While the southern hemisphere array will span the entire energy range of CTA, covering gamma-ray energies from 20 GeV to more than 300 TeV, the northern hemisphere array will be more limited in size and will focus on the low- and mid-energy ranges from 20 GeV to 20 TeV. For this reason, the northern hemisphere site will not host any Small-Sized Telescopes, which are tuned to capture the highest-energy gamma rays. The threshold configuration plan is for the site to host 4 Large-Sized Telescopes to capture the low-energy sensitivity of CTA and 5 Medium-Sized Telescopes to cover CTA’s core energy range. A further enhancement to the alfa configuration, pending on the approval of the necessary budget, would add other 4 Medium-Sized Telescopes to the array.