 ... rapidly lose heat; but, on the other hand, liquid or solid particles, whether originally carried up as such, or subsequently formed by condensation, would absorb the sun's heat, and at coronal distances would soon rise to a temperature not...  The Observatory - Page 1511885Full view - About this book
 | 1885 - 1234 pages
...in the near neighbourhood of the sun would be very different from that of liquid or solid particles. A gas need not be greatly heated, even when near the sun, by the radiated solar energy ; the hot gas from the photosphere would probably rapidlv lose heat ; but, on the other... | |
 | 1885 - 858 pages
...in the near neighborhood of the sun would be very different from that of liquid or solid particles. A gas need not be greatly heated, even when near the sun, by the radiated solar energy ; the hot gas from the photosphere would probably rapidly lose heat; but, on the other... | |
 | 1885 - 846 pages
...in the near neighborhood of the sun would be very different from that of liquid or solid particles. A gas need not be greatly heated, even when near the sun, by the radiated solar energy; the hot gas from the photosphere would probably rapidly lose heat; but, on the other... | |
 | Smithsonian Institution. Board of Regents - 1886 - 1026 pages
...great difference in the behavior of a gas and of liquid and solid particles in the immediate vicinity of the sun. A gas need not be greatly heated even when near the sun by the radiated energy ; when once heated it would rapidly lose its heat when above the photosphere ; but solid and liquid... | |
 | 1885 - 1098 pages
...in the near neighbourhood of the sun woidd be very different from that of liquid or solid particles. A gas need not be greatly heated, even when near the sun, by the radiated solar energy ; the hot gas from the photosphere would probably rapidly lose heat ; but, on the other... | |
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