Sentence examples for flare strength from inspiring English sources

The plots reveal that ΔH′ increases linearly with increasing flare strength.

According to Thomson et al. (2005), the D-region could be used as a solar flare strength indicator for flares greater than class X17 (for which the GOES detector saturates) up to X45 by extrapolating the phase profile.

Coincident with the occurrence of a large number of X-ray dips, a huge radio flare of strength 0.48 Jy (at 2.25 GHz) was found from the NRAO archival data.

The solar flares of strength C1.0 to C1.3 during the period of low solar activity produced perturbations, whereas flares of same class did not produce any detectable perturbations during the period of moderate solar activity, which is due to the higher sensitivity of the D-region during low solar activity.

where f, B, and L correspond to the fraction of energy released by a flare, the magnetic field strength of the starspots and the scale length of the starspot group respectively.

Their results showed that for a given strength solar flare, ΔH′ will be approximately 1 km greater during the solar minimum period than during the solar maximum, which is in agreement with our findings.

A flared edge provides extra strength at the rim and allows cooked eggs to slip out of the pan easily.

For example, it is estimated from the plots of McRae and Thomson (2004) for solar flares around 4 dB strength (equivalent to C2.5 class); the β values were 0.39 km−1 for solar minimum and 0.41 km−1 for moderate solar activity.

In contrast, our results indicate greater β values for the solar minimum than for the period of moderate solar activity for the same strength of flares, i.e., 0.35 km−1 and 0.33 km−1, respectively.

M-class solar flares are medium-strength sun storms that can still unleash powerful blasts of radiation and magnetic solar plasma.

Thomson et al. (2004) has estimated its strength of the flare as large as X45 ± 5 via other means.