In
situ combustion (ISC) has been regarded as an efficient technique
for the exploitation of heavy oil reserves. In this work, the thermal
behavior of one heavy crude oil and the fractions of its saturates,
aromatics, resins, and asphaltenes (SARA) during combustion was thoroughly
investigated using high-pressure differential scanning calorimetry.
Two typical isoconversional methods were adopted to determine the
variation of activation energy (E) and frequency
factor (A
r) versus conversion degree in
the course of the reaction, followed by the evaluation of the reaction
model, f(α), via the master plot method. The
results indicated that the heavy oil encountered larger thermal release
caused by low-temperature oxidation (LTO) reactions rather than high-temperature
oxidation (HTO) reactions, suggesting that appreciable heat could
be available within the low-temperature range. Saturates showed a
notably apparent heat release in the LTO reactions. For aromatics,
the exothermic effect at the LTO stage was apparently higher than
that at the HTO stage, contrary to the results detected at atmospheric
pressure. Saturates and asphaltenes gave the highest cumulative heat
release in the LTO and HTO regions, respectively. The variation of
kinetic parameters (E and A
r) versus conversion degree during combustion was quite different
for the heavy oil and its SARA fractions, implying their varying reaction
mechanisms and pathways. Saturates exhibited the lowest average value
of E at the LTO stage, whereas aromatics and resins
gave the lowest average value of E at the HTO stage.
The most probable f(α) of the LTO interval
for the oil and its SARA fractions followed power law reaction models
P–0.6, P–0.3, P0.1,
P0.05, and P0.2. The appropriate f(α) for the HTO interval of the oil, saturates, and aromatics
was the chemical process or mechanism non-invoking equations F2.1, F0.8, and F0.6, respectively. The
Sestak–Berggren reaction model SB(0.5,0.9) and Avrami–Erofeev
reaction model A2 were regarded as the rational f(α) for the HTO region of resins. These observations
could provide some guidance with regard to the numerical modeling
of SARA fractions to simulate the ISC process.