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Fig. 3. Left: the C/2001 C2 Ly α counts (summed over the slit length) versus time
curve as observed at 3.6 R (solid line) and the curve fit (dotted line). Right: the iso- χ 2
curves for the determination of the ( τ ion , t st )valuesatwhichthe χ 2 value is minimum
(see text).
second produced by outgassing) and to the unknown ionization and charge
exchange rates ( τ 1
ion
cx , respectively). These are proportional 11 , 12 to
the local electron density n e encountered by the comet. The N coma atoms
undergo a charge transfer with the ambient protons creating a number N tail
of neutrals (responsible for the observed Ly α emission)atarate τ 1
and τ 1
cx :this
process locally increases the number density of H atoms with respect to
the coronal density. As a consequence, the number of H atoms N tail left
by the comet along its path exponentially decays as exp(
t/τ ion )untilthe
cometary Ly α signal disappears (Fig. 3, left panel). By fitting with an expo-
nential curve (depending on N , τ ion ,thetime t st at which the comet first
entered the slit and other known parameters) the observed Ly α intensity
decay after the comet transit, it is possible to derive an estimate for the
cometary outgassing rate N and the local electron density n e (Fig.3,right
panel). Assuming a balance between the energy supplied by the solar radia-
tion impinging on a spherical nucleus and the energy required to sublimate
the quantity of ice derived from the N value, we may estimate (for isotropic
outgassing) the nucleus equivalent radius.
Table 1 gives the results obtained at different heliocentric distances
h (R ) of the comet for the sungrazers C/1996 Y1, C/2000 C6, and C/2001
C2, in particular the ice mass outgassed per second Q H 2 O (kg/s) and the
estimated nucleus radius r (m). An interesting result from Table 1 is the
UVCS detection of a significant surviving mass even after the comets disap-
peared from the LASCO/C2 FOV (hence below 6 R ), implying the pres-
ence at very low heliocentric distances of a hidden mass “inconsistent with
the nominal models based on the coronagraphic observations alone”. 13 This
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