What is it about?

Bursty bulk flows (BBFs) are transient phenomena in the magnetotail of earth, high speed streams of ions. These high speed streams constitute a significant part of the mass transfer from the tail back towards earth, a part of the magnetospheric circulation. The BBFs are dominated by and typically determined from measurements of the dominant ion, protons. We have studied how oxygen ions respond to BBFs. It is found that oxygen ions essentially do not take part in the proton BBFs, the oxygen ions observed during proton BBFs are not or only weakly accelerated. In general oxygen ions have much lower velocity than protons. We show that this is in part due to the large gyro radius of oxygen ions in the central magnetotail.

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Why is it important?

The circulation of oxygen ions may be important for the total loss of atmosphere from a magnetized planet such as earth, as the return flux of ions in the tail may reduce the atmospheric loss. More important i sthat oxygen ions affect the magnetosphere dynamics during magnetic storms and it is well established that the magnetosphere is enriched in oxygen content during storms. The slower transport of oxygen ions during storms will contribute to this engancement.

Perspectives

Protons and oxygen ions often show different behavior in the magnetosphere. To some extent this is due to different sourcfes, where the solar wind is an importnat (but not only) source of protons, the oxygen ions come from the ionosphere. Different gyro periods also frequently lead to different degree of heating of the ions due to wave-particle interaction. In this study we see differences in the central magnetotail (plasma sheet) and this seems related to the different gyro radius of protons and oxygen. We can therefore probe the detailed physics in better detail by comparing proton and oxygen ions in different regions of the magnetosphere.

dr Hans Nilsson
Institutet for rymdfysik

Read the Original

This page is a summary of: Oxygen ion response to proton bursty bulk flows, Journal of Geophysical Research Space Physics, August 2016, American Geophysical Union (AGU),
DOI: 10.1002/2016ja022498.
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