Measuring Neutral Hydrogen Properties in the Interplanetary Medium
Résumé
This supports development and deployment-to-space of a high-resolution spectrograph to distinguish different populations of H atoms that directly interact at the interface of the heliosheath, the region where the solar wind is subsonic. Resulting science would support Voyagers, IBEX, IMAP, New Horizons, and Interstellar Probe mission observations, and improve characterization of the solar wind.
Domaines
Planète et Univers [physics]Origine | Fichiers produits par l'(les) auteur(s) |
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