TY  - JOUR
A1  - Jordan, Thomas
A1  - Fechler, Nina
A1  - Xu, Jingsan
A1  - Brenner, Thomas J. K.
A1  - Antonietti, Markus
A1  - Shalom, Menny
T1  - "Caffeine Doping" of Carbon/Nitrogen-Based Organic Catalysts: Caffeine as a Supramolecular Edge Modifier for the Synthesis of Photoactive Carbon Nitride Tubes
JF  - ChemCatChem : heterogeneous & homogeneous & bio- & nano-catalysis ; a journal of ChemPubSoc Europe
N2  - An alternative method for the structure tuning of carbon nitride materials by using a supramolecular approach in combination with caffeine as lining-agent is described. The self-assembly of the precursor complex consisting of melamine and cyanuric acid can be controlled by this doping molecule in terms of morphology, electronic, and photophysical properties. Caffeine is proposed to insert as an edge-molecule eventually leading to hollow tube-like carbon nitride structures with improved efficiency of charge formation. Compared to the bulk carbon nitride, the caffeine-doped analogue possesses a higher photocatalytic activity for the degradation of rhodamineB dye. Furthermore, this approach is also shown to be suitable for the modification of carbon nitride electrodes.
KW  - caffeine
KW  - carbon nitride
KW  - films
KW  - photocatalysis
KW  - supramolecular chemistry
Y1  - 2015
U6  - https://doi.org/10.1002/cctc.201500343
SN  - 1867-3880
SN  - 1867-3899
VL  - 7
IS  - 18
SP  - 2826
EP  - 2830
PB  - Wiley-VCH
CY  - Weinheim
ER  - 
TY  - JOUR
A1  - Liebig, Ferenc
A1  - Sarhan, Radwan Mohamed
A1  - Prietzel, Claudia Christina
A1  - Reinecke, Antje
A1  - Koetz, Joachim
T1  - "Green" gold nanotriangles: synthesis, purification by polyelectrolyte/micelle depletion flocculation and performance in surface-enhanced Raman scattering
JF  - RSC Advances
N2  - The aim of this study was to develop a one-step synthesis of gold nanotriangles (NTs) in the presence of mixed phospholipid vesicles followed by a separation process to isolate purified NTs. Negatively charged vesicles containing AOT and phospholipids, in the absence and presence of additional reducing agents (polyampholytes, polyanions or low molecular weight compounds), were used as a template phase to form anisotropic gold nanoparticles. Upon addition of the gold chloride solution, the nucleation process is initiated and both types of particles, i.e., isotropic spherical and anisotropic gold nanotriangles, are formed simultaneously. As it was not possible to produce monodisperse nanotriangles with such a one-step procedure, the anisotropic nanoparticles needed to be separated from the spherical ones. Therefore, a new type of separation procedure using combined polyelectrolyte/micelle depletion flocculation was successfully applied. As a result of the different purification steps, a green colored aqueous dispersion was obtained containing highly purified, well-defined negatively charged flat nanocrystals with a platelet thickness of 10 nm and an edge length of about 175 nm. The NTs produce promising results in surface-enhanced Raman scattering.
Y1  - 2016
U6  - https://doi.org/10.1039/c6ra04808k
SN  - 2046-2069
VL  - 6
SP  - 33561
EP  - 33568
PB  - Royal Society of Chemistry
CY  - Cambridge
ER  - 
TY  - JOUR
A1  - Sadovnichii, V. A.
A1  - Panasyuk, M. I.
A1  - Amelyushkin, A. M.
A1  - Bogomolov, V. V.
A1  - Benghin, V. V.
A1  - Garipov, G. K.
A1  - Kalegaev, V. V.
A1  - Klimov, P. A.
A1  - Khrenov, B. A.
A1  - Petrov, V. L.
A1  - Sharakin, S. A.
A1  - Shirokov, A. V.
A1  - Svertilov, S. I.
A1  - Zotov, M. Y.
