Coronal Emission-Line Intensities in the Extreme Ultraviolet

1966 ◽  
Vol 145 ◽  
pp. 373 ◽  
Author(s):  
W. E. Austin ◽  
J. D. Purcell ◽  
R. Tousey ◽  
K. G. Widing
Keyword(s):  
Emission Line ◽  
Extreme Ultraviolet ◽  
Coronal Emission ◽  
Line Intensities ◽  
Coronal Emission Line

A possible E-W asymmetry of the coronal emission line intensities and K-corona brightness

1994 ◽  
Vol 218 (1) ◽  
pp. 35-57 ◽  
Author(s):  
H. Mavromichalaki ◽  
V. Tritakis ◽  
B. Petropoulos ◽  
E. Marmatsouri ◽  
A. Vassilaki ◽  
...  
Keyword(s):  
Emission Line ◽  
Coronal Emission ◽  
Line Intensities ◽  
Coronal Emission Line

Solar coronal structure: A comparison of NSO/SP ground-based coronal emission line intensities and temperatures with Yohkoh SXT and WSO magnetic data

1996 ◽  
Vol 17 (4-5) ◽  
pp. 235-238 ◽  
Author(s):  
R.C Altrock ◽  
P Hick ◽  
B.V Jackson ◽  
J.T Hoeksema ◽  
X.P Zhao ◽  
...  
Keyword(s):  
Emission Line ◽  
Magnetic Data ◽  
Coronal Structure ◽  
Coronal Emission ◽  
Line Intensities ◽  
Coronal Emission Line ◽  
Solar Coronal

Coronal emission line polarization

Solar Physics ◽  
1972 ◽  
Vol 23 (1) ◽  
pp. 103-119 ◽  
Author(s):  
Lewis L. House
Keyword(s):  
Emission Line ◽  
Coronal Emission ◽  
Coronal Emission Line

scholarly journals EUV Line Intensities and the Magnetic Field in Solar Active Regions

2001 ◽  
Vol 203 ◽  
pp. 276-279
Author(s):  
J. Ireland ◽  
A. Fludra
Keyword(s):  
Magnetic Field ◽  
Extreme Ultraviolet ◽  
Active Regions ◽  
Central Meridian ◽  
Coronal Emission ◽  
Data Set ◽  
Line Intensities ◽  
Doppler Imager ◽  
Synoptic Observations ◽  
The Magnetic Field

The Coronal Diagnostic Spectrometer (CDS) on SOHO carries out daily synoptic observations of the Sun in four EUV (extreme ultraviolet) spectra: He I 584 Å, O V 630 Å, Mg IX 368 Å and Fe XVI 360 Å, over a 4 arcmin-wide strip along the solar central meridian. Using 53 active regions observed in this data set along with co-temporally observed SOHO-MDI (Michelson Doppler Imager) magnetograms we study the correlation of the chromospheric, transition region and coronal emission with the photospheric magnetic field for meridional active regions, probing the relation between the radiative output and magnetic observables. We also establish empirical, quantitative relations among intensities of different lines, and between intensities and the magnetic field flux.

The formation and interpretation of the Fe XIII 10747 A coronal emission line

1982 ◽  
Vol 255 ◽  
pp. 764 ◽  
Author(s):  
C. W. Querfeld
Keyword(s):  
Emission Line ◽  
Coronal Emission ◽  
Coronal Emission Line

Improvement of coronal emission line photographs

Solar Physics ◽  
1969 ◽  
Vol 8 (1) ◽  
pp. 88-90 ◽  
Author(s):  
Thomas Pope
Keyword(s):  
Emission Line ◽  
Coronal Emission ◽  
Coronal Emission Line

How bright is the [Si X] 1431 nm coronal emission line?

Solar Physics ◽  
1994 ◽  
Vol 151 (1) ◽  
pp. 51-56 ◽  
Author(s):  
M. J. Penn ◽  
J. R. Kuhn
Keyword(s):  
Emission Line ◽  
Coronal Emission ◽  
Coronal Emission Line

Using a New Infrared Si x Coronal Emission Line for Discriminating between Magnetohydrodynamic Models of the Solar Corona During the 2006 Solar Eclipse

2018 ◽  
Vol 852 (1) ◽  
pp. 23 ◽  
Author(s):  
Gabriel I. Dima ◽  
Jeffrey R. Kuhn ◽  
Don Mickey ◽  
Cooper Downs
Keyword(s):  
Solar Corona ◽  
Emission Line ◽  
Solar Eclipse ◽  
Coronal Emission ◽  
Coronal Emission Line ◽  
Magnetohydrodynamic Models

A program to calculate coronal emission line strengths

1977 ◽  
Vol 13 (1) ◽  
pp. 25-38 ◽  
Author(s):  
P.L. Dufton
Keyword(s):  
Emission Line ◽  
Coronal Emission ◽  
Coronal Emission Line ◽  
Line Strengths

A program to calculate coronal emission line strengths

1984 ◽  
Vol 35 ◽  
pp. C-410
Author(s):  
P.L. Dufton
Keyword(s):  
Emission Line ◽  
Coronal Emission ◽  
Coronal Emission Line ◽  
Line Strengths
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