A Study of Polar Jet Parameters Based on Hinode XRT Observations

By A. Savcheva, J. Cirtain, E. DeLuca, L. Lundquist, L. Golub, M. Weber, M. Shimojo, K. Shibasaki, T. Sakao, N. Narukage and 2 more. 2007

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The Magnetic Landscape of the Sun's Polar Region (2008, background): “The X-ray telescope and extreme-UV imaging spectrometer aboard Hinode have observed remarkable activity in the polar regions in the form of microflares and jets (Savcheva et al. 2007; Cirtain et al. 2007).”
Characteristics of EUV Coronal Jets Observed with STEREO/SECCHI (2009, background): “…with the results of numerical simulations (e.g. Yokoyama and Shibata, 1996, Moreno-Insertis, Galsgard, and Ugarte-Urra, 2008, Pariat, SOLA: paper1ff.tex; 24 June 2009; 6:43; p. 6 Antiochos, and DeVore, 2009) and other data analysis (e.g. Savcheva et al., 2007, Filippov, Golub and Koutchmy, 2009).”
THREE-DIMENSIONAL MODELING OF QUASI-HOMOLOGOUS SOLAR JETS (2010, background): “The fact that X-ray jets occur much more frequently than previously believed (Cirtain et al. 2007; Savcheva et al. 2007) is partly due to this property.”
A MODEL FOR SOLAR POLAR JETS (2009, background): “…several classic geometrical features observed in jets, including the “inverse Y” or ”Eiffel tower” shape, the drift of the jet axis, the 3D helical structures (Patsourakos et al. 2008), and the recent observation of Alfvén waves within polar-hole jets (Cirtain et al. 2007; Savcheva et al. 2007).”