TY - JOUR A1 - Pena-Angulo, D. A1 - Nadal-Romero, E. A1 - Gonzalez-Hidalgo, J. C. A1 - Albaladejo, J. A1 - Andreu, V A1 - Bagarello, V A1 - Barhi, H. A1 - Batalla, R. J. A1 - Bernal, S. A1 - Bienes, R. A1 - Campo, J. A1 - Campo-Bescos, M. A. A1 - Canatario-Duarte, A. A1 - Canton, Y. A1 - Casali, J. A1 - Castillo, V A1 - Cerda, Artemi A1 - Cheggour, A. A1 - Cid, Patricio A1 - Cortesi, N. A1 - Desir, G. A1 - Diaz-Pereira, E. A1 - Espigares, T. A1 - Estrany, Joan A1 - Fernandez-Raga, M. A1 - Ferreira, Carla S. S. A1 - Ferro, Vito A1 - Gallart, Francesc A1 - Gimenez, R. A1 - Gimeno, E. A1 - Gomez, J. A. A1 - Gomez-Gutierrez, A. A1 - Gomez-Macpherson, H. A1 - Gonzalez-Pelayo, O. A1 - Hueso-Gonzalez, P. A1 - Kairis, O. A1 - Karatzas, G. P. A1 - Klotz, S. A1 - Kosmas, C. A1 - Lana-Renault, Noemi A1 - Lasanta, T. A1 - Latron, J. A1 - Lazaro, R. A1 - Le Bissonnais, Y. A1 - Le Bouteiller, C. A1 - Licciardello, F. A1 - Lopez-Tarazon, José Andrés A1 - Lucia, A. A1 - Marin, C. A1 - Marques, M. J. A1 - Martinez-Fernandez, J. A1 - Martinez-Mena, M. A1 - Martinez-Murillo, J. F. A1 - Mateos, L. A1 - Mathys, N. A1 - Merino-Martin, L. A1 - Moreno-de las Heras, M. A1 - Moustakas, N. A1 - Nicolau, J. M. A1 - Novara, A. A1 - Pampalone, V A1 - Raclot, D. A1 - Rodriguez-Blanco, M. L. A1 - Rodrigo-Comino, Jesús A1 - Romero-Diaz, A. A1 - Roose, E. A1 - Rubio, J. L. A1 - Ruiz-Sinoga, J. D. A1 - Schnabel, S. A1 - Senciales-Gonzalez, J. M. A1 - Simonneaux, V A1 - Sole-Benet, A. A1 - Taguas, E. A1 - Taboada-Castro, M. M. A1 - Taboada-Castro, M. T. A1 - Todisco, Francesca A1 - Ubeda, X. A1 - Varouchakis, E. A. A1 - Vericat, Damia A1 - Wittenberg, L. A1 - Zabaleta, A. A1 - Zorn, M. T1 - Spatial variability of the relationships of runoff and sediment yield with weather types throughout the Mediterranean basin JF - Journal of hydrology N2 - Soil degradation by water is a serious environmental problem worldwide, with specific climatic factors being the major causes. We investigated the relationships between synoptic atmospheric patterns (i.e. weather types, WTs) and runoff, erosion and sediment yield throughout the Mediterranean basin by analyzing a large database of natural rainfall events at 68 research sites in 9 countries. Principal Component Analysis (PCA) was used to identify spatial relationships of the different WTs including three hydro-sedimentary variables: rainfall, runoff, and sediment yield (SY, used to refer to both soil erosion measured at plot scale and sediment yield registered at catchment scale). The results indicated 4 spatial classes of rainfall and runoff: (a) northern sites dependent on North (N) and North West (NW) flows; (b) eastern sites dependent on E and NE flows; (c) southern sites dependent on S and SE flows; and, finally, (d) western sites dependent on W and SW flows. Conversely, three spatial classes are identified for SY characterized by: (a) N and NE flows in northern sites (b) E flows in eastern sites, and (c) W and SW flows in western sites. Most of the rainfall, runoff and SY occurred during a small number of daily events, and just a few WTs accounted for large percentages of the total. Our results confirm that characterization by WT improves understanding of the general conditions under which runoff and SY occur, and provides useful information for understanding the spatial variability of runoff, and SY throughout the Mediterranean basin. The approach used here could be useful to aid of the design of regional water management and soil conservation measures. KW - Synoptic weather types KW - Erosion KW - Sediment yield KW - Runoff KW - Mediterranean basin Y1 - 2019 U6 - https://doi.org/10.1016/j.jhydrol.2019.01.059 SN - 0022-1694 SN - 1879-2707 VL - 571 SP - 390 EP - 405 PB - Elsevier CY - Amsterdam ER - TY - JOUR A1 - Soliveres, Santiago A1 - Maestre, Fernando T. A1 - Ulrich, Werner A1 - Manning, Peter A1 - Boch, Steffen A1 - Bowker, Matthew A. A1 - Prati, Daniel A1 - Delgado-Baquerizo, Manuel A1 - Quero, Jose L. A1 - Schöning, Ingo A1 - Gallardo, Antonio A1 - Weisser, Wolfgang W. A1 - Müller, Jörg A1 - Socher, Stephanie A. A1 - Garcia-Gomez, Miguel A1 - Ochoa, Victoria A1 - Schulze, Ernst-Detlef A1 - Fischer, Markus A1 - Allan, Eric T1 - Intransitive competition is widespread in plant communities and maintains their species richness JF - Ecology letters N2 - Intransitive competition networks, those in which there is no single best competitor, may ensure species coexistence. However, their frequency and importance