Tags: West Asia Solar Solar Pv

4 FAQs about West asia solar rotation

What is solar rotation?

Solar rotation is the rotation of the Sun about its own axis. The Sun is not a solid body, but is composed of a gaseous plasma, and different latitudes rotate with different periods. The solar rotation period is 25.67 days at the equator and increases with increasing latitude, reaching 33.40 days at 75 degrees of latitude.

How often does the Sun rotate on its axis?

The Sun rotates on its axis once in about 27 days. This rotation was first detected by observing the motion of sunspots. The Sun's rotation axis is tilted by about 7.25 degrees from the axis of the Earth's orbit so we see more of the Sun's north pole in September of each year and more of its south pole in March.

How does solar activity affect monsoonal East Asia?

Further analyses suggest that intensified decadal to centennial solar activity can lead to enhanced and northward and westward extension of the western Pacific subtropical high, resulting in tripolar rainfall heterogenous patterns over monsoonal East Asia.

Is rainfall heterogeneity present in Southeast Asia and North China?

Here we show that such rainfall heterogeneity has been present at least in the last millennium, with decadal to centennial precipitation variations over southeast Asia and north China being broadly synchronous, while central to southwest China's variations are generally out-of-phase with those in southeast Asia and north China.

View/Download West asia solar rotation [PDF]

PDF version includes complete article with source references. Suitable for printing and offline reading.