| 1891 - 346 стор.
...as 1841 that the same principle, on which he had shown that a sound should become sharper or flatter if there were an approach or a recession between the...and he went on to say that the difference of colour ol some of the binary stars might be produced in this way by their motions. Doppler was right in that... | |
| 1892 - 986 стор.
...thousandth part of the whole." Doppler had also, in 1841, suggested that on the same principle on which a sound should become sharper or natter if there were...source of the sound would apply equally to light ; and Fizeau, about eight years later, had pointed out the importance of considering the individual wave-lengths... | |
| British Association for the Advancement of Science - 1892 - 1146 стор.
...as 1841 that the same principle, on which he had shown that a sound should become sharper or flatter if there were an approach or a recession between the...was wrong in the particular conclusion •which he drew from it. Even if we suppose a star to be moving with a sufficiently enormous velocity to alter... | |
| British Association for the Advancement of Science - 1892 - 1258 стор.
...as 1841 that the same principle, on which he had shown that a sound should become sharper or flatter if there were an approach or a recession between the...was wrong in the particular conclusion •which he drew from it. Even if we suppose a star to be moving with a sufficiently enormous velocity to alter... | |
| 1892 - 790 стор.
...confines of the visible universe (so long as it is bright enough), as in the case of a neighboring planet. Doppler had suggested as far back as 1841,...light ; and he went on to say that the difference of color of some of the binary stars might be produced in this way by their motions. Doppler was right... | |
| 1892 - 930 стор.
...thousandth part of the whole." Doppler had also, in 1841, suggested that on the same principle on which a sound should become sharper or natter if there were...source of the sound would apply equally to light ; and Fizeau, about eight years later, had pointed out the importance of considering the individual wave-lengths... | |
| Smithsonian Institution. Board of Regents - 1893 - 786 стор.
...confines of the visible universe (so long as it is bright enough), as in the case of a neighboring planet. Doppler had suggested as far back as 1841,...light; and he went on to say that the difference of color of some of the binary stars might be produced in this way by their motions. Doppler was right... | |
| Smithsonian Institution. Board of Regents - 1893 - 816 стор.
...confines of the visible universe (so long as it is bright enough), as in the case of a neighboring planet. Doppler had suggested as far back as 1841,...the sound, would apply equally to light; and he went onto say that the difference of color of some of the binary stars might be produced in this way by... | |
| Royal Astronomical Society - 1893 - 594 стор.
...an extension of the principle on -which he had shown that a sound should become sharper or flatter, if there were an approach or a recession between the ear and the source of the sound. Doppler supposed that stars might in this waj change their colour as observed by eye, but he did not... | |
| Royal Astronomical Society - 1893 - 586 стор.
...an extension of the principle on -which he had shown that a sound should become sharper or flatter, if there were an approach or a recession between the ear and the source of the sound. Doppler supposed that stars might in this way change their colour as observed by eye, but he did not... | |
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