The arrangement of continents and oceans has an important effect on climate, from regional to global scales. Throughout Earth's history, paleogeography has shaped key aspects of the climate system, including oceanic and atmospheric circulation, and the carbon cycle. An example in the ocean is the Antarctic Circumpolar Current (ACC), which could only develop after ocean passages opened 30 million years ago . The continental configuration also influences atmospheric circulation. It has been shown that through the geological time scale, paleogeography plays the most important role in influencing winter storm distribution. Also, monsoonal circulation is shown to be dependent on the continental configuration. For example, continents with a C-shape land distribution at the tropics, two continental landmasses at the two sides of the Equator connected with a bridging land, favours monsoon development . In an other aspect, when the majority of continents are located at the tropics and experience tropical precipitation, silicate weathering can effectively remove CO₂ from the atmosphere inducing a cooling and ice accumulation . Thus, tectonic changes have the capacity to trigger ice ages, through their influence on the carbon cycle. In paleoclimate research, attributing different forcing mechanisms is essential for understanding climate dynamics and for making conclusions transferable to also future scenarios. Moreover, studying past warm climates are of high relevance because of their information on how our climate system worked under high CO₂ concentrations.

Here, we consider the role of the early Eocene paleogeography on large-scale circulation patterns. The time period we focus on is the Early Eocene Climatic Optimum (EECO, ∼ 53–51 Ma), which is characterised by exceptional warmth (approximately 10–16 °C warmer than pre-industrial climate) , low meridional temperature gradients and high CO₂ concentrations (around 1600 ppm) . There has been coordinated effort amongst modelling and proxy groups, under the initiative known as the Deep-Time Model Intercomparison Project (DeepMIP), to increase our understanding of this period in Earth climate history . In our study, we consider the paleogeography used in the first phase of DeepMIP, from the early Eocene, the Ypresian stage representing the Earth between ∼ 55 to ∼ 50 Ma (see Fig. ) .

The most notable features of this early Eocene paleogeography are the wider Pacific Basin and thus narrower Atlantic Ocean, the tropical location of the Indian subcontinent and the lack of the Himalayas. Moreover, an important characteristic in the Northern Hemisphere is the connection between the Arctic and the Tethys Ocean through the shallow West-Siberian Sea . During the early Eocene there were no currents connecting the Arctic to the Pacific basin, as the Bering Strait was closed, thus oceanic heat transport from the tropics to the Arctic flow through the West Siberian Sea . This is underlined by proxy records showing that the mean annual sea surface temperature in the Arctic Ocean and the West-Siberian Sea was very similar and at least 20 °C . In the Southern Hemisphere, the location of the Antarctic continent was very similar to modern conditions, but both Australia and South America were located more to the south, causing the Drake Passage and the Tasman Gateway to be narrow and shallow, i.e. oceanographically closed (negligible water, heat or mass transport through it) and thus inhibiting the development of the ACC.

Previous analysis of the DeepMIP ensemble investigated the effects of CO₂ and non-CO₂ boundary conditions (paleogeography, lack of ice sheets, vegetation, rivers) on meridional heat transport (MHT) processes . The study showed that in the model simulations the total MHT does not change much due to the early Eocene non-CO₂ boundary conditions. Nevertheless, there are changes in the atmospheric heat transport (AHT), and in the ocean heat transport (OHT) (Fig. a). The AHT shifts slightly toward the northern hemisphere and the OHT shifts towards the southern hemisphere. The later one is likely related to the fact that, in most DeepMIP models' deep-water formation occurs in the Southern Ocean . Thus, due to the change in deep-water formation, respective to modern days, the hemispheric distribution of OHT changes as well. also showed that the partitions of AHT, namely the heat transport through different physical processes such as the atmospheric meridional overturning circulation (MOC), the stationary (SE) and the transient eddies (TE), also change due to the non-CO₂ paleo boundary conditions. Most notable is the increase in TE heat transport at the northern mid-latitudes, and the compensating decrease in SE heat transport (Fig. b). Meanwhile, over the southern mid-latitudes, a decrease in TE heat transport is identified in the data (Fig. b), which is not compensated by other processes, thus mainly responsible for the decrease in AHT over the Southern Hemisphere. The Southern Hemispheric AHT decrease is also linked to the aforementioned increase in OHT, consistent with the Bjerknes compensation mechanism.

In this study, we further investigate the changes seen in the heat transport analysis , and analyze how the non-CO₂ paleo boundary conditions, most notably the early Eocene paleogeography, influences large-scale circulation patterns, especially at the mid-latitudes where AHT and its differences are maximal. We are focusing primarily on mid-latitude circulations patters, cyclones and blockings. For the analysis we use data from CESM1.2 model simulations, which are the extensions of the DeepMIP simulations .

Our goals in this paper are:

To understand the early Eocene global circulation and climate. The better understanding of large-scale circulation patterns and their changes related to paleogeography helps the interpretation of proxy records.

This paper is structured as follows. In Sect. , we introduce the climate model simulations and the identifying algorithms for cyclones and blockings. In Sect. , we provide an overview of our results considering the Northern and Southern Hemisphere. In Sect. , we discuss our findings and the wider context of the dynamic changes and finish with a summary and our conclusions.

