1.2 Solar telescopes

Author(s):  
C. J. Durrant
Keyword(s):  

Solar Physics ◽  
2013 ◽  
Vol 283 (2) ◽  
pp. 651-665 ◽  
Author(s):  
Adriana Valio ◽  
P. Kaufmann ◽  
C. G. Giménez de Castro ◽  
J.-P. Raulin ◽  
L. O. T. Fernandes ◽  
...  


2016 ◽  
Author(s):  
L. V. Antoshkin ◽  
N. N. Botugina ◽  
L. A. Bolbasova ◽  
M. L. Demidov ◽  
V. M. Grigoriev ◽  
...  


2010 ◽  
Vol 49 (31) ◽  
pp. G155 ◽  
Author(s):  
Thomas Berkefeld ◽  
Dirk Soltau ◽  
Dirk Schmidt ◽  
Oskar von der Lühe




1990 ◽  
Vol 142 ◽  
pp. 113-117
Author(s):  
F. Kneer ◽  
D. Soltau ◽  
E. Wiehr

The German solar facilities at the Obsrvatorio del Teide are described first. Then, a few examples of recent results from magnetic features are given: spatial variation and velocity fluctuation of small-scale magnetic fluxtubes in the quiet Sun, Evershed flow and magnetic field in connection with penumbral fine structure, and magnetic field variation in sunspot umbrae.



1981 ◽  
Vol 93 ◽  
pp. 526 ◽  
Author(s):  
O. Engvold ◽  
R. Brahde ◽  
B. Fossum
Keyword(s):  


Author(s):  
Pavel Kovadlo ◽  
Vladimir Lukin ◽  
Dmitriy Kolobov ◽  
Victor Nosov ◽  
Maksim Eselevich ◽  
...  




Solar Physics ◽  
1996 ◽  
Vol 169 (2) ◽  
Author(s):  
JacquesM. Beckers


2012 ◽  
Vol 10 (H16) ◽  
pp. 439-470
Author(s):  
Gianna Cauzzi ◽  
Alexandra Tritschler ◽  
Yuanyong Deng

AbstractWith several large aperture optical and IR telescopes just coming on-line, or scheduled for the near future, solar physics is on the verge of a quantum leap in observational capabilities. An efficient use of such facilities will require new and innovative approaches to both observatory operations and data handling.This two-days long Special Session discussed the science expected with large solar telescopes, and started addressing the strategies necessary to optimize their scientific return. Cutting edge solar science as derived from state-of-the-art observations and numerical simulations and modeling was presented, and discussions were held on the role of large facilities in satisfying the demanding requirements of spatial and temporal resolution, stray-light correction, and spectro-polarimetric accuracy. Building on the experience of recently commissioned telescopes, critical issues for the development of future facilities were discussed. These included operational issues peculiar to large telecopes as well as strategies for their best use.



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