Modelling the Sun's small scale global photospheric magnetic field

We present a new model for the Sun's global photospheric magnetic field during a deep minimum of activity, in which no active regions emerge. The emergence and subsequent evolution of small- scale magnetic features across the full solar surface is simulated, subject to the influence of a global supergranular flow pattern. Visually, the resulting simulated magnetograms reproduce the typical structure and scale observed in quiet Sun magnetograms. Quantitatively, the simulation quickly reaches a steady state, resulting in a mean field and flux distribution that are in good agreement with those determined from observations. A potential coronal magnetic field is extrapolated from the simulated full Sun magnetograms, to consider the implications of such a quiet photospheric magnetic field on the corona and inner heliosphere. The bulk of the coronal magnetic field closes very low down, in short connections between small-scale features in the simulated magnetic network. Just 0.1% of the photospheric magnetic flux is found to be open at 2:5 Rʘ, around 10 - 100 times less than that determined for typical HMI synoptic map observations. If such conditions were to exist on the Sun, this would lead to a significantly weaker interplanetary magnetic field than is presently observed, and hence a much higher cosmic ray flux at Earth.

Industry-academia linkages in a high tech research field

Currently academic researches' focus started changing towards protecting IP rights and to transferring them into industrial actors. Accordingly, it is argued that academic's basic research focus started shifting towards applied research as it is essential for the radical inventions to be introduced in a competitive market. This research seeks to understand industry-academia linkages in a high tech field such as nano-crystals. In regards to supporting the technology transfer process within or cross country, this study illustrates the technology development trends and actors' engagement; nano-crystals technology and their interconnections; and maps the organisational (industry-academia) linkages that enhance the commercialisation of radical inventions. The results show that the industry-academia linkages that appeared as decentralized structure are more stable compared to other linkage types. Korean and Japanese organisations present such stable linkages. The linkages are even stronger when they appear as a mono-linkage type. Chinese organisations show a great illustration of such an effective mono-linkage of co-inventorships in high tech research field. The organisations in the US maintain international linkages.