Scientists have finally found direct evidence of small-scale torsional Alfvén waves in the Sun’s corona, solving an 80-year-old solar mystery. These elusive magnetic waves could be the energy source that powers the Sun’s multi-million-degree outer atmosphere.
The Harvard-Smithsonian Center for Astrophysics found that growing interest in moon resources could create international tension, as extraction becomes possible.
Prof Dr Daniela A. Wilson from the Institute for Molecules and Materials (IMM) tells us what we need to know about molecular intelligence – the rise of supramolecular nanomachines with controlled shape and motility.
Katri Huitu and Kati Lassila-Perini from Helsinki Institute of Physics, Finland, chart open science in the making including a short overview of related accelerator research expertise in Finland.
Professor Sandra Carvalho, University of Minho, Department of Physics, discusses the emergence of surface functionalization as a strategy in biotech and health.
Dr David Carroll from CU Aerospace LLC says that there are advantages to nano-satellites and the Space 2.0 environment, but they exacerbate the problem of orbital debris.
Drs Alfred Msezane and Kelvin Suggs discuss the possibilities of efficient tunable water oxidation to peroxide catalyzed by doubly charged atomic negative ions.
