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 K. A. Otto

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Journal Article (1)

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Journal Article
Lethuillier, A.; Feller, C.; Kaufmann, E.; Becerra, P.; Hänni, N.; Diethelm, R.; Kreuzig, C.; Gundlach, B.; Blum, J.; Pommerol, A. et al.; Kargl, G.; Laddha, S.; Denisova, K.; Kührt, E.; Capelo, H. L.; Haack, D.; Zhang, X.; Knollenberg, J.; Molinski, N. S.; Gilke, T.; Sierks, H.; Tiefenbacher, P.; Güttler, C.; Otto, K. A.; Bischoff, D.; Schweighart, M.; Hagermann, A.; Jäggi, N.: Cometary dust analogues for physics experiments. Monthly Notices of the Royal Astronomical Society 515, pp. 3420 - 3438 (2022)
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