Sentence examples for majority of anomalies from inspiring English sources

The majority of anomalies, especially in GEO satellites, occur during the midnight-to-dawn sector of magnetic local time (MLT).

It was pointed out that for the vast majority of anomalies, only the use of uterine categories was necessary, while cervical and vaginal ones were not.

Furthermore, the majority of anomalies were presented as technical failures, such as attitude loss and power drop, without identifying the cause of those conditions, such as environment, debris, or phantom command.

Previous attempts to link anomalies to magnetic activity, such as Fennell et al. (2001), showed that the majority of anomalies occurred during substorms, although not all substorms led to anomalies.

The mean local time calculation for the anomaly day with respect to the nighttime migration of energetic electrons revealed that the majority of anomalies (65%) occurred on the night side of Earth during the dusk-to-dawn sector of magnetic local time.

It was pointed out that for the vast majority of anomalies only the use of uterine categories was necessary, while cervical and vaginal ones were not.

It is clear that the majority of GEO anomalies occurred from the midnight-to-dawn sector of MLT.

This difficulty is mitigated by two facts: usually at the outset we have some idea of the kind of UXO present in the field and the (usually great) majority of detected anomalies will not be UXO and thus random digging will produce a varied sampling of the clutter present.

Generally in the literature, the majority of associated anomalies occur in cases involving clefts of the palate rather than of the lip.

While some alignment problems remain, the introduction of individual genome sequences corrects the majority of obvious anomalies and reveals a surprising amount of genetic regulatory information that was masked by alignment to the reference sequence.

The results showed that the majority of LEO satellite anomalies are linked to low-energy electron fluxes of 30 100 keV and magnetic perturbations that had a higher correlation coefficient (~ 90%) on the day of the anomaly.