LENA Movies

(Click on the images to start the movies)

Single Image from Movie
This LENA movie shows that there was a localized response in the ionosphere due to the compression of the magnetosphere by a CME shock front. The ionosphere is disturbed over a considerable range of latitude but a relatively small range of local time. LENA neutral atom observations show a dramatic increase in the oxygen count rate from the general direction of the Earth. The increase occurs about 38 minutes after the disturbance, at 0951, consistent with the travel time of 30 eV neutral oxygen from the ionosphere to the spacecraft. This suggests that there is no time delay between the ionospheric disturbance and the initiation of ion outflow from the ionosphere. See Fuselier et al., Ion outflow observed by IMAGE: Implications for source regions and heating mechanisms, Geophysical Research Letters, 28, 1163-1166, 2001 for further information.


Single Image from Movie Neutrals created by charge-exchange of low energy ion outflow from the ionosphere are imaged by the Low Energy Neutral Atom (LENA) imager on the IMAGE spacecraft. This movie shows that enhanced neutral fluxes are associated with changes in the solar wind during an ion outflow event on June 24, 2000 and indicate that changes in solar wind density are associated with episodic bursts of ion outflow. See Moore et al., Low energy neutral atoms in the magnetosphere, Geophysical Research Letters, 28, 1143-1146, 2001 for more information.



Single Image from Movie One of the first discoveries LENA made was that there are neutral atoms in the solar wind flow. One way LENA sees these are as flux increases from the direction of the Sun when the solar wind flux increases and one reason is enhanced solar wind charge exchange with the Earth's geocorona, the neutral atoms surrounding the Earth. This movie shows a simulation of the expected neutral hydrogen flux observed at LENA due to the solar wind interaction with the Earth's atmosphere on March 31, 2001. The simulation uses results from the BATSRUS global MHD code developed at the University of Michigan and run by the Community Coordinated Modelling Center at NASA's Goddard Space Flight Center. The simulation spectrogram compares favorably with the LENA data on this day. See Collier et al., Observations of neutral atoms from the solar wind, Journal of Geophysical Research, 106, 24,893-24,906, 2001 for more information.



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Responsible NASA Representative: Dr. Thomas E. Moore
Email: Thomas.E.Moore@gsfc.nasa.gov


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Last Modified: December 6, 2001