The Ice, Cloud, and land Elevation Satellite -2 (ICESat-2) observatory launched on September 15, 2018 with objectives to measure changes in ice sheet elevation, monitor sea ice freeboard, and enable a global assessment of vegetation and canopy height (Markus et al., 2017). ICESat-2 uses green laser light emitted by the Advanced Topographic Laser Altimeter System (ATLAS) as the basis for elevation measurements between 88° north and south latitudes (Martino et al., 2019). ATLAS provides the data necessary for ground processing to calculate the round-trip photon time-of-flight from the observatory to Earth and back again. These components are combined with the laser beam pointing vectors (Bae & Webb, 2017) and the position of the observatory in space (Luthcke et al., 2019) to generate the Global Geolocated Photon data product (ATL03) (Neumann et al., 2020a(Neumann et al., , 2020b) which provides a unique latitude, longitude, and elevation for each photon event telemetered for ground processing and an initial discrimination between a band of signal photons (emitted by ATLAS and reflected by Earth) and background photons (emitted by the sun in the same part of the electromagnetic spectrum). Schematics of the ATLAS transmitter and receiver are found in Neumann et al., 2019, Figures 2 and 3 respectively.The ATLAS telescope collects incoming light and is fiber-coupled to filters which only transmit light of the same wavelength as emitted by ATLAS (532 nm ± 0.15) (Neumann et al., 2019). After passing through these filters, light for a given spot is distributed across the elements of a multi-element photomultiplier tube to convert optical energy to electrical energy to be time tagged (a photon event) for further analysis. The ATL03 product is organized by ground tracks, which refer to the relative location of the 6 beams on the ground. Since the spacecraft orientation changes every ∼9 months in order to optimize the position of the solar array relative to the sun, ATLAS strong and weak spots change their relative orientation (from left to right). We organize our analyses by ATLAS spots which do not change with spacecraft orientation. ATLAS spots are numbered 1-6 indicating laser illumination from the instrument field of view, where 1, 3, and 5 are "strong" spots and have four times the energy of spots 2, 4, and 6, referred to as "weak" spots. Each of the three ATLAS strong spots have 16 detection elements (pixels) which supply 16 individual timing channels. Similarly, each of the three ATLAS weak spots have four independent pixels and timing channels (Martino Abstract NASA's ICESat-2 mission measures Earth's elevation with the Advanced Topographic Laser Altimeter System (ATLAS), a 6-beam photon-counting laser altimeter. The Global Geolocated Photon data product (ATL03) is the primary source of photon information used by surface-type-specific higherlevel products, along with the Atmospheric Layer Characteristics product (ATL09). ATL03 provides time-tagged, geolocated photon heights referenced to the ellipsoid and a paramete...