A1  - Yashin, I. V.
A1  - Gorbovskoy, E. S.
A1  - Lipunov, V. M.
A1  - Park, I. H.
A1  - Lee, J.
A1  - Jeong, S.
A1  - Kim, M. B.
A1  - Jeong, H. M.
A1  - Shprits, Yuri Y.
A1  - Angelopoulos, V.
A1  - Russell, C. T.
A1  - Runov, A.
A1  - Turner, D.
A1  - Strangeway, R. J.
A1  - Caron, R.
A1  - Biktemerova, S.
A1  - Grinyuk, A.
A1  - Lavrova, M.
A1  - Tkachev, L.
A1  - Tkachenko, A.
A1  - Martinez, O.
A1  - Salazar, H.
A1  - Ponce, E.
T1  - "Lomonosov" Satellite-Space Observatory to Study Extreme Phenomena in Space
JF  - Space science reviews
N2  - The "Lomonosov" space project is lead by Lomonosov Moscow State University in collaboration with the following key partners: Joint Institute for Nuclear Research, Russia, University of California, Los Angeles (USA), University of Pueblo (Mexico), Sungkyunkwan University (Republic of Korea) and with Russian space industry organi-zations to study some of extreme phenomena in space related to astrophysics, astroparticle physics, space physics, and space biology. The primary goals of this experiment are to study: -Ultra-high energy cosmic rays (UHECR) in the energy range of the Greizen-ZatsepinKuzmin (GZK) cutoff; -Ultraviolet (UV) transient luminous events in the upper atmosphere; -Multi-wavelength study of gamma-ray bursts in visible, UV, gamma, and X-rays; -Energetic trapped and precipitated radiation (electrons and protons) at low-Earth orbit (LEO) in connection with global geomagnetic disturbances; -Multicomponent radiation doses along the orbit of spacecraft under different geomagnetic conditions and testing of space segments of optical observations of space-debris and other space objects; -Instrumental vestibular-sensor conflict of zero-gravity phenomena during space flight. This paper is directed towards the general description of both scientific goals of the project and scientific equipment on board the satellite. The following papers of this issue are devoted to detailed descriptions of scientific instruments.
KW  - Gamma-ray bursts
KW  - Ultra-high energy cosmic rays
KW  - Radiation belts
KW  - Space mission
Y1  - 2017
U6  - https://doi.org/10.1007/s11214-017-0425-x
SN  - 0038-6308
SN  - 1572-9672
VL  - 212
SP  - 1705
EP  - 1738
PB  - Springer
CY  - Dordrecht
ER  - 
TY  - JOUR
A1  - Chen, Zupeng
A1  - Savateev, Aleksandr
A1  - Pronkin, Sergey
A1  - Papaefthimiou, Vasiliki
A1  - Wolff, Christian Michael
A1  - Willinger, Marc Georg
A1  - Willinger, Elena
A1  - Neher, Dieter
A1  - Antonietti, Markus
A1  - Dontsova, Dariya
T1  - "The Easier the Better" Preparation of Efficient Photocatalysts-Metastable Poly(heptazine imide) Salts
JF  - Advanced materials
N2  - Cost-efficient, visible-light-driven hydrogen production from water is an attractive potential source of clean, sustainable fuel. Here, it is shown that thermal solid state reactions of traditional carbon nitride precursors (cyanamide, melamine) with NaCl, KCl, or CsCl are a cheap and straightforward way to prepare poly(heptazine imide) alkali metal salts, whose thermodynamic stability decreases upon the increase of the metal atom size. The chemical structure of the prepared salts is confirmed by the results of X-ray photoelectron and infrared spectroscopies, powder X-ray diffraction and electron microscopy studies, and, in the case of sodium poly(heptazine imide), additionally by atomic pair distribution function analysis and 2D powder X-ray diffraction pattern simulations. In contrast, reactions with LiCl yield thermodynamically stable poly(triazine imides). Owing to the metastability and high structural order, the obtained heptazine imide salts are found to be highly active photo-catalysts in Rhodamine B and 4-chlorophenol degradation, and Pt-assisted sacrificial water reduction reactions under visible light irradiation. The measured hydrogen evolution rates are up to four times higher than those provided by a benchmark photocatalyst, mesoporous graphitic carbon nitride. Moreover, the products are able to photocatalytically reduce water with considerable reaction rates, even when glycerol is used as a sacrificial hole scavenger.
