Five times the solar disk in a long row from left to right with main colors orange, light green, blue, green-red sprinkles, blue-to-red gradient, respresenting exemplary PMI data products after on-board analysis from left to right: continuum intensity, magnetic field strength, magnetic field inclination, magnetic field azimuth and line-of-sight velocity.

Publications of Jack Carlyle

Journal Article (2)

1.
Journal Article
Carlyle, J.; Williams, D. R.; van Driel-Gesztelyi, L.; Innes, D.; Hillier, A.; Matthews, S.: Investigating the Dynamics and Density Evolution of Returning Plasma Blobs from the 2011 June 7 Eruption. Astrophysical Journal 782 (2), 87 (2014)
MPG.PuRe
DOI
2.
Journal Article
van Driel-Gesztelyi, L.; Baker, D.; Toeroek, T.; Pariat, E.; Green, L. M.; Williams, D. R.; Carlyle, J.; Valori, G.; Demoulin, P.; Kliem, B. et al.; Long, D. M.; Matthews, S. A.; Malherbe, J.-M.: Coronal Magnetic Reconnection Driven by CME Expansion-The 2011 June 7 Event. Astrophysical Journal 788 (1), 85 (2014)
MPG.PuRe
DOI

Thesis - PhD (1)

3.
Thesis - PhD
Carlyle, J.: Mass and Magnetic Field of Eruptive Solar Filaments. Dissertation, University College London, London (2016)
MPG.PuRe
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