| James Samuelson, William Crookes - Science - 1865 - 874 pages
...the corona and " red flames " were in this way exhibited to the audience. These photographs showed that as the moon proceeded over the sun's disc, the...which she was approaching ; thus showing that they belonged to the sun. Next, with regard to the photosphere, the first thing to be noticed is the fact... | |
| Chemistry - 1865 - 332 pages
...total eclipse which happened in Spain in July, 1860. These photographs (which were exhibited) showed that as the moon proceeded over the sun's disc the...which she was approaching ; thus showing that they belonged to the sun. Another proof in favour of these bodies belonging to the son is derived from the... | |
| Chemistry - 1865 - 640 pages
...total eclipse which happened in Spain in July, 1860. These photographs (which were exhibited) showed that as the moon proceeded over the sun's disc the...disc at that side towards which she was approaching; Una showing that they belonged to the sun. Another proof in favour of these bodies belonging to the... | |
| Royal Institution of Great Britain - Science - 1866 - 730 pages
...au extensive solar atmosphere. It appeared to the Astronomer Royal and some others as probable that these bodies belong to the sun ; but their connection...showing that they belong to the sun.) Another proof iu favour of the idea that the red flfKues belong to the sun is derived from the nature of the light... | |
| Mary Somerville - Matter - 1869 - 454 pages
...certainly belong to the sun ; for during the total eclipse in 1860 it was observed, that as the moon moved over the sun's disc, the red flames and part of the corona discovered themselves at the side which she had left, and were covered by her disc at the side towards which she was approaching.... | |
| Royal Institution of Great Britain - Science - 1866 - 742 pages
...Royal and some others as probable that these bodies belong to the sun ; but their connection witli our luminary was put beyond doubt by Mr. De la Rue,...from the nature of the light which they emit. This h:ts great photographic power compared to its luminosity, so much so that one prominence was photographed... | |
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