South Pole Neutron Monitor

Data courtesy of Bartol Research Institute, Delaware
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A neutron monitor is an instrument that measures the number of high-energy particles impacting Earth from space.

For historical reasons these particles, mostly protons and helium nuclei, are called “cosmic rays.” Because the intensity of cosmic rays hitting Earth is not uniform, it is important to place neutron monitors at multiple locations in order to form a complete picture of cosmic rays in space.

Bartol Research Institute currently operates eight neutron monitors.
The South Pole monitor is located (not surprisingly) at Lat: 90°S, Lon:–

Cosmic ray rates are affected by solar wind strength and density, and therefore CMEs can have a major effect when they “sweep away” some of the neutrons within the area of the earth’s magnetic field. The first image below shows the effect of a CME impacting earth on 2017-07-16 following an M1.4 (semi) earth-directed solar flare. This is called a “Forbush Decrease”. Cosmic ray bursts are caused by supernovae and other galactic events.

The second image shows a Forbush decrease following an X9 flare and earth-directed CME on 2017-09-07. It also shows a minor “Ground Level Event” where protons have reached ground level following a large X8.3 flare (from the same sunspot group). These events can cause an increase in radiation dose particularly for high altitude flyers especially flying over polar routes.

For further very detailed background information see here.

nutron_cme
An M1.4 flare followed by a CME caused this dip in the cosmic ray induced neutron count at the South Pole on 16 July 2017

 

Forbush decrease followed by minor Ground Level Event

 

Disclaimer for live data

Should not be used for scientific research purposes.
Use of these data for any purpose is “at your own risk.”

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