You have provided us NOTHING suggesting that the reporting of the GHG effect of CO2 is dishonest.
As your own source's have shown, the ocean's role in the planet's climate has been widely studied. They simply haven't found what you think they should have found.
The chartered purpose of the IPCC is the assess the science concerning the possible warming of the planet from human emission of greenhouse gases.
From AR6, WGI
"By the early 20th century, cyclical changes in insolation due to the interacting periodicities of orbital eccentricity, axial tilt and axial precession had been hypothesized as a chief pacemaker of ice age ā interglacial cycles on multi-millennial time scales (Milankovitch, 1920). Paleoclimate information derived from marine sediment provides quantitative estimates of past temperature, ice volume and sea level over millions of years (Figure 1.5; Emiliani, 1955; Shackleton and Opdyke, 1973; Siddall et al., 2003; Lisiecki and Raymo, 2005; Past Interglacials Working Group of PAGES, 2016). These estimates have bolstered the orbital cycles hypothesis (Hays et al., 1976; Berger, 1977, 1978). However, paleoclimatology of multi-million to billion-year periods reveals that CH4, CO2, continental drift, silicate rock weathering and other factors played a greater role than orbital cycles in climate changes during ice-free āhothouseā periods of Earthās distant past (Frakes et al., 1992; Bowen et al., 2015; Zeebe et al., 2016)."
2.2.1 Solar and Orbital Forcing
The AR5 assessed solar variability over multiple time scales, concluding that total solar irradiance (TSI) multi-millennial fluctuations over the past 9 kyr were <1 W mā2, but with no assessment of confidence provided. For multi-decadal to centennial variability over the last millennium, AR5 emphasized reconstructions of TSI that show little change (<0.1%) since the Maunder Minimum (1645ā1715) when solar activity was particularly low, again without providing a confidence level. The AR5 further concluded that the best estimate of radiative forcing due to TSI changes for the period 1750ā2011 was 0.05ā0.10 W mā2 (medium confidence), and that TSI very likely changed by ā0.04 [ā0.08 to 0.00] W mā2 between 1986 and 2008. Potential solar influences on climate due to feedbacks arising from interactions with galactic cosmic rays are assessed in Section 7.3.4.5.
Slow periodic changes in the Earthās orbit around the Sun mainly cause variations in seasonal and latitudinal receipt of incoming solar radiation. Precise calculations of orbital variations are available for tens of millions of years (Berger and Loutre, 1991; Laskar et al., 2011). The range of insolation averaged over boreal summer at 65°N was about 83 W mā2 during the past million years, and 3.2 W mā2 during the past millennium, but there was no substantial effect upon global average radiative forcing (0.02 W mā2 during the past millennium).
A new reconstruction of solar irradiance extends back 9 kyr based upon updated cosmogenic isotope datasets and improved models for production and deposition of cosmogenic nuclides (Poluianov et al., 2016), and shows that solar activity during the second half of the 20th century was in the upper decile of the range. TSI features millennial-scale changes with typical magnitudes of 1.5 [1.4 to 2.1] W mā2 (C.-J. Wu et al., 2018). Although stronger variations in the deeper past cannot be ruled out completely (Egorova et al., 2018; Reinhold et al., 2019), there is no indication of such changes having happened over the last 9 kyr.
Recent estimates of TSI and spectral solar irradiance (SSI) for the past millennium are based upon updated irradiance models (e.g., Egorova et al., 2018; C.-J. Wu et al., 2018) and employ updated and revised direct sunspot observations over the last three centuries (Clette et al., 2014; Chatzistergos et al., 2017) as well as records of sunspot numbers reconstructed from cosmogenic isotope data prior to this (Usoskin et al., 2016). These reconstructed TSI time series (Figure 2.2a) feature little variation in TSI averaged over the past millennium. The TSI between the Maunder Minimum (1645ā1715) and second half of the 20th century increased by 0.7ā2.7 W mā2 (Jungclaus et al., 2017; Egorova et al., 2018; Lean, 2018; C.-J. Wu et al., 2018; Lockwood and Ball, 2020; Yeo et al., 2020). This TSI increase implies a change in ERF of 0.09ā0.35 W mā2 (Section 7.3.4.4).
Estimation of TSI changes since 1900 (Figure 2.2b) has further strengthened, and confirms a small (less than about 0.1 W mā2) contribution to global climate forcing (Section 7.3.4.4). New reconstructions of TSI over the 20th century (Lean, 2018; C.-J. Wu et al., 2018) support previous results that the TSI averaged over the solar cycle very likely increased during the first seven decades of the 20th century and decreased thereafter (Figure 2.2b). TSI did not change significantly between 1986 and 2019. Improved insights (Krivova et al., 2006; Yeo et al., 2015, 2017; Coddington et al., 2016) show that variability in the 200ā400 nm UV range was greater than previously assumed. Building on these results, the forcing proposed by Matthes et al. (2017) has a 16% stronger contribution to TSI variability in this wavelength range compared to the forcing used in the 5th Phase of the Coupled Model Intercomparison Project (CMIP5).
To conclude, solar activity since the late 19th century was relatively high but not exceptional in the context of the past 9 kyr (high confidence). The associated global mean ERF is in the range of ā0.06 to +0.08 W mā2 (Section 7.3.4.4).
Within the well-studied mid-Pliocene Warm Period (MPWP, also called the mid-Piacenzian Warm Period, 3.3ā3.0 Ma), the interglacial period KM5c (3.212ā3.187 Ma) has become a focus of research because its orbital configuration, and therefore insolation forcing, was similar to present (global mean insolation = ā0.022 W mā2 relative to modern; Haywood et al., 2013), allowing for the climatic state associated with relatively high atmospheric CO2 to be assessed with fewer confounding variables.
Emile-Geay, J. et al., 2016: Links between tropical Pacific seasonal, interannual
and orbital variability during the Holocene. Nature Geoscience, 9, 168,
doi:10.1038/ngeo2608.
Laskar, J., A. Fienga, M. Gastineau, and H. Manche, 2011: La2010: a new
orbital solution for the long-term motion of the Earth. Astronomy &
Astrophysics, 532, A89, doi:10.1051/0004-6361/201116836.
Loulergue, L. et al., 2008: Orbital and millennial-scale features of atmospheric
CH4 over the past 800,000 years. Nature, 453, 383, doi:10.1038/nature06950.
Mollier-Vogel, E., G. Leduc, T. Bƶschen, P. Martinez, and R.R. Schneider, 2013:
Rainfall response to orbital and millennial forcing in northern Peru over
the last 18ka. Quaternary Science Reviews, 76, 29ā38, doi:10.1016/j.
quascirev.2013.06.021.
That was from the first 12 of 95 appearances of the term "orbital" in The Physical Science Basis. I can carry on if you'd like.