Science opportunities for IMAP-Lo observations of ISN He, Ne and O

Direct-sampling observations of interstellar neutral (ISN) species and their secondary populations inform on the physical state of the local interstellar medium and processes operating in the outer heliosheath. Such observations are performed from Earth's orbit by the IBEX-Lo experiment on board the Interstellar Boundary Explorer (IBEX) mission. IBEX ISN viewing is restricted to directions close to perpendicular to the Earth-Sun line, which limits the observations of interstellar species to several months during the year. A greatly improved data set will be possible for the upcoming IMAP mission due to a novel concept of putting the IMAP-Lo detector on a pivot platform that varies the angle of observation relative to the Sun-Earth line and the detector boresight, as planned for the IMAP-Lo instrument on the Interstellar Mapping and Acceleration Probe (IMAP) mission (McComas et al. 2018). Here we suggest a 2 year scenario for varying the viewing angle in such a way that all the necessary atom components can be observed sufficiently well to achieve the science goals of nominal IMAP mission. This scenario facilitates, among others, removal of the correlation of the inflow parameters of interstellar gas, unambiguous analysis of the primary and secondary populations of interstellar He, Ne and O, and determination of the ionization rates of He and Ne free of possible calibration bias. The scheme is operationally simple, provides a good counting statistics, and synergizes observations of interstellar species and heliospheric energetic neutral atoms.