TY  - GEN
A1  - Shprits, Yuri Y.
A1  - Zhelavskaya, Irina
A1  - Green, Janet C.
A1  - Pulkkinen, Antti A.
A1  - Horne, Richard B.
A1  - Pitchford, David
A1  - Glover, Alexi
T1  - Discussions on Stakeholder Requirements for Space Weather-Related Models
T2  - Space Weather: The International Journal of Research and Applications
N2  - Participants of the 2017 European Space Weather Week in Ostend, Belgium, discussed the stakeholder requirements for space weather-related models. It was emphasized that stakeholders show an increased interest in space weather-related models. Participants of the meeting discussed particular prediction indicators that can provide first-order estimates of the impact of space weather on engineering systems.
KW  - 7924
KW  - 7934
KW  - 7959
Y1  - 2018
U6  - https://doi.org/10.1002/2018SW001864
SN  - 1542-7390
VL  - 16
IS  - 4
SP  - 341
EP  - 342
PB  - American Geophysical Union
CY  - Washington
ER  - 
TY  - GEN
A1  - Schrape, Oliver
A1  - Balashov, Alexey
A1  - Simevski, Aleksandar
A1  - Benito, Carlos
A1  - Krstić, Miloš
T1  - Master-Clone placement with individual clock tree implementation
BT  - a Case on Physical Chip Design
T2  - 2018 IEEE Nordic Circuits and Systems Conference (NORCAS): NORCHIP and International Symposium of System-on-Chip (SoC)
N2  - A hybrid design approach of the hierarchical physical implementation design flow is presented and demonstrated on a fault-tolerant low-power multiprocessor system. The proposed flow allows to implement selected submodules in parallel with contrary requirements such as identical placement and individual block implementation. The overall system contains four Leon2 cores and communicates via the Waterbear framework and supports Adaptive Voltage Scaling (AVS) functionality. Three of the processor core variants are derived from the first baseline reference core but implemented individually at block level based on their clock tree specification. The chip is prepared for space applications and designed with triple modular redundancy (TMR) for control parts. The low-power performance is enabled by contemporary power and clock management control. An ASIC is fabricated in a low-power 0.13 mu m BiCMOS technology process node.
KW  - Hierarchical Design
KW  - Physical Implementation
KW  - Clock Tree Implementation
Y1  - 2018
SN  - 978-1-5386-7656-1
PB  - IEEE
CY  - New York
ER  - 
TY  - GEN
A1  - Wolff, Christian Michael
A1  - Canil, Laura
A1  - Rehermann, Carolin
A1  - Nguyen, Ngoc Linh
A1  - Zu, Fengshuo
A1  - Ralaiarisoa, Maryline
A1  - Caprioglio, Pietro
A1  - Fiedler, Lukas
A1  - Stolterfoht, Martin
A1  - Kogikoski, Junior, Sergio
A1  - Bald, Ilko
A1  - Koch, Norbert
A1  - Unger, Eva L.
A1  - Dittrich, Thomas
A1  - Abate, Antonio
A1  - Neher, Dieter
T1  - Correction to 'Perfluorinated self-assembled monolayers enhance the stability and efficiency of inverted perovskite solar cells' (2020, 14 (2), 1445−1456)
T2  - ACS nano
Y1  - 2020
U6  - https://doi.org/10.1021/acsnano.0c08081
SN  - 1936-0851
SN  - 1936-086X
VL  - 14
IS  - 11
SP  - 16156
EP  - 16156
PB  - American Chemical Society
CY  - Washington, DC
ER  - 
TY  - GEN
A1  - Saliba, Michael
A1  - Stolterfoht, Martin
A1  - Wolff, Christian Michael
A1  - Neher, Dieter
A1  - Abate, Antonio
T1  - Measuring aging stability of perovskite solar cells
T2  - Joule
Y1  - 2018
U6  - https://doi.org/10.1016/j.joule.2018.05.005
SN  - 2542-4351
VL  - 2
IS  - 6
SP  - 1019
EP  - 1024
PB  - Cell Press
CY  - Cambridge
ER  - 
TY  - GEN
A1  - Stete, Felix
A1  - Koopman, Wouter-Willem Adriaan
A1  - Bargheer, Matias
T1  - Signatures of strong coupling on nanoparticles
BT  - revealing absorption anticrossing by tuning the dielectric environment
T2  - Quantum Nano-Photonics
N2  - The electromagnetic coupling of molecular excitations to plasmonic nanoparticles offers a promising method to manipulate the light-matter interaction at the nanoscale. Plasmonic nanoparticles foster exceptionally high coupling strengths, due to their capacity to strongly concentrate the light-field to sub-wavelength mode volumes. A particularly interesting coupling regime occurs, if the coupling increases to a level such that the coupling strength surpasses all damping rates in the system. In this so-called strong-coupling regime hybrid light-matter states emerge, which can no more be divided into separate light and matter components. These hybrids unite the features of the original components and possess new resonances whose positions are separated by the Rabi splitting energy h Omega. Detuning the resonance of one of the components leads to an anticrossing of the two arising branches of the new resonances omega(+) and omega(-) with a minimal separation of Omega = omega(+) - omega(-).
