Sentence examples for wind density from inspiring English sources

Frequency analysis of both solar wind density (WIND) and INTERBALL magnetic field showed that the solar wind pressure variation contains the same spectrum (2.4 4.4 mHz).

As we move farther away from the Sun, the solar wind density decreases and consequently, its pressure as well.

Solar wind density compressions from stream interactions and interplanetary coronal mass ejections (ICMEs) (left) and SEP events (right) are seen at the orbits of Earth and ‪ ‎MAVEN‬.

We assumed that the plasma sheet density depends linearly on the solar wind density.

It is found that the O+ ion escape rate increases with increasing solar wind density.

For example, biofuel production requires large quantities of agricultural land, while wind farms require land with sufficient wind density.

The factors of secondary importance, marginally contributing to overall statistical quality, are IMF By, solar wind density, and IMF fluctuations.

The O+ ion escape rate saturates when the solar wind density becomes high (above 100 cm−3).

This behavior can be explained by the higher mean relative velocity of the solar wind density inhomogeneities traversing the radio ray path.

They are driven by fluctuations of the solar wind density and dynamic pressure at the same frequencies, via the modulation of the magnetopause current.

The solar wind and magnetosheath parameters correlate better for larger solar wind density and interplanetary magnetic field magnitude values and for larger relative standard deviations of their parameters.