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Fine Scale Structure in Cometary Dust Tails - Figure 6.9 - CME shell model sh...
Views of C/2002 V1 NEAT from SOHO LASCO C3, taken with the clear filter and enhanced as temporal difference images. The field of view of the instrument has been projected into... -
Fine Scale Structure in Cometary Dust Tails - Figure 6.7 - Temporal maps of C...
A sequences of 70 temporal maps of C/2002 V1's main dust tail created from the SOHO LASCO C3 clear filter data, enhanced as temporal difference images.The tail is shown from... -
Fine Scale Structure in Cometary Dust Tails - Figure 6.12 - Sunward aligned m...
Three sunward aligned maps of C/2002 V1's simulated dust tail position as seen by LASCO C3, showing the effects of increased solar wind dynamic pressure of varying strength.Dust... -
Fine Scale Structure in Cometary Dust Tails - Figure 6.14 - Localised high de...
View of C/2002 V1 NEAT from SOHO LASCO C3, taken with the clear filter and enhanced as temporal difference images.The field of view of the instrument has been projected into the... -
Fine Scale Structure in Cometary Dust Tails - Figure 6.15a - Temporal maps of...
Three temporal maps showing how the localised density enhancement model compares to observations of the bright stria in C/2002 V1's dust tail as seen by LASCO C3 clear with MGN... -
Fine Scale Structure in Cometary Dust Tails - Figure 6.15b - Temporal maps of...
Three temporal maps of the bright stria in C/2002 V1's dust tail as seen by LASCO C3.The tail is shown from 2003 February 18th at 07:54 UT until February 19th 04:54 UT. Dust is... -
FTIR Data Mars Sublimation Experiments
When the 2028 ESA/NASA Rosalind Franklin Rover mission arrives at Mars it will drill up to 2m into its surface and retrieve geological samples for analysis. It is crucial to...
