Sentence examples for disturbed time from inspiring English sources

Figure 5 Comparison of the coherences during a disturbed time and a slightly disturbed time at Kakioka.

Also we can observe the fade-out of the ionospheric layers at night during the geomagnetically disturbed time periods.

The coherences of the geoelectric and geomagnetic fields during a magnetic storm (circles) and during a slightly disturbed time (squares) for Kakioka are shown.

To estimate the errors, we use intensity profiles for airglow red emission presented by Sakai et al. (2014), which showed that the airglow emission of polar cap patches is peaked at ~280 km altitude during disturbed time.

On average, the irregularity index has dropped from 400 (0.4 TECU/min) during quiet time to 50 (0.05 TECU/min) on disturbed time with an amount of 350 (0.35 TECU/min).

Experimentally observed plasma pressure distribution in the inner magnetosphere during quiet and disturbed time is analyzed.

It is clear that SUIPEs are more likely to occur during magnetically disturbed times.

Figure 4 shows that SUIPEs are more likely to occur during magnetically disturbed times, possibly related to auroral activity in the vicinity of the radar beam.

The X component, in particular, is known to be contaminated at mid-latitudes by magnetic fields generated by high-latitude currents during geomagnetically disturbed times, and at low latitudes by the equatorial electrojet.

There is a clear preference for this type of uniform power enhancement to occur during magnetically disturbed times, possibly indicating an association with auroral activity in the vicinity of the radar beam.

The use of the POES observations also has problems as highlighted by Rodger et al. ([2010]): During geomagnetically disturbed times, i.e. when electron precipitation is likely to occur, up to 55% of the POES bounce loss cone electron flux (electrons precipitating into the atmosphere) observations are contaminated by energetic protons.