Y1  - 2018
SN  - 978-94-024-1546-9
SN  - 978-94-024-1544-5
SN  - 978-94-024-1543-8
U6  - https://doi.org/10.1007/978-94-024-1544-5_53
SN  - 1871-465X
SP  - 445
EP  - 447
PB  - Springer
CY  - Dordrecht
ER  - 
TY  - GEN
A1  - Stete, Felix
A1  - Schossau, Phillip Gerald
A1  - Koopman, Wouter-Willem Adriaan
A1  - Bargheer, Matias
T1  - Size Dependence of the Coupling Strength in Plasmon-Exciton Nanoparticles
T2  - Quantum Nano-Photonics
N2  - The coupling between molecular excitations and nanoparticles leads to promising applications. It is for example used to enhance the optical cross-section of molecules in surface enhanced Raman scattering, Purcell enhancement or plasmon enhanced dye lasers. In a coupled system new resonances emerge resulting from the original plasmon (ωpl) and exciton (ωex) resonances as
ω±=12(ωpl+ωex)±14(ωpl−ωex)2+g2−−−−−−−−−−−−−−−√,
(1)
where g is the coupling parameter. Hence, the new resonances show a separation of Δ = ω+ − ω− from which the coupling strength can be deduced from the minimum distance between the two resonances, Ω = Δ(ω+ = ω−).
Y1  - 2018
SN  - 978-94-024-1546-9
SN  - 978-94-024-1544-5
SN  - 978-94-024-1543-8
U6  - https://doi.org/10.1007/978-94-024-1544-5_26
SN  - 1871-465X
SP  - 381
EP  - 383
PB  - Springer
CY  - Dordrecht
ER  - 
TY  - GEN
A1  - Maier, Philipp
A1  - Wolf, Jürgen
A1  - Keilig, Thomas
A1  - Krabbe, Alfred
A1  - Duffard, Rene
A1  - Ortiz, Jose-Luis
A1  - Klinkner, Sabine
A1  - Lengowski, Michael
A1  - Müller, Thomas
A1  - Lockowandt, Christian
A1  - Krockstedt, Christian
A1  - Kappelmann, Norbert
A1  - Stelzer, Beate
A1  - Werner, Klaus
A1  - Geier, Stephan
A1  - Kalkuhl, Christoph
A1  - Rauch, Thomas
A1  - Schanz, Thomas
A1  - Barnstedt, Jürgen
A1  - Conti, Lauro
A1  - Hanke, Lars
T1  - Towards a European Stratospheric Balloon Observatory
BT  - the ESBO design study
T2  - Ground-based and Airborne Telescopes VII
N2  - This paper presents the concept of a community-accessible stratospheric balloon-based observatory that is currently under preparation by a consortium of European research institutes and industry. We present the technical motivation, science case, instrumentation, and a two-stage image stabilization approach of the 0.5-m UV/visible platform. In addition, we briefly describe the novel mid-sized stabilized balloon gondola under design to carry telescopes in the 0.5 to 0.6 m range as well as the currently considered flight option for this platform. Secondly, we outline the scientific and technical motivation for a large balloon-based FIR telescope and the ESBO DS approach towards such an infrastructure.
KW  - astronomy
KW  - balloon telescopes
KW  - UV
KW  - far infrared
KW  - detectors
KW  - observatory
Y1  - 2018
SN  - 978-1-5106-1954-8
U6  - https://doi.org/10.1117/12.2319248
SN  - 0277-786X
SN  - 1996-756X
VL  - 10700
PB  - SPIE-INT Soc Optical Engineering
CY  - Bellingham
ER  - 
TY  - GEN
A1  - Finch, Nicolle L.
A1  - Braker, I. P.
A1  - Reindl, Nicole
A1  - Barstow, Martin A.
A1  - Casewell, Sarah L.
A1  - Burleigh, M.
A1  - Kupfer, Thomas
A1  - Kilkenny, D.
A1  - Geier, Stephan
A1  - Schaffenroth, Veronika
A1  - Bertolami Miller, Marcelo Miguel
A1  - Taubenberger, Stefan
A1  - Freudenthal, Joseph
T1  - Spectral Analysis of Binary Pre-white Dwarf Systems
T2  - Radiative signatures from the cosmos
N2  - Short period double degenerate white dwarf (WD) binaries with periods of less than similar to 1 day are considered to be one of the likely progenitors of type Ia supernovae. These binaries have undergone a period of common envelope evolution. If the core ignites helium before the envelope is ejected, then a hot subdwarf remains prior to contracting into a WD. Here we present a comparison of two very rare systems that contain two hot subdwarfs in short period orbits. We provide a quantitative spectroscopic analysis of the systems using synthetic spectra from state-of-the-art non-LTE models to constrain the atmospheric parameters of the stars. We also use these models to determine the radial velocities, and thus calculate dynamical masses for the stars in each system.
Y1  - 2019
SN  - 978-1-58381-925-8
SN  - 1050-3390
VL  - 519
SP  - 231
EP  - 238
PB  - Astronomical soc pacific
CY  - San Fransisco
ER  -