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  • Fire and ice: the Antarctic volcanoes that hint at our climate future

    Professor John Smellie, Honorary Professor in the School of Geology, Geography and the Environment, talks about his career and his love of the volcanoes of the Antarctic as he receives his second Polar Medal.

  • Cell Proliferation and Differentiation

    Find out more about Cell Proliferation and Differentiation research at the University of Leicester.

  • jbridges: Page 10

    This blog is a record of my experiences and work during the Mars Science Laboratory mission, from the preparation, landing on August 5th 2012 Pacific Time, and onwards...I will also post updates about our other Mars work on meteorites, ExoMars and new missions.

  • March 3rd 2013 Sol 206

    Posted by jbridges in Mars Science Laboratory Blog on March 5, 2013 No new data or images over the last few sols.

  • Phil Duke

    The academic profile of Dr Phil Duke, Associate Professor at University of Leicester

  • The University of Leicester to take part in ERA 2 Initiative

    The University of Leicester School of Chemistry and the Materials Centre are to take part in the new Energy Research Accelerator (ERA) initiative, ERA-2.

  • Energy Research Accelerator appoints new CEO

    The Energy Research Accelerator (ERA) has today announced the appointment of Gordon Waddington as its Chief Executive Officer.

  • PSE: UK Poverty and social exclusion

    Posted by Andrew Dunn in Social Sciences and Humanities Librarians’ Blog on October 17, 2012 http://www.poverty.ac.uk/ has just been re-launched, with a host of new features to improve access to the project data and findings.

  • 18th March 2016 Sol 1285

    Posted by jbridges in Mars Science Laboratory Blog on March 18, 2016 One of the ChemCam capabilities is to use its  Remote MicroImager (RMI) to take images of our laser LIBS targets, but also of more distant features.

  • Thursday 6th September Sol 30

    Posted by jbridges in Mars Science Laboratory Blog on September 6, 2012 Telescopes on Earth need to measure ‘flat’ and ‘dark’ frames with every set of observations in order to correct for distortions on the telescope mirror and any false detections on the light detector.

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