Flows in active region loops observed by Hinode EIS
By G. D. Zanna. 2008
146 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Computational Mechanics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/63c3372d97abc15c5175331cb8dd3c2923c9f637
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In Astronomy and Astrophysics
Citations in the corpus
- Slow Solar Wind: Observations and Modeling (2016, unknown): “Del Zanna (2008) showed that persistent blueshifts, stronger in the hotter lines (typically 5–20 km s−1 in Fe XII and 10–30 km s−1 in Fe XV), were present in areas of weak emission, in a sharp boundary between the low-lying ‘hot’ 3 MK loops and the higher ‘cooler’ 1 MK loops.”
- Flows and Nonthermal Velocities in Solar Active Regions Observed with the EUV Imaging Spectrometer on Hinode: A Tracer of Active Region Sources of Heliospheric Magnetic Fields? (2008, result): “Opt., 45, 8674 Landi, E., Del Zanna, G., Young, P. R., Dere, K. P., Mason, H. E., & Landini, M. 2006, ApJS, 162, 261 Liewer, P. C., Neugebauer, M., & Zurbuchen, T. 2004, Sol.”