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1st September 2014 Sol 736
https://staffblogs.le.ac.uk/mars/2014/09/01/1st-september-2014-sol-736/
Posted by jbridges in Mars Science Laboratory Blog on September 1, 2014 We are in an uneven area of terrain with sand-filled hollows so we have changed direction, out of Hidden Valley and via Trilobite Crater. The rover planners ‘RP’s’ are cautious about slippage in sand.
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19th August 2014 Sol 724
https://staffblogs.le.ac.uk/mars/2014/08/19/19th-august-sol-724/
Posted by jbridges in Mars Science Laboratory Blog on August 19, 2014 We have started the condensed drilling procedures at Bonanza_King, having driven back out of Hidden Valley and its sandy deposits, to take another route.
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Phil Duke
https://le.ac.uk/people/phil-duke
The academic profile of Dr Phil Duke, Associate Professor at University of Leicester
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Diana Dukhia
https://le.ac.uk/people/diana-dukhia
The academic profile of Dr Diana Dukhia, Lecturer at University of Leicester
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Doug Battersby
https://le.ac.uk/people/doug-battersby
The academic profile of Dr Doug Battersby, Lecturer in Modern Literature at University of Leicester
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21st May 2015 Sol 992
https://staffblogs.le.ac.uk/mars/2015/05/21/21st-may-2015-sol-992/
Posted by jbridges in Mars Science Laboratory Blog on May 21, 2015 In a first for the mission we have successfully climbed a slope at Mt. Stimson.
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Doug Gregg
https://le.ac.uk/people/doug-gregg
The academic profile of Doug Gregg, PhD Researcher at University of Leicester
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Daqi Liu
https://le.ac.uk/people/daqi-liu
The academic profile of Dr Daqi Liu, Lecturer at University of Leicester
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18th June 2013 Sol 308
https://staffblogs.le.ac.uk/mars/2013/06/18/18th-june-2013-sol-308/
Posted by jbridges in Mars Science Laboratory Blog on June 18, 2013 I am taking my turn at being the GeoMin group theme lead this sol. I am also the ChemCam science theme group member.
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Thursday 6th September Sol 30
https://staffblogs.le.ac.uk/mars/2012/09/06/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.