The Visibitlity of the 10-CM Radio-Emissive Region and its Application in Finding the 10-CM Quiet Sun.

1960 ◽  
Vol 132 ◽  
pp. 435 ◽  
Author(s):  
Arthur E. Covington ◽  
Gladys A. Harvey
Keyword(s):  
Quiet Sun ◽  
Emissive Region

Interpretation of the Filament Depression at Millimetric and Centimetric Wavelengths

1979 ◽  
Vol 44 ◽  
pp. 131-134
Author(s):  
A. Raoult ◽  
P. Lantos ◽  
E. Fürst
Keyword(s):  
Radio Telescope ◽  
Active Regions ◽  
Simple Shape ◽  
Quiet Sun ◽  
Unstable Process

The depressions at centimetric and millimetric wavelengths associated with the filaments are studied using already published maps as well as unpublished observations from the Effelsberg 100 m radio telescope of the M.P.I., Bonn. The study has been restricted to large Ha quiescent prominences of relatively simple shape, situated far from the limb and from active regions. The data has been reduced employing one method whose main characteristics are choice of a local quiet sun definition and avoidance of the unstable process of deconvolution.

SUMER Observations of the Quiet‐Sun Transition Region

1999 ◽  
Vol 512 (2) ◽  
pp. 992-1005 ◽  
Author(s):  
N. W. Griffiths ◽  
G. H. Fisher ◽  
D. T. Woods ◽  
O. H. W. Siegmund
Keyword(s):  
Transition Region ◽  
Quiet Sun

scholarly journals SELF-CANCELLATION OF EPHEMERAL REGIONS IN THE QUIET SUN

2012 ◽  
Vol 752 (2) ◽  
pp. L24 ◽  
Author(s):  
Shuhong Yang ◽  
Jun Zhang ◽  
Ting Li ◽  
Yang Liu
Keyword(s):  
Quiet Sun

The solar chromosphere and corona: Quiet Sun

1977 ◽  
Vol 25 (9) ◽  
pp. 893-894
Author(s):  
Carole Jordan
Keyword(s):  
Solar Chromosphere ◽  
Quiet Sun

QUIET-SUN INTENSITY CONTRASTS IN THE NEAR-ULTRAVIOLET AS MEASURED FROM SUNRISE

2010 ◽  
Vol 723 (2) ◽  
pp. L154-L158 ◽  
Author(s):  
J. Hirzberger ◽  
A. Feller ◽  
T. L. Riethmüller ◽  
M. Schüssler ◽  
J. M. Borrero ◽  
...  
Keyword(s):  
Quiet Sun ◽  
Near Ultraviolet

scholarly journals DYNAMICS OF MULTI-CORED MAGNETIC STRUCTURES IN THE QUIET SUN

2015 ◽  
Vol 810 (1) ◽  
pp. 79 ◽  
Author(s):  
Iker S. Requerey ◽  
Jose Carlos Del Toro Iniesta ◽  
Luis R. Bellot Rubio ◽  
Valentín Martínez Pillet ◽  
Sami K. Solanki ◽  
...  
Keyword(s):  
Quiet Sun ◽  
Magnetic Structures

scholarly journals Two types of coronal bright points their characteristics, and evolution

2010 ◽  
Vol 6 (S273) ◽  
pp. 343-346
Author(s):  
Isroil Sattarov ◽  
Nina V. Karachik ◽  
Chori T. Sherdanov ◽  
Azlarxon M. Tillaboev ◽  
Alexei A. Pevtsov
Keyword(s):  
Maximum Brightness ◽  
Quiet Sun ◽  
Coronal Bright Points

AbstractUsing maximum brightness of coronal bright point's (CBP) as a criterion, we separate them on two categories: dim CBPs, associated with areas of a quiet Sun, and bright CBPs, associated with an active Sun. This study reports on characteristics of two types of CBPs and their evolution.

Ca II K line profile of the truly quiet Sun

Solar Physics ◽  
1996 ◽  
Vol 163 (1) ◽  
pp. 93-97 ◽  
Author(s):  
K. R. Sivaraman ◽  
S. S. Gupta ◽  
R. Kariyappa
Keyword(s):  
Line Profile ◽  
Quiet Sun
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