in maintaining diversity in real-world ecosystems remain unclear. We used two large data sets from drylands and agricultural grasslands to assess: (1) the generality of intransitive competition, (2) intransitivity-richness relationships and (3) effects of two major drivers of biodiversity loss (aridity and land-use intensification) on intransitivity and species richness. Intransitive competition occurred in >65% of sites and was associated with higher species richness. Intransitivity increased with aridity, partly buffering its negative effects on diversity, but was decreased by intensive land use, enhancing its negative effects on diversity. These contrasting responses likely arise because intransitivity is promoted by temporal heterogeneity, which is enhanced by aridity but may decline with land-use intensity. We show that intransitivity is widespread in nature and increases diversity, but it can be lost with environmental homogenisation. KW - Aridity KW - biodiversity KW - coexistence KW - drylands KW - land use KW - mesic grasslands KW - rock-paper-scissors game Y1 - 2015 U6 - https://doi.org/10.1111/ele.12456 SN - 1461-023X SN - 1461-0248 VL - 18 IS - 8 SP - 790 EP - 798 PB - Wiley-Blackwell CY - Hoboken ER - TY - JOUR A1 - Nishikawa, Ken-Ichi A1 - Mizuno, Yosuke A1 - Niemiec, Jacek A1 - Kobzar, Oleh A1 - Pohl, Martin A1 - Gomez, Jose L. A1 - Dutan, Ioana A1 - Frederiksen, Jacob Trier A1 - Nordlund, Ake A1 - Meli, Athina A1 - Sol, Helene A1 - Hardee, Philip E. A1 - Hartmann, Dieter H. T1 - Microscopic Processes in Global Relativistic Jets Containing Helical Magnetic Fields JF - Galaxies : open access journal N2 - In the study of relativistic jets one of the key open questions is their interaction with the environment on the microscopic level. Here, we study the initial evolution of both electron-proton (e(-)-p(+)) and electron-positron (e(+/-)) relativistic jets containing helical magnetic fields, focusing on their interaction with an ambient plasma. We have performed simulations of "global" jets containing helical magnetic fields in order to examine how helical magnetic fields affect kinetic instabilities such as the Weibel instability, the kinetic Kelvin-Helmholtz instability (kKHI) and the Mushroom instability (MI). In our initial simulation study these kinetic instabilities are suppressed and new types of instabilities can grow. In the e(-)-p(+) jet simulation a recollimation-like instability occurs and jet electrons are strongly perturbed. In the e(+/-) jet simulation a recollimation-like instability occurs at early times followed by a kinetic instability and the general structure is similar to a simulation without helical magnetic field. Simulations using much larger systems are required in order to thoroughly follow the evolution of global jets containing helical magnetic fields. KW - relativistic jets KW - particle-in-cell simulations KW - global jets KW - helical magnetic fields KW - kinetic instabilities KW - kink instability Y1 - 2016 U6 - https://doi.org/10.3390/galaxies4040038 SN - 2075-4434 VL - 4 PB - MDPI CY - Basel ER - TY - JOUR A1 - Nishikawa, Ken-Ichi A1 - Mizuno, Yosuke A1 - Gomez, Jose L. A1 - Dutan, Ioana A1 - Meli, Athina A1 - White, Charley A1 - Niemiec, Jacek A1 - Kobzar, Oleh A1 - Pohl, Martin A1 - Frederiksen, Jacob Trier A1 - Nordlund, Ake A1 - Sol, Helene A1 - Hardee, Philip E. A1 - Hartmann, Dieter H. T1 - Microscopic Processes in Global Relativistic Jets Containing Helical Magnetic Fields: Dependence on Jet Radius JF - Galaxies : open access journal N2 - In this study, we investigate the interaction of jets with their environment at a microscopic level, which is a key open question in the study of relativistic jets. Using small simulation systems during past research, we initially studied the evolution of both electron-proton and electron-positron relativistic jets containing helical magnetic fields, by focusing on their interactions with an ambient plasma. Here, using larger jet radii, we have performed simulations of global jets containing helical magnetic fields in order to examine how helical magnetic fields affect kinetic instabilities, such as the Weibel instability, the kinetic Kelvin-Helmholtz instability (kKHI) and the mushroom instability (MI). We found that the evolution of global jets strongly depends on the size of the jet radius. For example, phase bunching of jet electrons, in particular in the electron-proton jet, is mixed with a larger jet radius as a result