KW  - carbon nitride
KW  - glycerol oxidation
KW  - mesocrystals
KW  - poly(heptazine imide)
KW  - water reduction reactions
Y1  - 2017
U6  - https://doi.org/10.1002/adma.201700555
SN  - 0935-9648
SN  - 1521-4095
VL  - 29
SP  - 21800
EP  - 21806
PB  - Wiley-VCH
CY  - Weinheim
ER  - 
TY  - JOUR
A1  - Henkel, Carsten
A1  - Gardiner, Simon A.
A1  - Negretti, Antonio
T1  - (De)coherence physics with condensates in microtraps
N2  - We discuss the dynamics of a condensate in a miniaturized electromagnetic trap formed above a microstructured substrate. Recent experiments have found that trap lifetimes get reduced when approaching the substrate because atoms couple to thermally excited near fields. The data agree quantitatively with our theory [Appl. Phys. B 69, 379 (1999)]. We focus on the decoherence of a quantum degenerate gas in a quasi-one-dimensional trap. Monte Carlo simulations indicate that atom interactions reduce the condensate decoherence rate. This is explained by a simple theory in terms of the suppression of long-wavelength excitations. We present preliminary simulation results for the adiabatic generation of dark solitons
Y1  - 2004
SN  - 1054-660X
ER  - 
TY  - JOUR
A1  - Pade, Sylvia
A1  - Schmidt, Hartmut
A1  - Stumpe, Joachim
A1  - Fischer, Thomas M.
T1  - (Micro-)fluorescence spectroscopy of side chain polymers with bezanilide moieties
Y1  - 1996
ER  - 
TY  - JOUR
A1  - Mikat, Jürgen E. R.
A1  - Franco, Olga
A1  - Regenstein, Wolfgang
A1  - Reck, Günter
A1  - Knochenhauer, Gerald
A1  - Schulz, Burkhard
A1  - Orgzall, Ingo
T1  - 1,3,4-oxadiazole crystals under high pressure-phase transitions and properties
Y1  - 2000
ER  - 
TY  - JOUR
A1  - Eichler, Hans Joachim
A1  - Haase, Alfred
A1  - Menzel, Ralf
T1  - 100 watt average output power 1.2*diffraction limited beam from pulsed neodym single rod amplifier with SBS- phaseconjugation
BT  - Onehundred watt average output 1.2*diffraction limited beam from pulsed neodym single rod amplifier with SBS- phaseconjugation
T2  - Hundred watt average output power 1.2*diffraction limited beam from pulsed neodym single rod amplfier with SBS- phaseconjugation
Y1  - 1995
ER  - 
TY  - GEN
A1  - Schulze, Patricia S. C.
A1  - Bett, Alexander J.
A1  - Bivour, Martin
A1  - Caprioglio, Pietro
A1  - Gerspacher, Fabian M.
A1  - Kabaklı, Özde Ş.
A1  - Richter, Armin
A1  - Stolterfoht, Martin
A1  - Zhang, Qinxin
A1  - Neher, Dieter
A1  - Hermle, Martin
A1  - Hillebrecht, Harald
A1  - Glunz, Stefan W.
