Wi-Fi on rays of light: 100 times faster, and never overloaded

Researchers may have a new solution to your slow wifi. Credit: © wladimir1804 / Fotolia

Researchers may have a new solution to your slow wifi.
Credit: © wladimir1804 / Fotolia

Research team gets a speed of 42.8 Gbit/s with a ray of light in an optical wireless network. Researchers at Eindhoven University of Technology have come up with a surprising solution: a wireless network based on harmless infrared rays. The capacity is not only huge (more than 40Gbit/s per ray) but also there is no need to share since every device gets its own ray of light. This was the subject for which TU/e researcher Joanne Oh received her PhD degree with the ‘cum laude’ distinction last week.

The system is simple and, in principle, cheap to set up...

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New Hubble Mosaic of the Orion Nebula

This composite image of the Kleinmann-Low Nebula, part of the Orion Nebula complex, is composed of several pointings of the NASA/ESA Hubble Space Telescope in optical and near-infrared light. Infrared light allows to peer through the dust of the nebula and to see the stars therein. The revealed stars are shown with a bright red colour in the image. Credit: NASA, ESA/Hubble

This composite image of the Kleinmann-Low Nebula, part of the Orion Nebula complex, is composed of several pointings of the NASA/ESA Hubble Space Telescope in optical and near-infrared light. Infrared light allows to peer through the dust of the nebula and to see the stars therein. The revealed stars are shown with a bright red colour in the image.
Credit: NASA, ESA/Hubble

In the search for rogue planets and failed stars astronomers using Hubble have created a new mosaic image of the Orion Nebula. During their survey of the famous star formation region, they found what may be the missing piece of a cosmic puzzle; the third, long-lost member of a star system that had broken apart.

The Orion Nebula is the closest star formation region to Earth, only 1400 light-years away...

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The Rotation Axes of Stars tell us about how they were Born

Numerical simulation of the fragmentation of a cluster of stars up to the formation of stars (left) with a zoom on the most central part of the cluster (right). The inclination axes of the masses similar to those observed by the Kepler satellite (in cluster NGC 6791) align in this simulation when the kinetic energy of the original cloud is comparable to the ambient turbulent energy. © E.Corsaro & Y.-N Lee

Numerical simulation of the fragmentation of a cluster of stars up to the formation of stars (left) with a zoom on the most central part of the cluster (right). The inclination axes of the masses similar to those observed by the Kepler satellite (in cluster NGC 6791) align in this simulation when the kinetic energy of the original cloud is comparable to the ambient turbulent energy. © E.Corsaro & Y.-N Lee

Using asteroseismology, an international team including CEA, CNRS and Université Grenoble-Alpes discovered a surprising alignment of the rotation axes of stars in open clusters, shedding light on the conditions in which stars are formed in our galaxy...

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New Role for Immune Cells in Preventing Diabetes and Hypertension

 Eosinophils stimulate β3 adrenoreceptors through the release of soluble factors.

Eosinophils stimulate β3 adrenoreceptors through the release of soluble factors.

Immune cells which are reduced in number by obesity could be a new target to treat diseases such as type 2 diabetes and hypertension that affect overweight people, according to a collaborative study between The University of Manchester, Lund University and the University of Salford. In a study published in the journal Scientific Reports, reseachers investigated eosinophils. Eosinophils are present in perivascular adipose tissue (PVAT), which surrounds blood vessels and helps to maintain normal blood vessel function by reducing artery contraction.

The current research found that eosinophils were considerably reduced in the PVAT in obesity in mice, and that the PVAT function was severely impaired, contributing ...

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