Abstract
In this chapter, we shall discuss some aspects of solar phenomena that can be described as “what to observe in upper atmosphere.” As in the previous chapter, examples of the observational results will follow the content of the book. And, again, when possible, quantitative analysis based on theoretical aspects presented in the book will be discussed.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
C.E. Alissandrakis et al., Astron. Astrophys. 603, 95A (2017)
S.A. Anfinogentov et al., Astron. Astrophys. 583, A136 (2015)
M.J. Aschwanden Self-Organized Criticality in Astrophysics. The Statistics of Nonlinear Processes in the Universe (Springer, Heidelberg, 2011)
X.Y. Bai et al., Astrophys. J. 823, 60 (2016)
M. Berger, Phys. Rev. Lett. 70, 705 (1993)
M. Berger, M. Asgari-TarghiPant, A. DeLuca, Astrophys. J. 705, 347 (2015)
J.W. Cirtain et al., Nature 493, 501 (2013)
G.A. Doschek et al., Astrophys. J. 813, 32 (2015)
A. Drews, L. Rouppe van der Voort, Astron. Astrophys. 602, 80D (2017)
M. Druckmüller et al., Astrophys. J. 785, 14 (2014)
S. Habbal et al., Astrophys. J. 793, 119 (2014)
J. Jing et al., NatSR 624319J (2016)
M.S. Kirk et al., Solar Phys. 292, 72 (2017)
B. Lehnart, Phys. Scr. 9, 229 (1974)
X. Li et al., Astrophys. J. 752, 22 (2012)
M. Liggett, H. Zirin, Solar Phys. 91, 259 (1984)
R. Liu et al., NatSR 6, 34021 (2016)
R.E. Louis et al., Astrophys. J. 727, 49 (2011)
V.M. Nakariakov et al., Astron. Astrophys. 797, 36 (2016)
Y. Ohman, Solar Phys. 9, 427 (1969)
J. Okamoto et al., Astrophys. J. 831, 126 (2016)
V. Pant et al., Astrophys. J. 801, L2 (2015)
E. Parker, Astrophys. J. 174, 499 (1972)
E. Pettit, Publ. Yerkes Obs. 111, 205 (1925)
V. Polito et al., Astron. Astrophys. 601, 39 (2017)
B. Ravindra et al., Astrophys. J. 743, 33 (2011)
K. Reardon et al., Astrophys. J. 779, 143 (2013)
T. Rimmele, J. Marino, Astrophys. J. 646, 593 (2006)
P. Romano et al., Astron. Astrophys. 582, A55 (2015)
D. Ryutov, M. Ryutova, Geophys. Monogr. 58, 167 (1990)
M.P. Ryutova, R. Shine, Astrophys. J. 606, 571 (2004)
M. Ryutova, T. Berger, Z. Frank, A. Title, Astrophys. J. 686, 1404 (2008)
M. Ryutova, T. Berger, A. Title, Astrophys. J. 676, 1356 (2008)
M. Ryutova et al., SoPh 267, 75 (2010)
G. Scharmer et al., Nature 420, 151 (2002)
E. Scullion et al., Astrophys. J. 797, 36 (2014)
R. Shine et al., 1999 Fall AGU Meeting, SH41A-06 (1999)
J. Su et al., Astrophys. J. 710, 170 (2010)
P. Sütterlin et al., Astron. Astrophys. 424, 1049 (2004)
H. Tian, G. Li, K.K. Reeves et al., Astrophys. J. Lett. 797, L14 (2014)
H. Wang et al., Astrophys. J. 559, 1171 (2001)
W. Wang, R. Liu, Y. Wang, Astrophys. J. 834, 38 (2017)
T. Wang et al., Astrophys. J. 751, L27 (2012)
H. Watanabe et al., Astrophys. J. 796, 77 (2010)
S. Wedemeyer et al., Astrophys. J. 774, 123 (2013)
Author information
Authors and Affiliations
Rights and permissions
Copyright information
© 2018 Springer Nature Switzerland AG
About this chapter
Cite this chapter
Ryutova, M. (2018). What to Observe in the Upper Atmosphere. In: Physics of Magnetic Flux Tubes. Astrophysics and Space Science Library, vol 455. Springer, Cham. https://doi.org/10.1007/978-3-319-96361-7_23
Download citation
DOI: https://doi.org/10.1007/978-3-319-96361-7_23
Published:
Publisher Name: Springer, Cham
Print ISBN: 978-3-319-96360-0
Online ISBN: 978-3-319-96361-7
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)