the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Response of Late-Eocene warmth to incipient glaciation on Antarctica
Abstract. The Eocene-Oligocene Transition (EOT) is marked by a sudden δ18O excursion occurring in two distinct phases, ~500 ky apart. These phases signal a shift from the warm Middle- to Late-Eocene greenhouse climate to cooler conditions, with global surface air temperatures decreasing by 3–5 °C and the emergence of the first continent-wide Antarctic Ice Sheet (AIS). While ice-sheet modelling suggests that ice sheet growth can be triggered by declining pCO2, it still remains unclear how this transition has been initiated, in particular the first growth phase that seems to be related to oceanic and atmospheric cooling rather than ice sheet growth. Recent climate model simulations of the Late-Eocene show improved accuracy but depict climatic conditions that are not conducive to the survival of incipient ice sheets throughout the summer season. This study therefore examines whether it is plausible to develop ice sheets of sufficient scale to trigger the feedback mechanism(s) required to disrupt the atmospheric regime above the Antarctic continent during warm Late-Eocene summers and establish more favourable conditions for ice expansion. We thereby aim to assess the stability of an incipient AIS under varying radiative, orbital and cryospheric forcing. To do so, we evaluate Community Earth System Model 1.0.5 simulations, using a 38 Ma geo- and topographical reconstruction, considering different radiative (4 and 2 pre-industrial carbon) and orbital (present-day and low summer insolation) forcings. The climatic conditions prevailing during (the lead-up to) the EOT can be characterised as extremely seasonal and monsoonal, featuring a short yet intense summer period and contrasting cold winters — highly inhospitable to ice sheet growth for most of the continent, as limited snow accumulation is expected to survive the summer season. A narrow convergence zone with moist convection around the region where sub-cloud equivalent potential temperature is high is shown to exhibit a ring-like structure, advecting moist surface air advected from the Southern Ocean. This advection leads to high values of moist static energy and subsequent precipitation in these regions. To assess the influence of cryospheric forcing, we conducted another simulation, with regional, moderately-sized ice sheets imposed on the continent, to investigate their stability and influence on the atmospheric circulation. Regionally, these relatively small ice sheets respond strongly to radiative and orbital forcing, and demonstrate remarkably favourable self-sustaining and even expansion potential under 2 PIC and low summer insolation conditions. This emphasises a significant hysteresis effect for local and/or regional ice sheets on the Antarctic continent, suggesting the potential for a significant volume of ice on the Antarctic continent without an imminent full glaciation prior to the EOT.
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RC1: 'Comment on cp-2024-30', Anonymous Referee #1, 02 Jul 2024
Vermeulen et al. conduct a ice sheet model and climate model simulation, and analyze a set of existing climate model simulations, to investigate incipient Antarctic Ice Sheet (AIS) stability under a warm and monsoonal late Eocene climate which is thought to be inhospitable to ice sheet growth. They hypothesize that a moderate-size AIS could have disrupted this inhospitable climate, thereby triggering a feedback mechanism for glacial expansion at the EOT. They test this hypothesis and find that the prescribed ice sheets do not significantly disrupt this warm monsoonal climate, but their ice sheets still demonstrate the potential to self-sustain and even grow (i.e., they calculate positive surface mass balance, SMB).
The manuscript has clear prose and is well organized. The hypothesis is interesting, and their investigation contributes to this scientific field. The impact of the imposed ice sheets on the modeled climate is extensively described and discussed, supporting their first finding (that the imposition of these ice sheets into the model does not significantly disrupt the preexisting climate). However, I thought that the second finding (that these ice sheets are able to self-sustain and even grow) was missing an important discussion: what factor is dictating these positive SMB calculations? Lots of moisture? The calculation type (e.g., a PDD scheme or energy balance scheme? And does this relate to whether summer intensity vs summer duration is more impactful on ice sheet stability? E.g., Raymo & Huybers, 2008). The authors state many times that the monsoonal/seasonal late Eocene warm climate is inhospitable to ice growth due to limited summer snow accumulation -- but in the end, they find that this climate is not, in fact, inhospitable to ice growth. So I’m curious - what was that original assumption based on? Is it simply wrong? The authors don’t go back and reassess that claim.