A1  - Goldschmidt, Jan Christoph
T1  - 25.1% high-efficiency monolithic perovskite silicon tandem solar cell with a high bandgap perovskite absorber
T2  - Postprints der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe
N2  - Monolithic perovskite silicon tandem solar cells can overcome the theoretical efficiency limit of silicon solar cells. This requires an optimum bandgap, high quantum efficiency, and high stability of the perovskite. Herein, a silicon heterojunction bottom cell is combined with a perovskite top cell, with an optimum bandgap of 1.68 eV in planar p-i-n tandem configuration. A methylammonium-free FA(0.75)Cs(0.25)Pb(I0.8Br0.2)(3) perovskite with high Cs content is investigated for improved stability. A 10% molarity increase to 1.1 m of the perovskite precursor solution results in approximate to 75 nm thicker absorber layers and 0.7 mA cm(-2) higher short-circuit current density. With the optimized absorber, tandem devices reach a high fill factor of 80% and up to 25.1% certified efficiency. The unencapsulated tandem device shows an efficiency improvement of 2.3% (absolute) over 5 months, showing the robustness of the absorber against degradation. Moreover, a photoluminescence quantum yield analysis reveals that with adapted charge transport materials and surface passivation, along with improved antireflection measures, the high bandgap perovskite absorber has the potential for 30% tandem efficiency in the near future.
T3  - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 1197 
KW  - heterojunction silicon solar cells
KW  - interfaces
KW  - perovskite solar cells
KW  - tandem solar cells
KW  - thin films
Y1  - 2020
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-525668
SN  - 1866-8372
IS  - 7
ER  - 
TY  - JOUR
A1  - Schulze, Patricia S. C.
A1  - Bett, Alexander J.
A1  - Bivour, Martin
A1  - Caprioglio, Pietro
A1  - Gerspacher, Fabian M.
A1  - Kabaklı, Özde Ş.
A1  - Richter, Armin
A1  - Stolterfoht, Martin
A1  - Zhang, Qinxin
A1  - Neher, Dieter
A1  - Hermle, Martin
A1  - Hillebrecht, Harald
A1  - Glunz, Stefan W.
A1  - Goldschmidt, Jan Christoph
T1  - 25.1% high-efficiency monolithic perovskite silicon tandem solar cell with a high bandgap perovskite absorber
JF  - Solar RRL
N2  - Monolithic perovskite silicon tandem solar cells can overcome the theoretical efficiency limit of silicon solar cells. This requires an optimum bandgap, high quantum efficiency, and high stability of the perovskite. Herein, a silicon heterojunction bottom cell is combined with a perovskite top cell, with an optimum bandgap of 1.68 eV in planar p-i-n tandem configuration. A methylammonium-free FA(0.75)Cs(0.25)Pb(I0.8Br0.2)(3) perovskite with high Cs content is investigated for improved stability. A 10% molarity increase to 1.1 m of the perovskite precursor solution results in approximate to 75 nm thicker absorber layers and 0.7 mA cm(-2) higher short-circuit current density. With the optimized absorber, tandem devices reach a high fill factor of 80% and up to 25.1% certified efficiency. The unencapsulated tandem device shows an efficiency improvement of 2.3% (absolute) over 5 months, showing the robustness of the absorber against degradation. Moreover, a photoluminescence quantum yield analysis reveals that with adapted charge transport materials and surface passivation, along with improved antireflection measures, the high bandgap perovskite absorber has the potential for 30% tandem efficiency in the near future.
KW  - heterojunction silicon solar cells
KW  - interfaces
KW  - perovskite solar cells
KW  - tandem solar cells
KW  - thin films
Y1  - 2020
VL  - 4
IS  - 7
PB  - John Wiley & Sons, Inc.
CY  - New Jersey
ER  - 
TY  - JOUR
A1  - Ostermeyer, Martin
A1  - Heuer, Axel
A1  - Menzel, Ralf
T1  - 27 Watt average output power with 1.2*DL beam quality from a single rod Nd:YAG-Laser with phase conjugating SBS- mirror
BT  - Siebenundzwanzig Watt average output power with 1.2*DL beam quality from a single rod Nd:YAG-Laser with phase conjugating SBS-mirror
Y1  - 1998
ER  - 
TY  - JOUR
A1  - Evans, Chris J.
