Unraveling 66 million years of climate history from ocean sediments

Based on extensive data analysis, an international team publishes global reference curve in the academic journal Science

"Our goal was to create a new reference of past climate over the last 66 million years, which not only incorporates the highest-resolution data but is also more accurately dated," explains first author Thomas Westerhold of MARUM. "We now know more accurately when it was warmer or colder on the planet and we also have a better understanding of the underlying dynamics."

"Our mathematical analyses revealed what is at first invisible in the sediment - the hidden relationships and recurring patterns in the climate," says Norbert Marwan of PIK. "So the view into the past is also a glimpse into the future. We can learn something about the staggeringly rapid anthropogenic changes of our present century from the slow natural climate fluctuations occurring over millions of years." The climatic changes of the past 66 million years can be studied like a colorful barcode. {module INSIDE STORY}

Layers of sediment on the ocean floor have been cored across the world for more than five decades through internationally coordinated scientific ocean drilling expeditions of the International Ocean Discovery Program (IODP) and its predecessor programs (DSDP, ODP, IODP). By studying these sediments and the microfossils within, scientists are able to reconstruct and analyze global climate changes into the distant past. They examine the evidence preserved in oxygen and carbon isotopes, which provides information about the past deep-sea temperatures, global ice volumes and the carbon cycle. These clues are stored in the shells of microorganisms that once lived on the sea floor. They represent an archive of past climate conditions that researchers use to draw comparisons between the past, present and future.

The framework of a global climate reference curve has existed since 2001, although the data coverage older than 34 million years was generally poor. Since that pioneering work, however, the climate records obtained from many new sediment cores have improved, both quantitatively and qualitatively. Particularly over the past two decades, scientific drilling programs have targeted their drilling into older geological strata. Researchers therefore now have access to higher quality, more complete sediment archives, and are able to reconstruct global climate in much more detail than ever before.

The new climate reference curve, called CENOGRID (CENOzoic Global Reference benthic foraminifer carbon and oxygen Isotope Dataset), is a reconstruction of the Earth's climate since the last great extinction 66 million years ago, which introduced a new Era, the Cenozoic. "It is a tremendous joint effort by many colleagues internationally to recover the sample material, analyze it and compile it into an integrated curve," explains Westerhold.

The age model is the key component of the new reference curve. Recurring patterns in the sediment cores, called Milankovi cycles, reflect changes in the Earth's orbit around the sun. Like a metronome, these fluctuations have dictated the cyclic patterns of climate change. By identifying these astronomical cycles, the climate of the past 66 million years has now been timed continuously for the first time, allowing it to be dated much more accurately than ever before. "We have radically improved the data and age models for the time older than 34 million years in particular," says Westerhold. This is important because paleoclimate research is always concerned with finding parallels in the past to our current climate. "We want to understand what climate conditions existed in the past, what processes lay behind them, and how they proceeded. The time from 66 to 34 million years ago, when the planet was significantly warmer than it is today, is especially interesting."

Innovations in drilling strategy and technology in the early 90's helped over the past few decades to recover the high quality sediment archives required to produce a detailed global climate dataset. With new statistics, the CENOGRID makes it possible to apply advanced procedures for analyzing complex data. In the study, these are now making a significant contribution toward determining and better understanding the climate conditions and dynamics of the past. "We can thus show that there were four predominant climatic modes in the Cenozoic - hothouse, warmhouse, coolhouse and icehouse," explains Marwan. "In broad terms, this classification has been known for some time, but it was only through data analysis that we were able to identify the fundamental states with statistical precision and reveal their characteristic dynamics."

The key to this is the advanced statistical method of recurrence analysis. "Recurrence analysis reveals the dynamics of the complex climate system, including changes and hidden patterns," according to Norbert Marwan. "This, therefore, goes far beyond the direct data analyses from the drill cores." This kind of analysis also makes it possible to draw inferences about the probability of events, provided there is a large amount of data and long data series. The long time span of 66 million years is advantageous for various reasons, "because only then can we investigate whether climatic events or patterns recur and are therefore determined by natural processes. Or whether they are anomalous and therefore a cause for concern."

In the future, the new climate reference curve CENOGRID can serve as a basis for researchers worldwide to accurately correlate their data within the context of climate history. With more data, it is now possible to not only further refine the picture of the climatic past, but also to identify regional intricacies. The authors emphasize that this is fundamental for testing the reliability of climate models for the future.

VLA observations reveal giant magnetic ropes in a galaxy's halo

This image of the "Whale Galaxy" (NGC 4631), made with the National Science Foundation's Karl G. Jansky Very Large Array (VLA), reveals hair-like filaments of the galaxy's magnetic field protruding above and below the galaxy's disk.

The spiral galaxy is seen edge-on, with its disk of stars shown in pink. The filaments, shown in green and blue, extend beyond the disk into the galaxy's extended halo. Green indicates filaments with their magnetic field pointing roughly toward us and blue with the field pointing away. This phenomenon, with the field alternating in direction, has never before been seen in the halo of a galaxy. CAPTION This combined radio/optical image of the {module INSIDE STORY}

"This is the first time that we have clearly detected what astronomers call large-scale, coherent, magnetic fields far in the halo of a spiral galaxy, with the field lines aligned in the same direction over distances of a thousand light-years. We even see a regular pattern of this organized field changing direction," said Marita Krause, of the Max-Planck Institute for Radioastronomy in Bonn, Germany.

An international team of astronomers who are part of a project called the Continuum HAlos in Nearby Galaxies -- an EVLA Survey (CHANG-ES), led by Judith Irwin of Queen's University in Ontario, said the image indicates a large-scale, coherent magnetic field that is generated by dynamo action within the galaxy and spirals far outward in the form of giant magnetic ropes perpendicular to the disk.

