Encyclopedia of Physical Science and Technology, Volume 2Academic Press, 1992 - Physical sciences |
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Page 161
... solar atmo- sphere versus altitude . Note that a minimum tempera- ture is reached just above the visible - light surface , or photosphere , and temperature rises sharply in the transition region between the chromosphere and co- rona ...
... solar atmo- sphere versus altitude . Note that a minimum tempera- ture is reached just above the visible - light surface , or photosphere , and temperature rises sharply in the transition region between the chromosphere and co- rona ...
Page 412
Van Allen belt Solar wind particle Proton • Electron Solar magnetic field line - Magnetotail Magnetopause Plasma shoot EARTH FIG . 9. Schematic illustration of the noon - midnight meridian cross section of the magnetosphere . Solar wind ...
Van Allen belt Solar wind particle Proton • Electron Solar magnetic field line - Magnetotail Magnetopause Plasma shoot EARTH FIG . 9. Schematic illustration of the noon - midnight meridian cross section of the magnetosphere . Solar wind ...
Page 414
... solar wind - magnetospheric generator , there is a high probability that the power will increase ( according to the formula given in Section VI , A ) . Some flares , however , produce a large ℗ ( ~ 180 ° ) , while others produce a small ...
... solar wind - magnetospheric generator , there is a high probability that the power will increase ( according to the formula given in Section VI , A ) . Some flares , however , produce a large ℗ ( ~ 180 ° ) , while others produce a small ...
Contents
Guide to Using the Encyclopedia ix Atomic Physics | 339 |
Approximations and Expansions 1 Atomic Spectrometry | 357 |
Archaeological Geology 31 Atomic Spectroscopy | 381 |
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absorption acid aldoses angular momentum approximation asbestos atmosphere atoms auroral BASIC battery black hole Boolean algebra carbon fibers catalyst cell chemical chrysotile clouds collision complex components concentration convection cross section curve density developed disaccharide disk distribution dust electron elements emission emitted energy engine equations example expert system flux function galaxies heat hydrogen hydroxyl groups infrared input interaction interstellar interstellar medium ionization ions mass material measurements mechanism ment metal molecular molecules monosaccharides neutron stars nucleophile observed oligosaccharides operator orbital oxidation oxygen parameter particles photons plume problem radiation reaction reactor region result saccharide solar solution space spectral spectroscopy spectrum speed spline stable stars stellar structure surface techniques telescope temperature Theorem thermal tion tive turbulence ture typical variable velocity vertical wave wavelength weight white dwarf wind