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Geomagnetic observatory data, Ebre Observatory 2022
Geomagnetic observatory vector (X, Y, Z) and scalar (F) definitive data (quasi-definitive data is available while the definitive is not ready) recorded by the Ebre Observatory... -
Geomagnetic observatory data, Ebre Observatory 2024
Geomagnetic observatory vector (X, Y, Z) and scalar (F) definitive data (quasi-definitive data are available until the definitive data are ready) recorded by the Ebre... -
Geomagnetic observatory data, Ebre Observatory 2023
Geomagnetic observatory vector (X, Y, Z) and scalar (F) definitive data (quasi-definitive data are available until the definitive data are ready) recorded by the Ebre... -
Available data for "MIMiX: A Multipurpose In-situ Microreactor system for X-r...
This dataset has no description
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Fine Scale Structure in Cometary Dust Tails - Figure 5.2a - C/2011 L4 as seen...
View of C/2011 L4 Pan-STARRS from STEREO-B HI-1. The sun is centre below relative to all images (rotated 90 degrees counter-clockwise and flipped from nominal orientation). -
Fine Scale Structure in Cometary Dust Tails - Figure 5.24 - Solar Wind adjust...
Three solar wind aligned temporal maps of C/2011 L4's main dust tail region as seen by HI-1B with coarse-scale difference enhancement. The x-axis corresponds to the paths... -
Fine Scale Structure in Cometary Dust Tails - Figure 6.5 - Radial view of C/2...
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 6.2a, 6.2b - C/2002 V1 a...
Views of C/2002 V1 NEAT from SOHO LASCO C3, using the clear filter. -
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 5.19 - Sunward aligned t...
Sunward-aligned temporal maps of C/2011 L4's main dust tail region as seen by HI-1B with coarse-scale difference enhancement.Two points of note in the tail are points P (βr =... -
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... -
Fine Scale Structure in Cometary Dust Tails - Figure 5.9, 5.10 -Temporal map ...
A sequence of 235 temporal maps, with coarse-scale difference enhancement (i.e. using temporal difference images with a narrow dynamic range). This shows the main dust tail of... -
Fine Scale Structure in Cometary Dust Tails - Figure 6.2e, 6.2f, 6.3a - C/200...
Views of C/2002 V1 NEAT from SOHO LASCO C3, using the clear filter, enhanced as temporal difference images. -
Fine Scale Structure in Cometary Dust Tails - Figure 5.15 - Stria breaking up...
A sequence of images extracted from the STEREO-B HI-1 view of C/2011 L4, using coarse scale difference images. The breakup of a stria early on the 14th march is shown, centred... -
Fine Scale Structure in Cometary Dust Tails - Figure 5.7 - Temporal map seque...
A sequence of 275 temporal maps of C/2011 L4's dust tail with MGN enhancement. This shows the main dust tail of C/2011 L4 from 2013 March 10 00:00 UT until March 18 00:00 UT.... -
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 6.6 - 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 using MGN enhancement.The tail is shown from 2003 February 16th at... -
Fine Scale Structure in Cometary Dust Tails - Figure 5.18 - Sunward aligned t...
Sunward-aligned temporal maps of McNaught's main dust tail region as seen by HI-1A with MGN enhancement.After a 6 hour data gap, on 22:01 UT on January 12th 2007, new near... -
Fine Scale Structure in Cometary Dust Tails - Figure 5.14 - Stria breaking up...
A sequence of images extracted from the STEREO-B HI-1 view of C/2011 L4, using coarse scale difference images. The breakup of a stria early on the 14th march is shown, centred...
