Preprints
https://doi.org/10.5194/egusphere-2022-184
https://doi.org/10.5194/egusphere-2022-184
22 Apr 2022
 | 22 Apr 2022

Reconstructing Holocene temperatures in time and space using paleoclimate data assimilation

Michael P. Erb, Nicholas P. McKay, Nathan Steiger, Sylvia Dee, Chris Hancock, Ruza F. Ivanovic, Lauren J. Gregoire, and Paul Valdes

Abstract. Paleoclimatic records provide valuable information about Holocene climate, revealing aspects of climate variability for a multitude of sites around the world. However, such data also possess limitations. Proxy networks are spatially uneven, seasonally biased, uncertain in time, and present a variety of challenges when used in concert to illustrate the complex variations of past climate. Paleoclimatic data assimilation provides one approach to reconstructing past climate that can account for the diverse nature of proxy records while maintaining the physics-based covariance structures simulated by climate models. Here, we use paleoclimate data assimilation to create a spatially-complete reconstruction of temperature over the past 12,000 years using proxy data from the Temperature 12k database and output from transient climate model simulations. Following the last glacial period, the reconstruction shows Holocene temperatures warming to a peak near 6,400 years ago followed by a slow cooling toward the present day, supporting a preindustrial global mean surface temperature maximum during the mid-Holocene. Sensitivity tests show that if proxies have an overlooked summer bias, some apparent mid-Holocene warmth could actually represent summer trends rather than annual mean trends. Regardless, the potential effects of proxy seasonal biases are insufficient to align reconstructed global mean temperature with the warming trends seen in transient model simulations.

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Journal article(s) based on this preprint

15 Dec 2022
| Highlight paper
Reconstructing Holocene temperatures in time and space using paleoclimate data assimilation
Michael P. Erb, Nicholas P. McKay, Nathan Steiger, Sylvia Dee, Chris Hancock, Ruza F. Ivanovic, Lauren J. Gregoire, and Paul Valdes
Clim. Past, 18, 2599–2629, https://doi.org/10.5194/cp-18-2599-2022,https://doi.org/10.5194/cp-18-2599-2022, 2022
Short summary Co-editor-in-chief
Michael P. Erb, Nicholas P. McKay, Nathan Steiger, Sylvia Dee, Chris Hancock, Ruza F. Ivanovic, Lauren J. Gregoire, and Paul Valdes

Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2022-184', Anonymous Referee #1, 01 Jun 2022
    • AC1: 'Reply on RC1', Michael Erb, 19 Sep 2022
  • CC1: 'Comment on egusphere-2022-184', Jessica Tierney, 03 Jul 2022
    • AC3: 'Reply on CC1', Michael Erb, 22 Sep 2022
  • RC2: 'Comment on egusphere-2022-184', Anonymous Referee #2, 07 Jul 2022
    • AC2: 'Reply on RC2', Michael Erb, 19 Sep 2022

Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2022-184', Anonymous Referee #1, 01 Jun 2022
    • AC1: 'Reply on RC1', Michael Erb, 19 Sep 2022
  • CC1: 'Comment on egusphere-2022-184', Jessica Tierney, 03 Jul 2022
    • AC3: 'Reply on CC1', Michael Erb, 22 Sep 2022
  • RC2: 'Comment on egusphere-2022-184', Anonymous Referee #2, 07 Jul 2022
    • AC2: 'Reply on RC2', Michael Erb, 19 Sep 2022

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
ED: Publish subject to minor revisions (review by editor) (22 Sep 2022) by Steven Phipps
AR by Michael Erb on behalf of the Authors (28 Oct 2022)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (23 Nov 2022) by Steven Phipps
AR by Michael Erb on behalf of the Authors (23 Nov 2022)

Journal article(s) based on this preprint

15 Dec 2022
| Highlight paper
Reconstructing Holocene temperatures in time and space using paleoclimate data assimilation
Michael P. Erb, Nicholas P. McKay, Nathan Steiger, Sylvia Dee, Chris Hancock, Ruza F. Ivanovic, Lauren J. Gregoire, and Paul Valdes
Clim. Past, 18, 2599–2629, https://doi.org/10.5194/cp-18-2599-2022,https://doi.org/10.5194/cp-18-2599-2022, 2022
Short summary Co-editor-in-chief
Michael P. Erb, Nicholas P. McKay, Nathan Steiger, Sylvia Dee, Chris Hancock, Ruza F. Ivanovic, Lauren J. Gregoire, and Paul Valdes

Data sets

Holocene temperature reconstruction using paleoclimate data assimilation Michael P. Erb, Nicholas P. McKay, Nathan Steiger, Sylvia Dee, Chris Hancock, Ruza F. Ivanovic, Lauren J. Gregoire, and Paul Valdes https://doi.org/10.5281/zenodo.6426332

Model code and software

Code for the Holocene reconstruction Michael P. Erb and Nathan Steiger https://github.com/Holocene-Reconstruction/Holocene-code

Michael P. Erb, Nicholas P. McKay, Nathan Steiger, Sylvia Dee, Chris Hancock, Ruza F. Ivanovic, Lauren J. Gregoire, and Paul Valdes

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Latest update: 02 Sep 2024
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The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.

The manuscript presents a reconstruction of global temperature spanning the Holocene, which extends the scope of previous exercises in palaeoclimate data assimilation. The resulting reconstruction presents new insights into changes in global temperature over this period. Most notably, it confirms the results of previous studies that have shown a global cooling trend over the past 6,000 years. It also shows that a cooling trend is found even after allowing for potential biases in the proxies. These results are likely to be of considerable interest to the broader geoscience community.
Short summary
To look at climate over the past 12000 years, we reconstruct spatial temperature using natural climate archives and information from model simulations. We see mild global mean warm around 6000 years ago, which differs somewhat from past reconstructions. If more of our data represents summer values, this could explains some of the observed temperature change, but it still wouldn't explain the large difference between many reconstructions and climate models over this period.