A1  - van Loon, Jacco Th.
A1  - Hainich, Rainer
A1  - Bailey, M.
T1  - 2dF-AAOmega spectroscopy of massive stars in the Magellanic Clouds The north-eastern region of the Large Magellanic Cloud
JF  - Astronomy and astrophysics : an international weekly journal
N2  - We present spectral classifications from optical spectroscopy of 263 massive stars in the north-eastern region of the Large Magellanic Cloud. The observed two-degree field includes the massive 30 Doradus star-forming region, the environs of SN1987A, and a number of star-forming complexes to the south of 30 Dor. These are the first classifications for the majority (203) of the stars and include eleven double-lined spectroscopic binaries. The sample also includes the first examples of early OC-type spectra (AA Omega 30 Dor 248 and 280), distinguished by the weakness of their nitrogen spectra and by C IV lambda 4658 emission. We propose that these stars have relatively unprocessed CNO abundances compared to morphologically normal O-type stars, indicative of an earlier evolutionary phase. From analysis of observations obtained on two consecutive nights, we present radial-velocity estimates for 233 stars, finding one apparent single-lined binary and nine (>3 sigma) outliers compared to the systemic velocity; the latter objects could be runaway stars or large-amplitude binary systems and further spectroscopy is required to investigate their nature.
KW  - Magellanic Clouds
KW  - stars: early-type
KW  - stars: fundamental parameters
KW  - open clusters and associations: general
Y1  - 2015
U6  - https://doi.org/10.1051/0004-6361/201525882
SN  - 1432-0746
VL  - 584
PB  - EDP Sciences
CY  - Les Ulis
ER  - 
TY  - JOUR
A1  - Ostermeyer, Martin
A1  - Menzel, Ralf
T1  - 34 Watt flash lamp pumped single rod ND:YAG laser with 1.2 * DL beam quality via special resonator design
BT  - Vierunddreißig Watt flash lamp pumped single rod ND:YAG laser with 1.2 * DL beam quality via special resonator design
Y1  - 1997
ER  - 
TY  - THES
A1  - Ehrig, Sebastian
T1  - 3D curvature and its role on tissue organization
N2  - Shape change is a fundamental process occurring in biological tissues during embryonic development and regeneration of tissues and organs. This process is regulated by cells that are constrained within a complex environment of biochemical and physical cues. The spatial constraint due to geometry has a determining role on tissue mechanics and the spatial distribution of force patterns that, in turn, influences the organization of the tissue structure. An understanding of the underlying principles of tissue organization may have wide consequences for the understanding of healing processes and the development of organs and, as such, is of fundamental interest for the tissue engineering community.
This thesis aims to further our understanding of how the collective behaviour of cells is influenced by the 3D geometry of the environment. Previous research studying the role of geometry on tissue growth has mainly focused either on flat surfaces or on substrates where at least one of the principal curvatures is zero. In the present work, tissue growth from MC3T3-E1 pre-osteoblasts was investigated on surfaces of controlled mean curvature. 
One key aspect of this thesis was the development of substrates of controlled mean curvature and their visualization in 3D. It was demonstrated that substrates of controlled mean curvature suitable for cell culture can be fabricated using liquid polymers and surface tension effects.
Using these substrates, it was shown that the mean surface curvature has a strong impact on the rate of tissue growth and on the organization of the tissue structure. It was thereby not only demonstrated that the amount of tissue produced (i.e. growth rates) by the cells depends on the mean curvature of the substrate but also that the tissue surface behaves like a viscous fluid with an equilibrium shape governed by the Laplace-Young-law. It was observed that more tissue was formed on highly concave surfaces compared to flat or convex surfaces.
Motivated by these observations, an analytical model was developed, where the rate of tissue growth is a function of the mean curvature, which could successfully describe the growth kinetics. This model was also able to reproduce the growth kinetics of previous experiments where tissues have been cultured in straight-sided prismatic pores.
