On the Nature of the Solar Corona, with some Suggestions for Work at the next Total Eclipse

Nature ◽  
1901 ◽  
Vol 63 (1627) ◽  
pp. 230-231
Author(s):  
R. W. WOOD
Keyword(s):  
Solar Corona ◽  
Total Eclipse

Spectropolarimetric analysis of the solar corona during the 12 November 1966 total eclipse

Solar Physics ◽  
1971 ◽  
Vol 17 (1) ◽  
pp. 89-96 ◽  
Author(s):  
B. Caccin ◽  
G. Moschi ◽  
M. Rigutti ◽  
R. Falciani
Keyword(s):  
Solar Corona ◽  
Total Eclipse

Structure and photometry of the solar corona at the total eclipse of 1997 March 9

2000 ◽  
Vol 24 (2) ◽  
pp. 211-216 ◽  
Author(s):  
Zhong-wei Hu ◽  
Cheng Fang ◽  
Shi-zhong Xu ◽  
Jia-rong Yan ◽  
Yong Wang ◽  
...  
Keyword(s):  
Solar Corona ◽  
Total Eclipse

On the Continuous Spectrum of the Solar Corona at the Total Eclipse in 1943

1950 ◽  
Vol 5 (2) ◽  
pp. 106-110
Author(s):  
Tutomu Tanaka ◽  
Hirobumi Oura ◽  
Tosio Murakami ◽  
Takio Mitunobu
Keyword(s):  
Solar Corona ◽  
Continuous Spectrum ◽  
Total Eclipse

On the Spectrum of the Solar Corona at the Total Eclipse in 1943. II. On the Continuous Spectrum

1946 ◽  
Vol 1 (1) ◽  
pp. 30B-30B
Author(s):  
Tutomu Tanaka ◽  
Hirobumi Oura ◽  
Tosio Murakami ◽  
Takio Mitunobu
Keyword(s):  
Solar Corona ◽  
Continuous Spectrum ◽  
Total Eclipse

On the Spectrum of the Solar Corona at the Total Eclipse in 1943. I. On the Coronal Lines

1946 ◽  
Vol 1 (1) ◽  
pp. 30A-30A
Author(s):  
Tutomu Tanaka ◽  
Hirobumi Oura ◽  
Tosio Murakami ◽  
Takio Mitunobu
Keyword(s):  
Solar Corona ◽  
Total Eclipse

scholarly journals The Solar Corona during the Total Eclipse on 1806 June 16: Graphical Evidence of the Coronal Structure during the Dalton Minimum

2020 ◽  
Vol 900 (2) ◽  
pp. 114
Author(s):  
Hisashi Hayakawa ◽  
Mathew J. Owens ◽  
Michael Lockwood ◽  
Mitsuru Sôma
Keyword(s):  
Solar Corona ◽  
Coronal Structure ◽  
Total Eclipse ◽  
Dalton Minimum

Colour Photometry of the Solar Corona of July 11, 1991

1994 ◽  
Vol 144 ◽  
pp. 597-599 ◽  
Author(s):  
I. V. Alexeyeva ◽  
N. L. Kroussanova ◽  
M. V. Streltsova
Keyword(s):  
Solar Corona ◽  
Red Emission ◽  
Coronal Structures

AbstractThe results of photometry of colour positives of the solar corona of July 11, 1991 are presented. Observations of the white corona were made without radial niters in Jojutla (Mexico). Dependences of coronal brightness on distance in the red (640 nm) and blue (420 nm) wavelength intervals are deduced for different coronal structures up to 3.0-3.5R⊙. The effect of ”reddening“ is noted. The excess of the red emission to the blue one (I640nm/I420nm) is found to be 1.20 and 1.17 at distance of 2.2R⊙for the N-E helmet streamer (P ≃ 37°) and the N-W region of low brightness (P ≃ 339°), respectively.

July 11, 1991 Eclipse Corona Photometry by the Results of Electropolarimetric and CCD-Matrix Observations

1994 ◽  
Vol 144 ◽  
pp. 567-569
Author(s):  
V. Kulidzanishvili ◽  
D. Georgobiani
Keyword(s):  
Solar Corona ◽  
Observational Data ◽  
Solar Limb ◽  
Ccd Matrix

AbstractThe observational data of July 11, 1991 eclipse solar corona obtained by both electropolarimeter (EP) and CCD-matrix were processed. Using these data, the solar corona photometry was carried out. The results of EP data are compared with the ones of CCD data. It must be noted here that the CCD data give us only characteristics of the inner corona, while the EP data show the features of both the inner and middle corona up to 4R⊙. Standard flattening indexϵis evaluated from both data. The dependence of the flattening index on the distance from the solar limb is investigated. The isophotes in Na and Ca lines are plotted. Based on these data some ideas and conclusions on the type of the solar corona are presented.

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