I must admit that I mostly think about paleo ice sheet stability and I lack expertise in atmospheric circulation dynamics. Given that caveat, I wonder if portions of the Results & Discussions sections could be shortened or streamlined. I was often confused about the relevance of the detailed analyses/descriptions of model climate dynamics (although this may have more to do with lack of expertise rather than the quality of the manuscript). I very much appreciated sentences that spelled out the relevancy of the various analyses (for example, L319, “This is a crucial part of the Antarctic Eocene climate, as the circulation pattern basically redirects the storm track… resulting in high precipitation over DML..”).
I also wondered fairly frequently while reading this manuscript about ‘false precision’, i.e., how much of these details around wind direction and seasonality are dictated by uncertainties in the model or boundary conditions, rather than a robust paleo-climate feature. The authors do address this a bit in Sect 4.1 by comparing their results to other models, though; I simply mention this as food for thought.
In sum, I recommend this paper for publication, but found the ice sheet analyses a bit underdeveloped relative to the stated premise of the paper.
A few small comments:
- Abstract: L13-16 is restating L7? And it seems like that sentence is stating existing information - from Baatsen et al 2024 - but then the next sentence is a finding of this work?
- Some parentheses are unnecessary and break up the flow of the narrative (for example, L51, L64, L81, etc.)
- L84: I found the ‘ab- and presence’ to be jarring, similarly ‘topo-and geography’
- L299: Here and elsewhere, re: late Eocene seasonality/monsoonal conditions, I’m not always sure what is a reference to Baatsen et al 2024 versus new findings from this study.
Citation: https://doi.org/10.5194/cp-2024-30-RC1 -
AC1: 'Reply on RC1', Dennis H.A. Vermeulen, 22 Jul 2024
Vermeulen et al. conduct a ice sheet model and climate model simulation, and analyze a set of existing climate model simulations, to investigate incipient Antarctic Ice Sheet (AIS) stability under a warm and monsoonal late Eocene climate which is thought to be inhospitable to ice sheet growth. They hypothesize that a moderate-size AIS could have disrupted this inhospitable climate, thereby triggering a feedback mechanism for glacial expansion at the EOT. They test this hypothesis and find that the prescribed ice sheets do not significantly disrupt this warm monsoonal climate, but their ice sheets still demonstrate the potential to self-sustain and even grow (i.e., they calculate positive surface mass balance, SMB).
The manuscript has clear prose and is well organized. The hypothesis is interesting, and their investigation contributes to this scientific field. The impact of the imposed ice sheets on the modeled climate is extensively described and discussed, supporting their first finding (that the imposition of these ice sheets into the model does not significantly disrupt the preexisting climate).
AR: Thank you for your positive evaluation.
However, I thought that the second finding (that these ice sheets are able to self-sustain and even grow) was missing an important discussion: what factor is dictating these positive SMB calculations? Lots of moisture? The calculation type (e.g., a PDD scheme or energy balance scheme? And does this relate to whether summer intensity vs summer duration is more impactful on ice sheet stability? E.g., Raymo & Huybers, 2008). The authors state many times that the monsoonal/seasonal late Eocene warm climate is inhospitable to ice growth due to limited summer snow accumulation -- but in the end, they find that this climate is not, in fact, inhospitable to ice growth. So I’m curious - what was that original assumption based on? Is it simply wrong? The authors don’t go back and reassess that claim.
AR: That’s a good point; we will add this to the final version of the manuscript.
I must admit that I mostly think about paleo ice sheet stability and I lack expertise in atmospheric circulation dynamics. Given that caveat, I wonder if portions of the Results & Discussions sections could be shortened or streamlined. I was often confused about the relevance of the detailed analyses/descriptions of model climate dynamics (although this may have more to do with lack of expertise rather than the quality of the manuscript). I very much appreciated sentences that spelled out the relevancy of the various analyses (for example, L319, “This is a crucial part of the Antarctic Eocene climate, as the circulation pattern basically redirects the storm track… resulting in high precipitation over DML..”).
AR: We agree. This is also mentioned in RC2, so we will go over the Results and Discussion sections again to make those more concise.
