unstable isotopes play a key role in the nucleosynthesis i-, r-, p-, rp-and νp-processes occurring in astrophysical scenarios. While direct cross section measurements are possible for long-living unstable isotopes using the neutron Time-of-Flight method, the currently available neutron intensities (≈ 10 6 n/s) require large samples which are not feasible for shorter lifetime isotopes. For the last four decades, the 7 Li(p, n) reaction has been used to provide a neutron field at a stellar temperature of ≈ 0.3 GK with significantly higher intensity, allowing the successful measurement of many cross sections along the s-process path. In this paper we describe a novel method to use this reaction to produce neutron fields at temperatures of ≈ 1.5-3.5 GK, relevant to scenarios such as convective shell C/Ne burning, explosive Ne/C burning, and corecollapse supernovae. This method will allow direct cross section measurements of many important reactions at explosive temperatures, such as 26 Al(n, p), 75 Se(n, p) and 56 Ni(n, p).