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 Jialong Wang

Journal Article (1)

1.
Journal Article
Wang, T.; Yan, Y.; Wang, J.; Kurokawa, H.; Shibata, K.: The large-scale coronal field structure and source region features for a halo coronal mass ejection. Astrophysical Journal 572, pp. 580 - 597 (2002)

Book Chapter (1)

2.
Book Chapter
Solanki, S. K.; Bogdan, T.; Christensen-Dalsgaard, J.; Heinzel, P.; Rutten, R. J.; Kosovichev, A.; Mariska, J.; Venkatakrishnan, P.; Wang, J.: Commission 12: Solar Radiation and Structure. In: Reports on Astronomy, pp. 90 - 105 (Ed. Rickman, H.). Kluwer, Dordrecht (2003)

Conference Paper (1)

3.
Conference Paper
Zhang, J.; Solanki, S. K.; Wang, J.: Statistical properties of Moving-Magnetic-Feature pairs. In: 1st Potsdam Thinkshop on Sunspots and Starspots Poster Proceedings, pp. 127 - 129 (Eds. Strassmeier, K. G.; Washuettl, A.). Brandenburgische Universitätsdruckerei, Golm (2002)

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