of the more complicated structures of magnetic fields with excited kinetic instabilities. In our simulation, these kinetic instabilities led to new types of instabilities in global jets. In the electron-proton jet simulation, a modified recollimation occurred, and jet electrons were strongly perturbed. In the electron-positron jet simulation, mixed kinetic instabilities occurred early, followed by a turbulence-like structure. Simulations using much larger (and longer) systems are required in order to further thoroughly investigate the evolution of global jets containing helical magnetic fields. KW - relativistic jets KW - particle-in-cell simulations KW - global jets KW - helical magnetic fields KW - kinetic instabilities KW - kink-like instability KW - recollimation shocks KW - polarized radiation Y1 - 2017 U6 - https://doi.org/10.3390/galaxies5040058 SN - 2075-4434 VL - 5 PB - MDPI CY - Basel ER - TY - GEN A1 - Nishikawa, Ken-Ichi A1 - Mizuno, Yosuke A1 - Niemiec, Jacek A1 - Kobzar, Oleh A1 - Pohl, Martin A1 - Gómez, Jose L. A1 - Duţan, Ioana A1 - Pe’er, Asaf A1 - Frederiksen, Jacob Trier A1 - Nordlund, Åke A1 - Meli, Athina A1 - Sol, Helene A1 - Hardee, Philip E. A1 - Hartmann, Dieter H. T1 - Microscopic processes in global relativistic jets containing helical magnetic fields T2 - Galaxies N2 - In the study of relativistic jets one of the key open questions is their interaction with the environment on the microscopic level. Here, we study the initial evolution of both electron-proton (e(-)-p(+)) and electron-positron (e(+/-)) relativistic jets containing helical magnetic fields, focusing on their interaction with an ambient plasma. We have performed simulations of "global" jets containing helical magnetic fields in order to examine how helical magnetic fields affect kinetic instabilities such as the Weibel instability, the kinetic Kelvin-Helmholtz instability (kKHI) and the Mushroom instability (MI). In our initial simulation study these kinetic instabilities are suppressed and new types of instabilities can grow. In the e(-)-p(+) jet simulation a recollimation-like instability occurs and jet electrons are strongly perturbed. In the e(+/-) jet simulation a recollimation-like instability occurs at early times followed by a kinetic instability and the general structure is similar to a simulation without helical magnetic field. Simulations using much larger systems are required in order to thoroughly follow the evolution of global jets containing helical magnetic fields. T3 - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 446 KW - relativistic jets KW - particle-in-cell simulations KW - global jets KW - helical magnetic fields KW - kinetic instabilities KW - kink instability Y1 - 2018 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-407604 ER - TY - JOUR A1 - Nishikawa, Ken-Ichi A1 - Mizuno, Yosuke A1 - Gomez, Jose L. A1 - Duţan, Ioana A1 - Meli, Athina A1 - Niemiec, Jacek A1 - Kobzar, Oleh A1 - Pohl, Martin A1 - Sol, Hélène A1 - MacDonald, Nicholas A1 - Hartmann, Dieter H. T1 - Relativistic jet simulations of the weibel instability in the slab model to cylindrical jets with helical magnetic fields JF - Galaxies : open access journal N2 - The particle-in-cell (PIC) method was developed to investigate microscopic phenomena, and with the advances in computing power, newly developed codes have been used for several fields, such as astrophysical, magnetospheric, and solar plasmas. PIC applications have grown extensively, with large computing powers available on supercomputers such as Pleiades and Blue Waters in the US. For astrophysical plasma research, PIC methods have been utilized for several topics, such as reconnection, pulsar dynamics, non-relativistic shocks, relativistic shocks, and relativistic jets. PIC simulations of relativistic jets have been reviewed with emphasis placed on the physics involved in the simulations. This review summarizes PIC simulations, starting with the Weibel instability in slab models of jets, and then focuses on global jet evolution in helical magnetic field geometry. In particular, we address kinetic Kelvin-Helmholtz instabilities and mushroom instabilities. KW - particle-in-cell simulations KW - relativistic jets KW - the Weibel instability KW - kink-like instability KW - mushroom instability KW - global jets KW - helical magnetic fields KW - recollimation shocks Y1 - 2019 U6 - https://doi.org/10.3390/galaxies7010029 SN - 2075-4434 VL - 7 IS - 1 PB - MDPI CY - Basel ER -