A second part of this thesis focuses on the tissue structure, which influences the mechanical properties of the mature bone tissue. Since the extracellular matrix is produced by the cells, the cell orientation has a strong impact on the direction of the tissue fibres. In addition, it was recently shown that some cell types exhibit collective alignment similar to liquid crystals. 
Based on this observation, a computational model of self-propelled active particles was developed to explore in an abstract manner how the collective behaviour of cells is influenced by 3D curvature. It was demonstrated that the 3D curvature has a strong impact on the self-organization of active particles and gives, therefore, first insights into the principles of self-organization of cells on curved surfaces.
N2  - Formänderung ist ein fundamentaler Vorgang während der embryonalen Entwicklung und der Regeneration von Geweben und Organen. Dieser Prozess wird von Zellen reguliert die in einer komplexen Umgebung von biochemischen und physikalischen Signalen eingebettet sind. Die räumliche Begrenzung der Zellen führt dabei zu Unterschieden in der Gewebemechanik und der räumlichen Verteilung von Kräften und hat damit einen Einfluss auf die Organisation der Gewebestruktur. Ein Verständnis der Organisationsprozesse von Geweben hat weitreichende Konsequenzen im Hinblick auf das Verständnis von Heilungsprozessen und der Entwicklung von Organen bis hin zu medizinischen Anwendungen wie der Entwicklung von Implantaten.
Die vorliegende Arbeit zielt auf ein besseres Verständnis wie das kollektive Verhalten von Gewebezellen von der dreidimensionalen Krümmung der Umgebung beeinflusst wird. Die bisherige Forschung war bislang limitiert auf flache Oberflächen oder auf Substrate in denen zumindest eine der beiden Hauptkrümmungen Null ist. In dieser Arbeit wurde daher das Gewebewachstum von MC3T3-E1 Pre-Osteoblasten auf Oberflächen mit konstanter mittlerer Krümmung studiert.
Ein wichtiger Teil der Arbeit war die Entwicklung von Substraten mit kontrollierter mittlerer Krümmung und deren Visualisierung in 3D. Es wurde gezeigt, dass sich die Oberflächen- spannung von Polymerlösungen nutzen lässt um eben solche Substrate zu erzeugen. 
Mit Hilfe dieser Substrate wurde gezeigt, dass die mittlere Krümmung der Oberfläche einen entscheidenden Einfluss auf die Wachstumsrate und die Organisation der Gewebestruktur hat. Es konnte nicht nur gezeigt werden dass die Menge an gebildetem Gewebe von der mittleren Krümmung abhängig ist, sondern auch dass die Oberfläche des Gewebes sich dabei wie eine Flüssigkeit verhält und dem Laplace-Young Gesetz folgt. Es wurde beobachtet dass sich mehr Gewebe auf konkaven als auf flachen oder konvexen Oberflächen gebildet hat.
Basierend auf diesen Beobachtungen wurde ein analytisches Modell entwickelt, welches die Wachstumsrate als Funktion der mittleren Krümmung beschreibt und mit Hilfe dessen sich das Gewebewachstum erfolgreich beschreiben lässt. Dieses Modell kann auch die Ergebnisse früherer Arbeiten reproduzieren, in denen Gewebe in prismatischen Poren kultiviert wurden.
Ein weiterer Teil der Arbeit befasste sich mit der Struktur des Gewebes, welche einen Einfluss auf die späteren mechanischen Eigenschaften des maturierten Knochengewebes hat. Da die extrazelluläre Matrix des Gewebes von den Zellen gebildet wird, hat die Orientierung der Zellen einen entscheidenden Einfluss auf die Ausrichtung der Gewebefasern. Außerdem wurde vor kurzem gezeigt, dass sich manche Zellen wie Flüssigkristalle anordnen können. 
