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Detailed Reference Information |
Sandel, B.R., King, R.A., Forrester, W.T., Gallagher, D.L., Broadfoot, A.L. and Curtis, C.C. (2001). Initial results from the IMAGE Extreme Ultraviolet Imager. Geophysical Research Letters 28: doi: 10.1029/2001GL012885. issn: 0094-8276. |
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The Extreme Ultraviolet Imager (EUV) of the IMAGE mission is providing the first global images of the He+ distribution in Earth's plasmasphere. The EUV instrument images the He+ resonance line emission at 30.4 nm at a time resolution of 10 minutes and a spatial resolution of 0.1 RE. Each image encompasses the entire plasmasphere in a single frame, to permit study of the structure and dynamics of the plasmasphere in its entirety. Here we survey several of the most striking features of the plasmasphere as seen by EUV. These features include convection tails, depleted regions that we call voids, isolated magnetic flux tubes filled to higher He+ density than their neighbors, and shoulders in the He+ distribution. ¿ 2001 American Geophysical Union |
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Abstract |
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Keywords
Magnetospheric Physics, Magnetosphere—inner, Magnetospheric Physics, Plasma convection, Magnetospheric Physics, Plasmasphere, Magnetospheric Physics, Storms and substorms |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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