This section includes scientific and technological news from the IAC and its Observatories, as well as press releases on scientific and technological results, astronomical events, educational projects, outreach activities and institutional events.

  • 88th Meeting of the ICC

    The representatives of the international committee of the institutions which are members of the Observatories, run by the Instituto de Astrofísica de Canarias (IAC) in La Palma and Tenerife met on the 15th and 16th November in La Laguna. In this biennial meeting which was held on the premises of the Office of International Relations of the University of La Laguna, reports were presented on the state of the new and future telescopes in the Canary Observatories, such as the Cherenkov Telescope Array (CTA), ASTRI and the Thirty Meter Telescope (TMT). In addition there was discussion about

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  • Equipo de IACTEC-Tecnología Médica

    Today, November 14th, World Diabetes Day, the programme of IACTEC-Medical Technology of the Instituto de Astrofísica de Canarias (IAC) dedicated to the transfer of astrophysical technology to the biomedical field, celebrates the progress obtained in the development of an anthropomorphic model of a foot, which permits the simulation of pathologies of a diabetic foot. Within the MUTANT( Multimodal Tissue phANToms) line of resarch, oriented towards the development of components which simulate biological tissues, an anthropomorphic model of a foot is being developed, whose outer sheath is

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  • OGS green láser

    The workshop “25 years of cooperation in optical technologies and future trends”, will take place next Monday, November 14th, at the Headquarters of the Instituto de Astrofísica de Canarias (IAC) with scientific and engineering staff from the IAC, and from ESTEC, the European Space Technology and Research Centre of the European Space Agency (ESA). At the meeting, the two institutions will present their work on optomechanical engineering and set out the basis for further collaboration. They will discuss, among other subjects, thermal techniques and optical instrumentation developments, cryo

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  • The Subcommission of Scientific and Technical Affairs of COPUOS visits the IAC

    This week the Ambassadors, permanent representatives at the International Organizations with headquarters in Vienna, of Spain, Esther Monterrubio, and of Paraguay, Juan Francisco Facetti, were shown the installations of the IAC. During their stay they visited some of the scientific infrastructures of the Canary Islands Observatories (OCAN) and showed interest in the projects being developed there. Among the various duties of these two permanent Ambassadors is that of representing their countries in the United Nations Commission on the Peaceful Uses of Outer Space (COPUOS) and its two

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  • Eduardo L. Martín

    The European Research Council (ERC) has awarded an ERC Advanced Grant, funding for the development of research projects at the frontiers of knowledge, to the Professor of the Higher Council for Scientific Research (CSIC) Eduardo L. Martín Guerrero de Escalante, who is an active researcher at the Instituto de Astrofísica de Canarias (IAC). The project, entitled “Substellar Science with the Euclid Space Mission“ (SUBSTELLAR) has, as one of its main objectives, the use of data from the future space telescope Euclid to increase our knowledge of objects with substellar masses (brown dwarfs and

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  • Results of the recent 2D model of CBPs. Left: temperature. Right: Image showing how the simulation would look like if observed with the Solar Orbiter mission in the extreme ultraviolet from space. The CBP is distinguished by the hot magnetic loops that appear bright in the right panel.

    When the Sun is observed in X-ray or extreme ultraviolet wavelengths, hundreds of bright and compact structures with a rounded shape and sizes similar to that of our planet Earth can be easily distinguished in the solar corona. These structures are known as Coronal Bright Points or CBPs and they consist of sets of magnetic loops that connect areas of opposite magnetic polarity on the solar surface. These loops confine the solar plasma and in them, by mechanisms that have been debated for many years among solar physicists, the gas remains with temperatures of several million degrees, emitting

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