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- W2034118810 abstract "The variations in total brightness of a comet when it is most active, near perihelion, are presently used as the bases of a volatility index (VI) for short-period (SP) and long-period (LP) comets. Volatility does not correlate with period among the LP comets, and thereby shows no 'aging' effect; similarly, the VI measurements are the same for SP and for LP comets and exhibit no correlation with (1) absolute magnitude near perihelion, (2) orbital inclination, or (3) activity index measuring the intrinsic brightness change from great solar distances to the maximum near perihelion. Active comets are shown to be basically alike irrespective of their orbits or 'ages'." @default.
- W2034118810 created "2016-06-24" @default.
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- W2034118810 date "1992-07-01" @default.
- W2034118810 modified "2023-09-27" @default.
- W2034118810 title "A volatility index for comets" @default.
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- W2034118810 doi "https://doi.org/10.1016/0019-1035(92)90211-o" @default.
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