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Parker Solar Probe (PSP), launched on August 12th, 2018, is an ongoing mission to probe the solar corona (perihelion from 35.7 solar radii (Rs) to 9.86 Rs). In particular, this gives us an opportunity to study the solar wind energy flux in the inner heliosphere, which is of great importance to determine the acceleration of the solar wind at the base of the corona. We investigate the solar wind energy flux in the inner heliosphere using 12-day observations around each perihelion of Encounter Onedoi:10.5281/zenodo.4660278 fatcat:yxvs23rxufhqdjrhrd44enk4ee