SM41C-2490
Reconstructing Ion Spectra from Low-Altitude ENAs: Moderate to Large Storms.
Thursday, 17 December 2015
Poster Hall (Moscone South)
Kristie LLera1,2, Jerry Goldstein3, David J McComas3 and Philip W Valek4, (1)University of Texas at San Antonio, Department of Physics & Astronomy, San Antonio, TX, United States, (2)Southwest Research Institute San Antonio, San Antonio, TX, United States, (3)Southwest Research Institute, San Antonio, TX, United States, (4)Southwest Research Inst, San Antonio, TX, United States
Abstract:
Two Wide-angle Imaging Neutral-atom Spectrometers (TWINS) Energetic neutral atom (ENA) imagers regularly observe Low-altitude Emission (LAE) intensifications during geomagnetic storm intervals. Since LAEs are produced by the interaction between ions and the near-Earth exosphere (altitudes ~200-800 km), they are a global signature of how the ring current decays in response to solar wind conditions. In this “optically thick” region, an ENA readily becomes reionized, and an ion is readily neutralized. Therefore, emerging ENAs that contribute to the LAE signal (detectable several RE away) have undergone multiple charge exchange and electron stripping interactions. Accounting for the ~36 eV energy loss per interaction, we developed a model to quantify the total energy lost by emergent LAEs. The analytical tool is applied to an ensemble of moderate to large storms (including the recent 17 March and 23 June storms in 2015) to reconstruct the parent ion spectra from TWINS ENA images. We examine the ion spectra energy characteristics among the various storm events.
