Signal Processing for the Measurement of the Deuterium/Hydrogen Ratio in the Local Interstellar Medium

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dc.contributor.authorRodríguez Moreno, Diego Francisco
dc.contributor.authorWurz, Peter
dc.contributor.authorSaul, Lukas
dc.contributor.authorBzowski, Maciej
dc.contributor.authorKubiak, Marzena Aleksanda
dc.contributor.authorSokół, Justyna Maria
dc.contributor.authorFrisch, Priscilla
dc.contributor.authorFuselier, Stephen Anthony
dc.contributor.authorMcComas, David John
dc.contributor.authorMöbius, Eberhard
dc.contributor.authorSchwadron, Nathan
dc.date.accessioned2021-04-19T14:55:36Z
dc.date.available2021-04-19T14:55:36Z
dc.date.issued2014-02-24
dc.date.updated2021-04-19T14:55:36Z
dc.description.abstractWe report on a comprehensive signal processing procedure for very low signal levels for the measurement of neutral deuterium in the local interstellar medium from a spacecraft in Earth orbit. The deuterium measurements were performed with the IBEX-Lo camera on NASA's Interstellar Boundary Explorer (IBEX) satellite. Our analysis technique for these data consists of creating a mass relation in three-dimensional time of flight space to accurately determine the position of the predicted D events, to precisely model the tail of the H events in the region where the H tail events are near the expected D events, and then to separate the H tail from the observations to extract the very faint D signal. This interstellar D signal, which is expected to be a few counts per year, is extracted from a strong terrestrial background signal, consisting of sputter products from the sensor's conversion surface. As reference we accurately measure the terrestrial D/H ratio in these sputtered products and then discriminate this terrestrial background source. During the three years of the mission time when the deuterium signal was visible to IBEX, the observation geometry and orbit allowed for a total observation time of 115.3 days. Because of the spinning of the spacecraft and the stepping through eight energy channels the actual observing time of the interstellar wind was only 1.44 days. With the optimised data analysis we found three counts that could be attributed to interstellar deuterium. These results update our earlier work.
dc.description.departmentPhysics and Astronomy
dc.identifierdoi: 10.3390/e16021134
dc.identifier.citationEntropy 16 (2): 1134-1168 (2014)
dc.identifier.urihttps://hdl.handle.net/20.500.12588/333
dc.rightsAttribution 4.0 United States
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subjectenergetic neutral atoms
dc.subjectdeuterium
dc.subjectD/H ratio
dc.subjectISM
dc.subject3D-TOF analysis
dc.subjectIBEX-Lo
dc.titleSignal Processing for the Measurement of the Deuterium/Hydrogen Ratio in the Local Interstellar Medium
dc.typeArticle

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