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The flux intensities corresponding to different classes of the flares are given in Table 1.
The variations in the amplitude of NWC signal along with the respective X-ray flux intensities during both the flares are shown in Figure 3a, b.
A feature of interest seen here is the time difference in the peak occurrences of the solar flux intensities and the respective amplitudes during these flares.
Solar flares are classified in different categories, namely A, B, C, M and X in the 'XL' band, based on the peak flux intensities (in W/m2).
An excellent agreement between measured and simulated flux intensities over the whole energy range at the sample position for the X-ray beamline SUL has been found.
It is demonstrated that the optical performance of Fresnel array is very close to that of PTC, with similar values of maximum flux intensities.
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The open circuit solenoid coil was designed as the magnetic circuit for magnetic flux intensity.
Also presented are sensitivity analysis, temperature, heat flux intensity and manufacturing constraints of the relevant design.
In this paper, spatial distribution of neutron flux intensity was evaluated by foil activation method.
During these flares, the NWC amplitude and phase enhancements showed clear proportional variation with the X-ray flux intensity.
The amplitudes of VTX and NLK with the corresponding solar flux intensity are presented in Figure 3e, f.
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