Sentence examples for maximum obscuration and from inspiring English sources

Three vertical lines stand for the first contact, maximum obscuration, and last contact of eclipse.

The left panels are during the maximum obscuration, and the right panels are after the maximum obscuration.

Cooling by 3 5°C in the 50 52-km 50 52-kmnd a decrease in wind speed clayerto the mandmum obscuration andecreaserease in wind speed towards the end of the eclosee, were observed during tois partheular event.

Solar eclipses are rare events and each eclipse is unique with respect to the time of their occurrence, the percentage of the maximum obscuration, and the path of the eclipse.

In general, a substantial increase in the amplitude of shorter (2 8 km) vertical wavelengths in the zonal and meridional wind components in the troposphere and stratosphere during the maximum obscuration, and even after 2 hours of the maximum obscuration, is found on the eclipse day compared to that on control day.

The amplitude of larger (10 16 km) vertical wavelengths remains almost the same during, and after, the maximum obscuration in the troposphere and stratospheric region and this can be attributed to short-period planetary waves not associated with the eclipse.

Measurements of temperature and winds in the middle atmospheric region were made over the equatorial station Thumba (8.5°N, 77°E), using balloons, rockets and meteor wind radar during, and after, the maximum obscuration of the Sun.

The observations were made during, and after, the maximum obscuration on the day of the eclipse, as well as at the same time on a control day.

The first contact of the annular eclipse at Thumba was at 11 04 IST (= GMT + 5 30 hr), the maximum obscuration of ~92% was at 13:14IST and the last contact was at 15:05 IST.

The zonal and meridional wind measurements on 14 and 15 January, 2010, using balloon (12 30 13 30 IST), rocket (13:07 13 30 IST), and meteor wind radar (12 30 13 30 IST), observations around the maximum obscuration of the Sun in the height regions of 0 65 and 82 98 km are analysed to look for the perturbations in wind components and the resulting dynamical processes.

Height profiles of (a) zonal, and (b) meridional, winds in the 0 65-km height region measured using balloon and rocket ascents during 12:30 65-km IST (theightimum obscuregion).