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13313 results for: ‘HIS（医院信息管理系统）系统源码✅项目合作 二开均可 TG：saolei44✅.cpCKQqtlQX’

• 25th March 2015 Sol 936

  https://staffblogs.le.ac.uk/mars/2015/03/25/25th-march-2015-sol-936/

  Posted by jbridges in Mars Science Laboratory Blog on March 25, 2015 This MAHLI image (field of view about 20 cm) shows how water has travelled through the Garden City mudstone rock.  It has left trails in veins – probably of gypsum or a similar mineral.

• Cancer Cell and Molecular Biology

  https://le.ac.uk/modules/2024/nt4004

  Module code: NT4004 This module will give you an insight into the impact of cancer in today’s society and an in-depth understanding of the molecular basis of human cancer.

• TEDxLeicester to take satellite technology one step beyond

  https://le.ac.uk/news/2017/september/tedxleicester-to-take-satellite-technology-2018one-step-beyond2019

  Some of the innovative and cutting-edge applications that satellite technology and its data are being put to will be explored in a TEDxLeicester event in partnership with the University of Leicester and the National Space Centre.

• Monday 14th January 2013 Sol 157

  https://staffblogs.le.ac.uk/mars/2013/01/15/monday-14th-january-2013-sol-157/

  Posted by jbridges in Mars Science Laboratory Blog on January 15, 2013 AS we are thinking about a drill target, the rock around us has a clastic texture, that is it is made of rounded grains that have been transported by water or wind.

• March 14th 2013 Sol 215

  https://staffblogs.le.ac.uk/mars/2013/03/14/march-14th-2013-sol-215/

  Posted by jbridges in Mars Science Laboratory Blog on March 14, 2013 The results from our drill hole are showing that the John Kein rocks include mudstone, with about 20% of it composed of a clay called smectite.

• 17th February 2014 Sol 545

  https://staffblogs.le.ac.uk/mars/2014/02/17/17th-february-2014-sol-545/

  Posted by jbridges in Mars Science Laboratory Blog on February 17, 2014 As we approach a full martian year (669 sols) we have travelled about 5 km.  There is fine tuning to be done on the route to get us relatively quickly to the clay and iron oxide concentrations in Mt.

• 14th July 2014 Sol 688

  https://staffblogs.le.ac.uk/mars/2014/07/14/14th-july-2014-sol-688/

  Posted by jbridges in Mars Science Laboratory Blog on July 14, 2014 In addition to driving towards the Murray Buttes gap in the dunes, and our path onto Mt. Sharp, we stop sometimes to do contact science.  The image gives an example of what this entails.

• Tuesday 25th September Sol 49

  https://staffblogs.le.ac.uk/mars/2012/09/25/tuesday-25th-september-sol-49/

  Posted by jbridges in Mars Science Laboratory Blog on September 25, 2012 We are now getting a combination of the high resolution MAHLI images, APXS and ChemCam compositional data and the other camera images.

• 14th October 2013 Sol 424

  https://staffblogs.le.ac.uk/mars/2013/10/14/october-14th-2013-sol-424/

  Posted by jbridges in Mars Science Laboratory Blog on October 14, 2013 The noon to pre-dawn temperature variation at Gale Crater can be up to 90 degrees centigrade.   This MastCam image shows the effects of this extreme temperature variation.

• 20th May 2013 Sol 280

  https://staffblogs.le.ac.uk/mars/2013/05/20/20th-may-2013-sol-280/

  Posted by jbridges in Mars Science Laboratory Blog on May 20, 2013 Here is a MAHLI image of our second drill hole at Cumberland.  Like the first drill hole it shows the difference between the reddish uppermost surface of Mars and what lies underneath.