Basierend auf dieser Beobachtung wurde ein Computermodell aktiver Partikel entwickelt, mit dessen Hilfe sich der Einfluss des kollektiven Verhaltens der Zellen auf dreidimensional gekrümmten Oberflächen abstrahieren lässt. Es konnte dabei gezeigt werden, dass die dreidimensionale Krümmung einen entscheidenden Einfluss auf die Selbstorganisation dieser Partikel hat und gibt damit erste Einblicke in ein mögliches Organisationsverhalten von Zellen auf 3D Oberflächen.
KW  - biophysics
KW  - tissue engineering
KW  - mechanobiology
Y1  - 2017
ER  - 
TY  - JOUR
A1  - Pham, Cong Duc
A1  - Petre, Anca
A1  - Berquez, Laurent
A1  - Flores Suárez, Rosaura
A1  - Mellinger, Axel
A1  - Wirges, Werner
A1  - Gerhard, Reimund
T1  - 3D high-resolution mapping of polarization profiles in thin poly(vinylidenefluoride-trifluoroethylene) (PVDF- TrFE) films using two thermal techniques
N2  - In this paper, two non-destructive thermal methods are used in order to determine, with a high degree of accuracy, three-dimensional polarization distributions in thin films (12 mu m) of poly(vinylidenefluoride- trifluoroethylene) (PVDF-TrFE). The techniques are the frequency-domain Focused Laser Intensity Modulation Method (FLIMM) and time-domain Thermal-Pulse Tomography (TPT). Samples were first metalized with grid-shaped electrode and poled. 3D polarization mapping yielded profiles which reproduce the electrode-grid shape. The polarization is not uniform across the sample thickness. Significant polarization values are found only at depths beyond 0.5 mu m from the sample surface. Both methods provide similar results, TPT method being faster, whereas the FLIMM technique has a better lateral resolution.
Y1  - 2009
UR  - http://ieeexplore.ieee.org/servlet/opac?punumber=94
U6  - https://doi.org/10.1109/TDEI.2009.5128505
SN  - 1070-9878
ER  - 
TY  - JOUR
A1  - Madura, T. I.
A1  - Clementel, N.
A1  - Gull, T. R.
A1  - Kruip, C. J. H.
A1  - Paardekooper, J.-P.
A1  - Icke, V.
T1  - 3D hydrodynamical and radiative transfer modeling of η Carinae's colliding winds
JF  - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015
N2  - We present results of full 3D hydrodynamical and radiative transfer simulations of the colliding stellar winds in the massive binary system η Carinae. We accomplish this by applying the SimpleX algorithm for 3D radiative transfer on an unstructured Voronoi-Delaunay grid to recent 3D smoothed particle hydrodynamics (SPH) simulations of the binary colliding winds. We use SimpleX to obtain detailed ionization fractions of hydrogen and helium, in 3D, at the resolution of the original SPH simulations. We investigate several computational domain sizes and Luminous Blue Variable primary star mass-loss rates. We furthermore present new methods of visualizing and interacting with output from complex 3D numerical simulations, including 3D interactive graphics and 3D printing. While we initially focus on η Car, the methods employed can be applied to numerous other colliding wind (WR 140, WR 137, WR 19) and dusty `pinwheel' (WR 104, WR 98a) binary systems. Coupled with 3D hydrodynamical simulations, SimpleX simulations have the potential to help determine the regions where various observed time-variable emission and absorption lines form in these unique objects.
Y1  - 2015
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87930
SP  - 163
EP  - 166
ER  - 
TY  - GEN
A1  - Kubatova, Brankica
A1  - Hamann, Wolf-Rainer
A1  - Kubat, Jiri
A1  - Oskinova, Lida
T1  - 3D Monte Carlo Radiative Transfer in Inhomogeneous Massive Star Winds
BT  - Application to Resonance Line Formation
T2  - Radiative signatures from the cosmos
N2  - Already for decades it has been known that the winds of massive stars are inhomogeneous (i.e. clumped). To properly model observed spectra of massive star winds it is necessary to incorporate the 3-D nature of clumping into radiative transfer calculations. In this paper we present our full 3-D Monte Carlo radiative transfer code for inhomogeneous expanding stellar winds. We use a set of parameters to describe dense as well as the rarefied wind components. At the same time, we account for non-monotonic velocity fields. We show how the 3-D density and velocity wind inhomogeneities strongly affect the resonance line formation. We also show how wind clumping can solve the discrepancy between P v and H alpha mass-loss rate diagnostics.
