Computation of Emergent Intensities of ENAs and Ions From Low Altitude Emission

Physics

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2716 Energetic Particles: Precipitating, 2730 Magnetosphere: Inner, 7837 Neutral Particles (2151)

Scientific paper

The energetic neutral atom (ENA) cameras on the TWINS spacecraft have been observing low-altitude emission (LAE) from the auroral regions during recent weak geomagnetic activitiy [ Bazell et al.; McComas et al., this Special Session]. When the observing viewpoint is favorable, LAE can be the brightest ENA emission in the TWINS images, even during large geomagnetic storms. The production of LAE is a "thick- target" process involving many collisions at altitudes <500km with monatomic oxygen (O): charge exchange of H+, stripping of neutral H, as well as energy losses due to ionization and excitation of the O when the energetic hydrogen is in either its charged (H+) or neutral (H) state. The theory of LAE therefore requires two coupled transport equations for the ion and ENA intensities. These have been developed in the extreme forward-scattering approximation. Pitch-angle changes in the Earth's magnetic field are also included, because they profoundly influence the emerging intensities of both ENAs and ions. Analytic solutions for these intensities have been obtained [ Roelof, this Special Session] that are expressed in two "eigen-functions" that are linear combinations of the ENA and ion intensities. They are functions of a "helical column density" that is accumulated by a gyrating particle during its downward path to its mirror point and then upward until its emergence as either an ENA or an ion. The solution also includes the history of the particle's energy, which constantly decreases during its trajectory due to the energy loss in every kind of atomic collision. The emergent spectra are highly directional (both with respect to the zenith and the local magnetic field vector), and they depend upon the shape of the precipitating ion spectrum. Numerical examples from the analytic solutions are presented for these functions and the emergent intensities of both ENA emission and energetic ion albedo.

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