The following sections have been revised in category 90 Geophysics, Astronomy, and Astrophysics:
N - new (red); M - modified (blue)--- [2001 text for modified codes in green]; D - deleted (purple).
91.60.-x Physical properties of rocks and minerals (for rheological properties of geological materials, see 83.50 and 83.80.Nb)
91.60.Ba Elasticity, fracture, and flow
91.60.Dc Creep and deformation
91.60.Ed Crystal structure and defects
91.60.Fe Equations of state
91.60.Gf High-pressure behavior
91.60.Hg Phase changes
91.60.Ki Thermal properties
91.60.Lj Acoustic properties
91.60.Mk Optical properties
M 91.60.Pn Magnetic and
electric properties; environmental magnetism ---[Original
text: Magnetic and electric properties]
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96.50.-e Interplanetary space (for asteroids, see 96.30.Ys)
M 96.50.Bh Solar and interplanetary electric and magnetic fields (including solar wind fields) [Original text: Solar electric and magnetic fields (including solar wind fields)]
96.50.Ci Solar wind plasma
96.50.Dj Interplanetary gas and dust (including gegenschein and zodiacal light)
96.50.Ek Solar wind interactions with planets, satellites, and comets (for interactions with Earth, see 94.30.Va)
96.50.Fm Shock waves
96.50.Gn Comets
96.50.Hp Oort cloud
96.50.Jq Kuiper belt
96.50.Kr Meteors, meteoroids, and meteor streams
96.50.Mt Meteorites, micrometeorites, and tektites
96.50.Pw Particle acceleration
96.50.Qx Stream-stream interactions
96.50.Ry Waves and discontinuities
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96.60.-j Solar physics
96.60.Bn Diameter, figure, rotation, mass
96.60.Fs Chemical composition
96.60.Hv Electric and magnetic fields
96.60.Jw Solar interior (for solar neutrinos, see 26.65.+t in nuclear astrophysics)
96.60.Ly Oscillations and waves; helioseismology
96.60.Mz Photosphere, granulation
96.60.Na Chromosphere and chromosphere–corona transition; spicules
96.60.Pb Corona; coronal loops, streamers, and holes
96.60.Qc Sunspots, faculae, plages
96.60.Rd Flares, bursts, and related phenomena
96.60.Se Prominences
96.60.Tf Solar electromagnetic radiation (see also 92.60.Vb Solar radiation in meteorology )
M 96.60.Vg Particle radiation, solar wind, and solar neutrinos (see also 96.50.Ci Solar wind plasma and 96.50.Ek Solar wind interactions with planets, satellites, and comets) [Original text: Particle radiation, solar wind (see also 96.50.Ci Solar wind plasma and 96.50.Ek Solar wind interactions with planets, satellites, and comets)]
96.60.Wh Coronal mass ejection
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98.80-k Cosmology (see also 04 General relativity and gravitation; for origin and evolution of galaxies, see 98.62.Ai; for elementary particle and nuclear processes, see 95.30.Cq; for dark matter, see 95.35.; for superclusters and large-scale tructure of the Universe, see 98.65.Dx)
98.80.Bp Origin and formation of the Universe
M 98.80.Cq Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.) [Original text: same] (see also 11.25.-w Strings and branes, and 11.10.-z in general theory of fields and particles)
98.80.Es Observational cosmology (including Hubble constant, distance scale, cosmological constant, early Universe, etc)
98.80.Ft Origin, formation, and abundances of the elements (see also 26.35 Big Bang nucleosynthesis)
D 98.80.Hw Mathematical and relativistic aspects of cosmology; quantum cosmology (see also 04.60 Quantum gravity in general relativity and gravitation)
N 98.80.Jk Mathematical and relativistic aspects of cosmology (see also 04.20.-q Classical general relativity)
N 98.80.Qc Quantum cosmology (see also
04.60 Quantum gravity in general relativity and gravitation)
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D 99.10.+g Errata
N 99.10.-x Errata and other corrections
N 99.10.Cd Errata
N 99.10.Fg Publisher's note
N 99.10.Jk Corrected
article
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