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DMP estimated from 22 h measurements correlated moderately well with 2 h emission measures (r2 of 0.42 0.48) and 1 h measures (r2 of 0.39 0.43).
We obtain four temperatures: 1.6, 5.2, 8.2, and ≳20 MK, emission measures and abundances.
The emission measures derived from the radio observation may also contain errors.
That means the radio and EUV emission measures required the different filling factors.
However, short-term emission measures have been reported to correlate well with DMP.
We discuss the brightness temperatures, emission measures and the hard X-ray spectral properties of these microevents.
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cI3 stands for reduced CO2 emission, measured in × 10 4g/bit.
(c) Peak emission measure derived from AIA observations.
The spatial distribution of the emission measure derived from the NoRH data corresponded well with that of the peak emission measure from the AIA data.
The column emission measure and T of the coronal plasma can be derived from the EUV flux (hereafter, the EM means the column emission measure in this paper).
The average emission measure of the LT region was 4.2 × 1025 (cm−5).
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