Atomslöjd - Nanoforskarna använder naturens egna grepp

Nanovetenskap: Forskning, undervisning och tillämpningar

Balancing Act

Can Europe achieve energy security without compromising climate goals?

Preparing a network structure for rule extraction

The medicine as a fetish. Or the meaning of magic feelings in trust relationships and self trust.

Evaluation of Some Algorithms for Hardware-Oriented Message Authentication

In this technical report, we consider ultra light-weight constructions of message authentication in hardware applications. We examine several known constructions and evaluate details around their hardware implementations. These constructions are all based on the framework of universal hash functions.

Gendered Aspects of the Process of Leaving Home in Post-War Sweden. A Micro-level Analaysis of the Swedish Family Life Survey

Kundorienterade organisationslösningar för ökad effektivitet i offentlig sektor

Tool Support for Requirements Management Quality from a User Perspective

Fabrication, optical characterization and modelling of strain core-shell nanowires

Total cost of ERP systems implementation in Danish, Slovak and Slovenian Companies

Agreeing passives in Finnish

Some results on correlations in the Bluetooth stream cipher

The Happy Update: Self-reported Happiness Linked to Semantic Representations of Status Updates in Facebook

World Conference on Healthy Buildings: Airborne nanoparticles are a health risk

The Market for Tractors in the EU: Price Differences and Convergence

Method and an apparatus in tuning a PID-regulator

Post-occupancy evaluation of complex computerized work environment. An environmental psychology case-study

Travelling by urban public transport: Exploration of usability problems in a travel chain perspective

Manganese Abundances in Cluster and Field Stars

We have derived Mn abundances for more than 200 stars in 19 globular clusters. In addition, Mn abundance determinations have been made for a comparable number of halo field and disk stars possessing an overlapping range of metallicities and stellar parameters. Our primary data set was comprised of high-resolution spectra previously acquired at the McDonald, Lick, and Keck Observatories. To enlarge