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 N. Dadashi

Journal Article (2)

1.
Journal Article
Dadashi, N.; Teriaca, L.; Tripathi, D.; Solanki, S. K.; Wiegelmann, T.: Doppler shift of hot coronal lines in a moss area of an active region. Astronomy and Astrophysics 548, A115 (2012)
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DOI
2.
Journal Article
Dadashi, N.; Teriaca, L.; Solanki, S. K.: The quiet Sun average Doppler shift of coronal lines up to 2 MK. Astronomy and Astrophysics 534, A90 (2011)
MPG.PuRe
DOI

Thesis - PhD (1)

3.
Thesis - PhD
Dadashigharehbalagh, N.: Diagnostic of the solar transition region and corona from VUV spectroscopy and imaging. Dissertation, Technische Universität Braunschweig (2013)
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