The low-latitude inner corona of the sun observed by SUMER on SOHO

1999 ◽  
Author(s):  
Klaus Wilhelm
Keyword(s):  
The Sun ◽  
Low Latitude ◽  
Corona Of The Sun

scholarly journals Magnetic jam in the corona of the Sun

2015 ◽  
Vol 11 (6) ◽  
pp. 492-495 ◽  
Author(s):  
F. Chen ◽  
H. Peter ◽  
S. Bingert ◽  
M. C. M. Cheung
Keyword(s):  
The Sun ◽  
Corona Of The Sun

Plasma Corona and Dust Corona of the Sun

1994 ◽  
pp. 449-476
Author(s):  
Takao Saito ◽  
S.-I. Akasofu ◽  
Y. Kozuka ◽  
S. Minami ◽  
S. Tuneta
Keyword(s):  
The Sun ◽  
Plasma Corona ◽  
Corona Of The Sun

Results of observations of the dust distribution in the F-corona of the sun

2016 ◽  
Vol 50 (2) ◽  
pp. 143-160 ◽  
Author(s):  
L. I. Shestakova ◽  
B. I. Demchenko
Keyword(s):  
The Sun ◽  
Dust Distribution ◽  
Corona Of The Sun

scholarly journals Seismology of the corona of the Sun

2004 ◽  
Vol 45 (4) ◽  
pp. 4.26-4.27 ◽  
Author(s):  
V M Nakariakov ◽  
E Verwichte
Keyword(s):  
The Sun ◽  
Corona Of The Sun

The Corona of the Sun

Science ◽  
1937 ◽  
Vol 86 (2225) ◽  
pp. 8-8
Keyword(s):  
The Sun ◽  
Corona Of The Sun

scholarly journals The Bakerian lecture.―On the corona of the Sun

1886 ◽  
Vol 39 (239-241) ◽  
pp. 108-135 ◽  
Keyword(s):  
The Sun ◽  
Relative Brightness ◽  
Higher Temperature ◽  
The One ◽  
Corona Of The Sun

The sun is the only star the corona of which we have been able to observe, for all other stars are too distant to give true images in the telescope. If the sun were removed to a distance equal to that of the nearest star, its disk would subtend less than the one-hundredth of a second of arc. We have also to consider the small relative brightness of the corona, the light from which has been estimated at different times to be from 1/100000 to about the 1/400000 part of the sun’s light. It is, indeed, possible that stars which have a higher temperature than our sun, are surrounded by coronæ of greater extent and brightness.

Temperature of Polar Corona of the Sun According to Kislovodsk Observations During 1957–2002

Solar Physics ◽  
2006 ◽  
Vol 237 (1) ◽  
pp. 201-210 ◽  
Author(s):  
V. I. Makarov ◽  
A. G. Tlatov ◽  
D. K. Callebaut
Keyword(s):  
The Sun ◽  
Corona Of The Sun

scholarly journals The Large-scale Magnetic Field in the Global Solar Cycle: Observational Aspects

1991 ◽  
Vol 130 ◽  
pp. 213-217
Author(s):  
V.I. Makarov ◽  
K.R. Sivaraman
Keyword(s):  
Magnetic Field ◽  
Solar Cycle ◽  
High Latitude ◽  
Weak Magnetic Field ◽  
Large Scale ◽  
Meridional Flow ◽  
The Sun ◽  
Low Latitude ◽  
Large Scale Magnetic Field ◽  
Global Cycle

Abstract The global solar cycle is considered as an interaction of 3 types of activity: at low-latitude (sunspots), at high-latitude (polar faculae) and the weak magnetic field. The properties of single and 3-fold reversals of the polar magnetic field are considered. The variation spectrum of the large-scale magnetic field of the Sun is analyzed in the range of 1–30 nHz. A dependence between the rate of a poleward meridional flow and phase of the global cycle is discussed.

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