Y1  - 2019
SN  - 978-1-58381-925-8
SN  - 1050-3390
VL  - 519
SP  - 209
EP  - 212
PB  - Astronomical soc pacific
CY  - San Fransisco
ER  - 
TY  - JOUR
A1  - Reyes-Iturbide, J.
A1  - Velázquez, Pablo F.
A1  - Rosado, M.
T1  - 3D numerical model for NGC 6888 Nebula
JF  - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015
N2  - We present 3D numerical simulations of the NGC6888 nebula considering the proper motion and the evolution of the star, from the red supergiant (RSG) to the Wolf-Rayet (WR) phase. Our simulations reproduce the limb-brightened morphology observed in [OIII] and X-ray emission maps. The synthetic maps computed by the numerical simulations show filamentary and clumpy structures produced by instabilities triggered in the interaction between the WR wind and the RSG shell.
Y1  - 2015
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88485
SP  - 363
ER  - 
TY  - JOUR
A1  - Thompson, W. T.
A1  - Kliem, Bernhard
A1  - Toeroek, Tibor
T1  - 3D reconstruction of a rotating erupting prominence
JF  - Solar physics : a journal for solar and solar-stellar research and the study of solar terrestrial physics
N2  - A bright prominence associated with a coronal mass ejection (CME) was seen erupting from the Sun on 9 April 2008. This prominence was tracked by both the Solar Terrestrial Relations Observatory (STEREO) EUVI and COR1 telescopes, and was seen to rotate about the line of sight as it erupted; therefore, the event has been nicknamed the "Cartwheel CME." The threads of the prominence in the core of the CME quite clearly indicate the structure of a weakly to moderately twisted flux rope throughout the field of view, up to heliocentric heights of 4 solar radii. Although the STEREO separation was 48A degrees, it was possible to match some sharp features in the later part of the eruption as seen in the 304 line in EUVI and in the H alpha-sensitive bandpass of COR1 by both STEREO Ahead and Behind. These features could then be traced out in three-dimensional space, and reprojected into a view in which the eruption is directed toward the observer. The reconstructed view shows that the alignment of the prominence to the vertical axis rotates as it rises up to a leading-edge height of a parts per thousand aEuro parts per thousand 2.5 solar radii, and then remains approximately constant. The alignment at 2.5 solar radii differs by about 115A degrees from the original filament orientation inferred from H alpha and EUV data, and the height profile of the rotation, obtained here for the first time, shows that two thirds of the total rotation are reached within a parts per thousand aEuro parts per thousand 0.5 solar radii above the photosphere. These features are well reproduced by numerical simulations of an unstable moderately twisted flux rope embedded in external flux with a relatively strong shear field component.
KW  - Corona, active
KW  - Prominences, active
KW  - Coronal mass ejections
KW  - Initiation and propagation
KW  - Magnetic fields, corona
Y1  - 2012
U6  - https://doi.org/10.1007/s11207-011-9868-5
SN  - 0038-0938
VL  - 276
IS  - 1-2
SP  - 241
EP  - 259
PB  - Springer
CY  - Dordrecht
ER  - 
TY  - JOUR
A1  - Ostermeyer, Martin
A1  - Menzel, Ralf
T1  - 50 Watt average output power with 1.2*DL beam quality from a single rod Nd:YALO laser with phase-conjugating SBS mirror
BT  - Fünfzig Watt average output power with 1.2*DL beam quality from a single rod Nd:YALO laser with phase- conjugating SBS mirror
Y1  - 1999
ER  -