I also wondered fairly frequently while reading this manuscript about ‘false precision’, i.e., how much of these details around wind direction and seasonality are dictated by uncertainties in the model or boundary conditions, rather than a robust paleo-climate feature. The authors do address this a bit in Sect 4.1 by comparing their results to other models, though; I simply mention this as food for thought.
AR: That indeed is a good question. In our opinion, large seasonality is a robust feature that is also visible in other models, as indeed is discussed in Sect. 4.1. We did not extensively compare (surface or 850 hPa) pressure to other models, but qualitatively it makes sense that during JJA a (thermal) high pressure area is formed over the (East-)Antarctic continent and a (thermal) low pressure area over the Weddell Sea. Furthermore, this dipole is a robust feature in all of our scenarios. Of course, this could be model-dependent, so we will elaborate a bit more on this nuance in Sect. 4.1.
In sum, I recommend this paper for publication, but found the ice sheet analyses a bit underdeveloped relative to the stated premise of the paper. A few small comments:
- Abstract: L13-16 is restating L7? And it seems like that sentence is stating existing information - from Baatsen et al 2024 - but then the next sentence is a finding of this work?
AR: We agree and we will correct this. - Some parentheses are unnecessary and break up the flow of the narrative (for example, L51, L64, L81, etc.)
AR: We will check again where parentheses disturb the flow of reading. - L84: I found the ‘ab- and presence’ to be jarring, similarly ‘topo-and geography’
AR: We will correct this. - L299: Here and elsewhere, re: late Eocene seasonality/monsoonal conditions, I’m not always sure what is a reference to Baatsen et al 2024 versus new findings from this study.
AR: Good point, we will make this clearer.
Citation: https://doi.org/10.5194/cp-2024-30-AC1 - Abstract: L13-16 is restating L7? And it seems like that sentence is stating existing information - from Baatsen et al 2024 - but then the next sentence is a finding of this work?
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RC2: 'Comment on cp-2024-30', Anonymous Referee #2, 08 Jul 2024
This manuscript performed several paleoclimate simulations to study the Antarctic climate conditions during the EOT with focuses on the role of Earth’s orbital forcing and the impact from incipient ice sheets. The authors’ simulations suggest strong seasonal and monsoonal climate over the Antarctica with intense summer warming that prevents large-scale snow accumulation. When imposing the ice sheets derived from offline ice sheet model, the authors find regional positive surface mass balance, indicating the potential of growth of the incipient ice sheets. The authors’ results suggest the potential for the existence of substantial volume of ice before the EOT.
The research topic is of high relevance and fits nicely with Climate of the Past. I enjoyed reading the abstract and the introduction very much. I think the manuscript need revision to better highlight its key points and novelty before it can be published in Climate of the Past. Below are my major comments on Results and Discussion sections, along with a few minor comments and editing suggestions.
Major comments:
- I think the Results and Discussion sections could be improved to highlight the most important findings and novelty from the present study. In its current form, the Results and Discussion simply lists many detailed descriptions of simulation results without sufficient summary of the main points of each subsection/paragraph, making it very difficult for the readers to follow.
- At places, the manuscript is very descriptive and lacks in-depth analysis/understanding on the results. For example, which processes drive the SMB? If the incipient ice sheets were imposed over other regions (e.g., more interior), should we expect similar SMB (based on our understanding of the physical processes)?
Minor comments:
- Title needs to be revised. The manuscript is focusing on Antarctica, not the global climate. I suggest the authors revise the title to reflect the regional focus of the present manuscript.
- Line 17: check the writing of “is high is shown”.
- Line 97: the better performance of the newer models in Lunt et al. 2021 is not attributed to the “higher resolution”. Instead, it may be attributable to the improved model physics (e.g., Zhu, Poulsen, & Tierney, 2019).
- Line 118: ‒1.8 ℃ (not 1.8 ℃).
- Table 1: check the units of obliquity and precession.
- Subsection title “Ice sheet Stability” could be revised to, for example, “Ice sheet sustainability”.
- Line 338: delete one redundant “)”
- The use of many region names, such as Dronning Maud Land, Marie Byrd Land, may be hard for some readers who are not familiar with the Antarctica geology to follow. Please consider labeling names of key regions in Figure 1.
