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  • 1
    Publication Date: 2012-01-28
    Description: The standard model for the origin of galactic magnetic fields is through the amplification of seed fields via dynamo or turbulent processes to the level consistent with present observations. Although other mechanisms may also operate, currents from misaligned pressure and temperature gradients (the Biermann battery process) inevitably accompany the formation of galaxies in the absence of a primordial field. Driven by geometrical asymmetries in shocks associated with the collapse of protogalactic structures, the Biermann battery is believed to generate tiny seed fields to a level of about 10(-21) gauss (refs 7, 8). With the advent of high-power laser systems in the past two decades, a new area of research has opened in which, using simple scaling relations, astrophysical environments can effectively be reproduced in the laboratory. Here we report the results of an experiment that produced seed magnetic fields by the Biermann battery effect. We show that these results can be scaled to the intergalactic medium, where turbulence, acting on timescales of around 700 million years, can amplify the seed fields sufficiently to affect galaxy evolution.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Gregori, G -- Ravasio, A -- Murphy, C D -- Schaar, K -- Baird, A -- Bell, A R -- Benuzzi-Mounaix, A -- Bingham, R -- Constantin, C -- Drake, R P -- Edwards, M -- Everson, E T -- Gregory, C D -- Kuramitsu, Y -- Lau, W -- Mithen, J -- Niemann, C -- Park, H-S -- Remington, B A -- Reville, B -- Robinson, A P L -- Ryutov, D D -- Sakawa, Y -- Yang, S -- Woolsey, N C -- Koenig, M -- Miniati, F -- England -- Nature. 2012 Jan 25;481(7382):480-3. doi: 10.1038/nature10747.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Physics, University of Oxford, Parks Road, Oxford OX1 3PU, UK. g.gregori1@physics.ox.ac.uk〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22281596" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 2
    Publication Date: 2022-10-06
    Description: Prominent excursions in the number of cosmogenic nuclides (e.g., 10Be) around 774 CE/775 document the most severe solar proton event (SPE) throughout the Holocene. Its manifestation in ice cores is valuable for geochronology, but also for solar‐terrestrial physics and climate modeling. Using the ECHAM/MESSy Atmospheric Chemistry (EMAC) climate model in combination with the Warning System for Aviation Exposure to SEP (WASAVIES), we investigate the transport, mixing, and deposition of the cosmogenic nuclide 10Be produced by the 774 CE/775 SPE. By comparing the model results to the reconstructed 10Be time series from four ice core records, we study the atmospheric pathways of 10Be from its stratospheric source to its sink at Earth's surface. The reconstructed post‐SPE evolution of the 10Be surface fluxes at the ice core sites is well captured by the model. The downward transport of the 10Be atoms is controlled by the Brewer‐Dobson circulation in the stratosphere and cross‐tropopause transport via tropopause folds or large‐scale sinking. Clear hemispheric differences in the transport and deposition processes are identified. In both polar regions the 10Be surface fluxes peak in summertime, with a larger influence of wet deposition on the seasonal 10Be surface flux in Greenland than in Antarctica. Differences in the peak 10Be surface flux following the 774 CE/775 SPE at the drilling sites are explained by specific meteorological conditions depending on the geographic locations of the sites.
    Description: Plain Language Summary: During large solar storms, high energy particles are hurled with enormous force toward Earth by the Sun. As these particles collide with atmospheric constituents (such as oxygen or nitrogen) unique nuclides of cosmogenic origin are formed in the higher atmosphere. From there they are transported downwards and finally precipitate at the surface due to different sink processes. Their imprints can be conserved over thousands of years within natural archives, such as ice cores or tree rings. Analysis of these natural archives around the globe indicates that the strongest solar storm over the last 10.000 years happened around 774 CE/775. This event is estimated to have been up to two orders of magnitude stronger, than the strongest known events documented for the satellite era. In this study, we model and analyze the transport and deposition of the cosmogenic nuclides produced by the extreme 774 CE/775 event, by applying a new experimental setup. Our results might help to interpret the fingerprints of historical extreme events with respect to the prevailing atmospheric conditions.
    Description: Key Points: The modeled transport and deposition of the cosmogenic nuclide10Be produced by the 774/775 solar proton event was compared to 10Be ice core records. Hemispheric differences in stratospheric and cross‐tropopause transport, and deposition were identified, with polar summertime maxima of 10Be surface flux. Differences in reconstructed10Be surface fluxes are explained by the local ratio of wet to dry deposition maximizing in the summertime.
    Description: MEXT Japan Society for the Promotion of Science http://dx.doi.org/10.13039/501100001691
    Keywords: ddc:551.5
    Language: English
    Type: doc-type:article
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  • 3
    Publication Date: 2012-01-01
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Published by Springer Nature
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  • 4
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    In:  XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
    Publication Date: 2023-09-06
    Description: We model the atmospheric transport and deposition of Beryllium-10 produced by singular solar proton events (SPE) and continuous galactic cosmic rays (GCR), to shed light on the complex interplay of solar activity, atmospheric dynamics and deposition mechanisms. Our modeling approach, which uses the chemistry-climate model EMAC (ECHAM/MESSy Atmospheric Chemistry), incorporates approximations for the production of Beryllium-10 for both SPE and GCR background concentrations, atmospheric dynamics in the middle atmosphere and troposphere as well as different deposition mechanisms such as dry deposition, wet deposition and sedimentation. We find good agreement between the simulated Beryllium-10 surface fluxes of the 774/5 AD SPE and four different proxy data sets from ice core analysis. Furthermore, we analyse the global deposition pattern of Beryllium-10 produced by GCR and investigate how multiple factors such as stratospheric dynamics, e.g. the Brewer–Dobson circulation, wind systems like jetstreams, precipitation, sea ice coverage and surface properties correlate with the deposition pattern and the different deposition mechanisms.
    Language: English
    Type: info:eu-repo/semantics/conferenceObject
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