694 research outputs found
Broadband interactive services provided through TV-centric technologies via bidirectional satellite connection
Stationary shapes of deformable particles moving at low Reynolds numbers
Lecture Notes of the Summer School ``Microswimmers -- From Single Particle
Motion to Collective Behaviour'', organised by the DFG Priority Programme SPP
1726 (Forschungszentrum J{\"{u}}lich, 2015).Comment: Pages C7.1-16 of G. Gompper et al. (ed.), Microswimmers - From Single
Particle Motion to Collective Behaviour, Lecture Notes of the DFG SPP 1726
Summer School 2015, Forschungszentrum J\"ulich GmbH, Schriften des
Forschungszentrums J\"ulich, Reihe Key Technologies, Vol 110, ISBN
978-3-95806-083-
From regional climate modelling to hydrological impact analysis: current capabilities and future research needs
Die Kritik der Politischen Ökonomie der Medien/Kommunikation: ein hochaktueller Ansatz
This debate article discusses how topical the approach of the Critique of the Political Economy of Media/Communication is today. The paper analyses the status of this field. At the international level, there is a longer tradition in the Critical Political Economy of Media/Communication, especially in the United Kingdom and North America. Since the start of the new crisis of capitalism in 2008, the interest in Marx’s works has generally increased. At the same time communicative and ideological features of societal changes’ unpredictable turbulences have become evident. This contribution introduces some specific approaches. It also discusses 14 aspects of why the complex, multidimensional, open and dynamic research approach of the critique of capitalism and society that goes back Marx’s theory remains relevant today
On Observability and Monitoring of Distributed Systems: An Industry Interview Study
Business success of companies heavily depends on the availability and
performance of their client applications. Due to modern development paradigms
such as DevOps and microservice architectural styles, applications are
decoupled into services with complex interactions and dependencies. Although
these paradigms enable individual development cycles with reduced delivery
times, they cause several challenges to manage the services in distributed
systems. One major challenge is to observe and monitor such distributed
systems. This paper provides a qualitative study to understand the challenges
and good practices in the field of observability and monitoring of distributed
systems. In 28 semi-structured interviews with software professionals we
discovered increasing complexity and dynamics in that field. Especially
observability becomes an essential prerequisite to ensure stable services and
further development of client applications. However, the participants mentioned
a discrepancy in the awareness regarding the importance of the topic, both from
the management as well as from the developer perspective. Besides technical
challenges, we identified a strong need for an organizational concept including
strategy, roles and responsibilities. Our results support practitioners in
developing and implementing systematic observability and monitoring for
distributed systems
Planck Intermediate Results. IX. Detection of the Galactic haze with Planck
Using precise full-sky observations from Planck, and applying several methods
of component separation, we identify and characterize the emission from the
Galactic "haze" at microwave wavelengths. The haze is a distinct component of
diffuse Galactic emission, roughly centered on the Galactic centre, and extends
to |b| ~35 deg in Galactic latitude and |l| ~15 deg in longitude. By combining
the Planck data with observations from the WMAP we are able to determine the
spectrum of this emission to high accuracy, unhindered by the large systematic
biases present in previous analyses. The derived spectrum is consistent with
power-law emission with a spectral index of -2.55 +/- 0.05, thus excluding
free-free emission as the source and instead favouring hard-spectrum
synchrotron radiation from an electron population with a spectrum (number
density per energy) dN/dE ~ E^-2.1. At Galactic latitudes |b|<30 deg, the
microwave haze morphology is consistent with that of the Fermi gamma-ray "haze"
or "bubbles," indicating that we have a multi-wavelength view of a distinct
component of our Galaxy. Given both the very hard spectrum and the extended
nature of the emission, it is highly unlikely that the haze electrons result
from supernova shocks in the Galactic disk. Instead, a new mechanism for
cosmic-ray acceleration in the centre of our Galaxy is implied.Comment: 15 pages, 9 figures, submitted to Astronomy and Astrophysic
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