Citation: https://doi.org/10.5194/cp-2024-30-RC2 -
AC2: 'Reply on RC2', Dennis H.A. Vermeulen, 22 Jul 2024
This manuscript performed several paleoclimate simulations to study the Antarctic climate conditions during the EOT with focuses on the role of Earth’s orbital forcing and the impact from incipient ice sheets. The authors’ simulations suggest strong seasonal and monsoonal climate over the Antarctica with intense summer warming that prevents large-scale snow accumulation. When imposing the ice sheets derived from offline ice sheet model, the authors find regional positive surface mass balance, indicating the potential of growth of the incipient ice sheets. The authors’ results suggest the potential for the existence of substantial volume of ice before the EOT.
The research topic is of high relevance and fits nicely with Climate of the Past. I enjoyed reading the abstract and the introduction very much.
AR: Thank you for your positive evaluation of the abstract and the introduction.
I think the manuscript need revision to better highlight its key points and novelty before it can be published in Climate of the Past. Below are my major comments on Results and Discussion sections, along with a few minor comments and editing suggestions.
Major comments:
- I think the Results and Discussion sections could be improved to highlight the most important findings and novelty from the present study. In its current form, the Results and Discussion simply lists many detailed descriptions of simulation results without sufficient summary of the main points of each subsection/paragraph, making it very difficult for the readers to follow.
AR: We agree, and since this is also mentioned in RC1, we will make the Result and Discussion sections more concise. Furthermore, we will add summary paragraphs at the end of each subsection in the Results section to highlight the most important findings. - At places, the manuscript is very descriptive and lacks in-depth analysis/understanding on the results. For example, which processes drive the SMB? If the incipient ice sheets were imposed over other regions (e.g., more interior), should we expect similar SMB (based on our understanding of the physical processes)?
AR: This point is also mentioned in RC1. Specifically for the section about the ice sheets and SMB we will add a clearer interpretation, but we will go over the whole Discussion section again to make it less descriptive.
Minor comments:
- Title needs to be revised. The manuscript is focusing on Antarctica, not the global climate. I suggest the authors revise the title to reflect the regional focus of the present manuscript.
AR: We interpret ‘on Antarctica’ at the end of the title as applying to the title as a whole, but apparently this causes confusion. We will think of a better way of putting emphasis on the regional scale of the study. - Line 17: check the writing of “is high is shown”.
AR: We will correct this. - Line 97: the better performance of the newer models in Lunt et al. 2021 is not attributed to the “higher resolution”. Instead, it may be attributable to the improved model physics (e.g., Zhu, Poulsen, & Tierney, 2019).
AR: Indeed, thank you for pointing this out. We will correct this. - Line 118: ‒1.8 ℃ (not 1.8 ℃).
AR: We will correct this. - Table 1: check the units of obliquity and precession.
AR: Indeed, this should not be [°C] but only [°]. Thank you for your keen eye. - Subsection title “Ice sheet Stability” could be revised to, for example, “Ice sheet sustainability”.
AR: We agree the topic is more on sustainability than stability, so we will correct this. - Line 338: delete one redundant “)”
AR: We will correct this. - The use of many region names, such as Dronning Maud Land, Marie Byrd Land, may be hard for some readers who are not familiar with the Antarctica geology to follow. Please consider labeling names of key regions in Figure 1.
AR: We were under the impression that this was already the case, but we used an old version of Figure 1. Thank you for pointing out; we will include the newer version.
Citation: https://doi.org/10.5194/cp-2024-30-AC2 - I think the Results and Discussion sections could be improved to highlight the most important findings and novelty from the present study. In its current form, the Results and Discussion simply lists many detailed descriptions of simulation results without sufficient summary of the main points of each subsection/paragraph, making it very difficult for the readers to follow.
Data sets
4PIC, 2PIC/s, 2PIC/l and 2PIC/li data set Dennis Vermeulen, Michiel Baatsen, and Anna von der Heydt https://doi.org/10.24416/UU01-A0VMKZ
Model code and software
4PIC, 2PIC/s, 2PIC/l and 2PIC/li analysis code Dennis Vermeulen, Michiel Baatsen, and Anna von der Heydt https://doi.org/10.24416/UU01-A0VMKZ
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