The analysis of the cyclone tracks shows a change in spatial pattern in both Hemispheres between the pre-industrial and the 1 × CO₂ simulations (Fig. ). Under pre-industrial conditions, mid-latitude cyclones in the Northern Hemisphere are concentrated around two distinct areas over the Pacific and Atlantic Oceans (Fig. a). On the other hand, Southern Hemisphere cyclone tracks distribute around Antarctica in a O shape (Fig. c). However, under early Eocene conditions, the spatial distribution of cyclone tracks becomes more balanced as the distinction between the Pacific and Atlantic paths becomes less pronounced (Fig. b). Also, there is an increase in cyclone tracks passing over land areas, especially over Europe. In contrast, in the Southern Hemisphere there are fewer cyclone tracks under early Eocene conditions compared to pre-industrial, and the track climatology shows several small density centres around Antarctica (Fig. d), which is due to the more fragmented Southern Ocean basin. These changes are also reflected in the number of cyclones (Fig. ), with an average annual increase of 36 % in the Northern Hemisphere and a decrease of 32 % in the Southern Hemisphere. This makes the cyclone distribution between the hemispheres more balanced, although the average annual cyclone number is still higher in the south than in the north. Moreover, there is a decrease in the annual cyclone number globally under early Eocene conditions compared to pre-industrial. The changes are consistent through all seasons, but most prominent during each hemisphere's winter and spring season. The heat, transported by the mid-latitude cyclones, is what we call transient eddy heat transport in the heat transport analysis. Thus these findings are in line with the increased transient eddy heat transport in the northern mid-latitudes and the decreased transient eddy heat transport in the southern mid-latitudes, respectively (Fig. ).

Early Eocene blocking frequencies in the northern mid-latitudes show a general decrease and a shift from modern Europe to the east to the West-Siberian Sea (Fig. a and b). This is also in line with the heat transport analysis, showing a decrease in the stationary eddy heat transport at the northern mid-latitudes (see Fig. ). The eastward shift of blocking frequency is in line with the eastward shift of the cyclone tracks to the West-Siberian Sea since the eastern boundary of cyclone tracks is a common region of blocking formation. The heat transport analysis does not show large changes in the stationary eddy heat transport at the southern mid-latitudes, which is reflected in the visually similar blocking frequencies in the early Eocene and in the pre-industrial period (Fig. c and d). Nevertheless, in the early Eocene the southern blockings have a more dispersed spatial distribution around Antarctica than in the pre-industrial climate.

Mid-latitude cyclones play a key role in the hydroclimate as they transport moisture and are associated with a large portion of extratropical precipitation. They generally produce more precipitation over oceanic regions than over land due to greater moisture availability. Moreover, enhanced precipitation also occurs when mid-latitude cyclones encounter orographic barriers, and orographic lifting takes place. For qualitative measure we plotted boreal winter (December, January and February) and southern winter (June, July and August) cyclone track densities along the respective seasonal precipitation fields (Figs.  and ). In the Northern Hemisphere, cyclones are more prominent during winter and they precipitate along the Tethys Ocean and the West-Siberian Sea, bringing moisture to an area which is dryer under modern conditions. Moreover, during the early Eocene the west coast of North America is experiencing high precipitations, which is probably due to a combination of the higher number of cyclone tracks in the region and the cyclones' interaction with orography. In the Southern Hemisphere the most cyclones occure during the southern winter (see Fig. ) and they bring precipitation to the western coast of Australia and South America (Fig. ). Both of these regions are located souther in the early Eocene topography than in modern times, thus more in the paths of the mid-latitude cyclones.

The meridional heat transport analysis identified three main characteristics (Fig. ) when comparing the pre-industrial and 1 × CO₂ Eocene simulations:

increase of transient eddy heat transport at the northern mid-latitudes

These characteristics are due to the paleo boundary conditions, most notably the different configuration of continents and their orography. The cyclone and blocking analysis showed that the increase of transient eddy transport over the northern mid-latitudes is due to the increase in cyclone numbers, the decrease of stationary eddy transport is due to less frequent blockings at the northern mid-latitudes. Moreover, the southern mid-latitude transient eddy heat transport decrease is connected to the decrease of cyclone numbers. This change in the Southern Hemisphere is not compensated by other processes in the atmosphere, thus effects the AHT. Nevertheless, it is compensated by the OHT through the Bjerknes compensation. Thus, the total MHT remains very similar in the pre-industrial and 1 × CO₂ Eocene simulations.

The changes in paleogeography influence the air-sea interactions in the climate system. In the Northern Hemisphere, the Tethys Ocean and the West Siberian Sea served as additional sources of heat and moisture. This effect was especially pronounced during winter, when the thermal contrast between the epicontinental West Siberian Sea and the neighbouring land areas of Europe and Asia was highest. Comparing the latent and sensible heat fluxes over the Eurasian region reveals that over the West Siberian Sea the two fluxes are of comparable magnitude, thus the Western Siberian Sea enhances thermal contrast and act as a moisture source, whereas over the Tethys Ocean the surface energy exchange is dominated by latent heat flux (Fig. ). This configuration enhances baroclinic instability in this region, which we saw as an increase in cyclone numbers.

