Parker Solar Probe, WISPR Level 3 Data

data designed to reveal the variations in solar K-corona via a subtraction of a "background" model (L2b data; see below) that primarily removes the dominant F-coronal signal. These data are usually in units of MSB, though this should be verified by inspection of the FITS headers. We do not provide L3 data for the high-cadence observations. Important: please see our disclaimer about the L3 data product.