Cold Ion Demagnetization near the X-line of Magnetic Reconnection
Although the effects of magnetic reconnection in magnetospheres can be observed at planetary scales, reconnection is initiated at electron scales in a plasma. Surrounding the electron diffusion region, there is an Ion-Decoupling Region (IDR) of the size of the ion length scales (inertial length and...
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Veröffentlicht in: | Geophysical research letters 2016-07, Vol.43 (13), p.6759-6767 |
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Hauptverfasser: | , , , , , , , , , , , , , , , , , , , , , , , , |
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Sprache: | eng |
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Zusammenfassung: | Although the effects of magnetic reconnection in magnetospheres can be observed at planetary scales, reconnection is initiated at electron scales in a plasma. Surrounding the electron diffusion region, there is an Ion-Decoupling Region (IDR) of the size of the ion length scales (inertial length and gyroradius). Reconnection at the Earths magnetopause often includes cold magnetospheric (few tens of eV), hot magnetospheric (10 keV), and magnetosheath (1 keV) ions, with different gyroradius length scales. We report observations of a subregion inside the IDR of the size of the cold ion population gyroradius (approx. 15 km) where the cold ions are demagnetized and accelerated parallel to the Hall electric field. Outside the subregion, cold ions follow the E x B motion together with electrons, while hot ions are demagnetized. We observe a sharp cold ion density gradient separating the two regions, which we identify as the cold and hot IDRs. |
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ISSN: | 0094-8276 1944-8007 1944-8007 |
DOI: | 10.1002/2016GL069877 |