In the Southern Hemisphere, the most significant changes in paleogeography compared to modern are the nearly closed Drake Passage and Tasman Gateway. These two narrow and shallow straights prevented the development of the wind driven circumpolar ocean current around Antarctica, the Antarctic Circumpolar Current (ACC). The wind field at the lowest model level, which is following the surface, is indeed weaker in the 1 × CO₂ Eocene simulation than under modern circumstances (Fig. a and b). Under pre-industrial conditions the ACC is crucial in maintaining the strong oceanic temperature gradient between cold polar and warmer subtropical waters. This, in turn, enhances meridional temperature gradients in the lower atmosphere, which, through the thermal wind relationship, increases baroclinic instability, the fuel of mid-latitude cyclones. Under early Eocene conditions, without the ACC, the baroclinic instability decreases in the region, which is also evident by the weaker Southern Hemispheric jet stream (Fig. c and d). Overall, the ACC is dynamically connected to the Southern Hemispheric mid-latitude cyclones, and its absence in the 1 × CO₂ Eocene simulation is in line with the fewer cyclone number in the region (Fig. ). showed that in modern climate the Southern Hemispheric jet stream is stronger than its northern counterpart, and the Southern Hemisphere is stormier. In our results, we found that under early Eocene conditions the signal between the hemispheres are more balanced, due to the increase in Northern Hemispheric storms and the decrease in Southern Hemispheric storms.

We conclude that through air-sea interactions, the paleogeography notably influences atmospheric large-scale circulation patterns. Under early Eocene circumstances, this influence meant increased mid-latitude baroclinity over the Northern, but decresed baroclinicity over the Southern Hemisphere, which results in a more balanced heat transport among hemispheres and atmospheric processes than in the pre-industrial climate. In the Northern Hemisphere, the increased baroclinic instability resulted in increased heat transport by large eddies, nevertheless this process seems to be compensated by less heat transport via blocking systems. On the other hand, in the Southern Hemisphere the decreased baroclinity and thus less heat transport via mid-latitude cyclones is not compensated by other processes in the atmosphere. The net effect of paleogeography related changes on AHT, is a shift towards the Northern Hemisphere, which is, in turn, compensated by a southward shift in OHT. This increase in southward OHT is connected to the southern deep-water formation under early Eocene paleo boundary conditions . The compensation is needed, because from the energetic perspective, a change in AHT needs to be compensated by the OHT to fulfil the top of the atmosphere energetic constraint on MHT. Thus, under the early Eocene conditions due to the AHT changes, the ocean needs to increase its heat transport over the Southern Hemisphere, which favours the development of a Southern Hemisphere-driven overturning circulation .

This study shows that the early Eocene paleogeography affects atmospheric large scale processes and ocean circulation both in a direct and indirect way. For the ocean, the direct effects consist of strait geometry, and the indirect effects include the heat transport processes' influence on deep-water formation. Our results support the hypothesis that under early Eocene boundary conditions the Southern Ocean deep-water formation is more likely to fulfil the energetic constraints of the climate system.

In this paper, we investigated the role of early Eocene orography on large scale circulation patterns. We compared atmosphere only CESM model simulations describing pre-industrial conditions and modern day orography versus 1 × CO₂ simulations containing early Eocene boundary conditions including paleogeography, the lack of ice sheets, different vegetation and rivers. For ocean boundary conditions, we used the SST values form DeepMIP CESM simulations. Our research was motivated by a meridional heat transport analysis, which showed changes in the heat transport of transient eddies (cyclones) and stationary eddies (blockings) at the mid-latitudes. We found that the increase in transient eddy transport in the northern mid-latitudes is connected to the increase in cyclone numbers. In the early Eocene continental configuration, the presence of the warm and shallow epicontinental West Siberian Sea enhances air-sea interactions and acts as an extra heat and moisture source, which increases the baroclinic instability in the region. The change in cyclone numbers and paths also resulted in more moisture transport into the Asian continental interior. On the other hand, we found that the increased heat transport through cyclones is compensated by a decreased fraction of blocking under early Eocene conditions. Over the Southern Hemisphere, we found a decrease in mid-latitude cyclone numbers, which is connected to the decrease in temperature gradient between polar and subpolar surface water due to the lack of the ACC. Our results suggest, that the decrease in southern AHT infers the increase in OHT, which is achieved by the Southern Hemisphere-driven overturning circulation in the ocean. We conclude that under early Eocene conditions the atmospheric heat transport processes are more symmetric between the hemispheres than in the pre-industrial climate. This is achieved through air-sea-land interactions, where the pealoegeography has an important role in forming the large scale circulation both in the atmosphere and in the ocean. The next step of this research is the investigation of early Eocene cyclones in a high CO₂ simulation, which is representing the paleo conditions more accurately. Our previous analysis showed a slight increase in transient eddy heat transport in high CO₂ simulations. Thus, we are interested to see if this is achieved through more frequent cyclones or by more heat transport per cyclone, through the warmer and moister atmosphere of the EECO climate.