"We are a little bit like the blind men and the elephant, since each time we look at the galaxy in a different way we reach a different conclusion about its nature! However, we seem to have one of those rare occasions where a classical theory, about magnetic generators called dynamos, predicted the observations of NGC 4631 quite well. Our dynamo model produces spiraling magnetic fields in the halo that are a continuation of the normal spiral arms in the galaxy's disc," said Richard Henriksen, of Queen's University.

The scientists are continuing their work to further refine their understanding of the galaxy's full magnetic structure.

The image was made by combining data from multiple observations with the VLA's giant dish antennas arranged in different configurations to show both large structures and finer details within the galaxy. The naturally-emitted radio waves from the galaxy were analyzed to reveal the magnetic fields, including their directions.

The scientists said the techniques used to determine the direction of the magnetic field lines, illustrated by this image, now can be used on this and other galaxies to answer important questions about whether coherent magnetic fields are common in galactic halos and what their shapes are.

Building such a picture, they said, can answer important questions such as how galaxies acquire magnetic fields, and whether all such fields are produced by a dynamo effect. Can these galaxy halo fields illuminate the mysterious origin of the even larger intergalactic magnetic fields that have been observed?

NGC 4631, 25 million light-years from Earth in the constellation Canes Venatici, is about 80,000 light-years across, slightly smaller than our own Milky Way. It was discovered by the famous British astronomer Sir William Herschel in 1787. This image also shows a companion, NGC 4627, a small elliptical galaxy, just above NGC 4631.

Oxford, Warwick researchers' twist to an old approach produces new ultrafast quantum simulations

  • New method of studying large numbers of particles at quantum level developed by Universities of Warwick and Oxford
  • Electrons and ions behave on vastly different timescales, making it prohibitive to simulate both on the same footing
  • Ultrafast quantum simulation overcomes this limitation and allows for the study of the dynamics of the interactions between electron and ion
  • The new approach offers insights into the behaviour of matter inside giant planets and in the highly compressed core during laser-driven nuclear fusion

Billions of tiny interactions occur between thousands of particles in every piece of matter in the blink of an eye. Simulating these interactions in their full dynamics was said to be elusive but has now been made possible by the new work of researchers from Oxford and Warwick.

In doing so, they have paved the way for new insights into the complex mutual interactions between the particles in extreme environments such as at the heart of large planets or laser nuclear fusion.

Researchers at the University of Warwick and the University of Oxford have developed a new way to simulate quantum systems of many particles, that allows for the investigation of the dynamic properties of quantum systems fully coupled to slowly moving ions.

Effectively, they have made the simulation of the quantum electrons so fast that it could run extremely long without restrictions and the effect of their motion on the movement of the slow ions would be visible.

Reported in the journal Science Advances, it is based on a long-known alternative formulation of quantum mechanics (Bohm dynamics) which the scientists have now empowered to allow the study of the dynamics of large quantum systems.

Many quantum phenomena have been studied for single or just a few interacting particles as large complex quantum systems overpower scientists’ theoretical and computational capabilities to make predictions. This is complicated by the vast difference in timescale the different particle species act on ions evolve thousands of times more slowly than electrons due to their larger mass. To overcome this problem, most methods involve decoupling electrons and ions and ignoring the dynamics of their interactions - but this severely limits our knowledge of quantum dynamics.

To develop a method that allows scientists to account for the full electron-ion interactions, the researchers revived an old alternative formulation of quantum mechanics developed by David Bohm. In quantum mechanics, one needs to know the wave function of a particle. It turns out that describing it by the mean trajectory and a phase, as done by Bohm, is very advantageous. However, it took an additional suit of approximations and many tests to speed up the calculations as dramatic as required. Indeed, the new methods demonstrated an increase of speed by more than a factor of 10,000 (four orders of magnitude) yet are still consistent with previous calculations for static properties of quantum systems.

The new approach was then applied to a simulation of warm dense matter, a state between solids and hot plasmas, that is known for its inherent coupling of all particle types and the need for a quantum description. In such systems, both the electrons and the ions can have excitations in the form of waves and both waves will influence each other. Here, the new approach can show its strength and determined the influence of the quantum electrons on the waves of the classical ions while the static properties were proven to agree with previous data.

Many-body quantum systems are the core of many scientific problems ranging from the complex biochemistry in our bodies to the behavior of matter inside of large planets or even technological challenges like high-temperature superconductivity or fusion energy which demonstrates the possible range of applications of the new approach.

Prof Gianluca Gregori (Oxford), who led the investigation, said: “Bohm quantum mechanics has often been treated with skepticism and controversy. In its original formulation, however, this is just a different reformulation of quantum mechanics. The advantage in employing this formalism is that different approximations become simpler to implement and this can increase the speed and accuracy of simulations involving many-body systems.”

Dr. Dirk Gericke from the University of Warwick, who assisted the design of the new supercomputer code, said: “With this huge increase of numerical efficiency, it is now possible to follow the full dynamics of fully interacting electron-ion systems. This new approach thus opens new classes of problems for efficient solutions, in particular, where either the system is evolving or where the quantum dynamics of the electrons has a significant effect on the heavier ions or the entire system.

“This new numerical tool will be a great asset when designing and interpreting experiments on warm dense matter. From its results, and especially when combined with designated experiments, we can learn much about the matter in large planets and for laser fusion research. However, I believe its true strength lies in its universality and possible applications in quantum chemistry or strongly driven solids.”