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The Structure of the Global Heliosphere as Seen by In-Situ Ions from the Voyagers and Remotely Sensed ENAs from Cassini

MPG-Autoren
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Hilchenbach,  Martin
Planetary Science Department, Max Planck Institute for Solar System Research, Max Planck Society;

Externe Ressourcen

https://ui.adsabs.harvard.edu/abs/2022SSRv..218...21D
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Zitation

Dialynas, K., Krimigis, S. M., Decker, R. B., Hill, M., Mitchell, D. G., Hsieh, K. C., et al. (2022). The Structure of the Global Heliosphere as Seen by In-Situ Ions from the Voyagers and Remotely Sensed ENAs from Cassini. Space Science Reviews, 218, 21. doi:10.1007/s11214-022-00889-0.


Zitierlink: https://hdl.handle.net/21.11116/0000-000D-B710-2
Zusammenfassung
The exploration of interplanetary space and our solar bubble, the heliosphere, has made a big leap over the past two decades, due to the path-breaking observations of the two Voyager spacecraft, launched more than 44 years ago. Their in-situ particle and fields measurements were complemented by remote observations of 5.2 to 55 keV Energetic Neutral Atoms (ENA) from the Cassini mission (Ion and Neutral Camera-INCA), revealing a number of previously unanticipated heliospheric structures such as the "Belt", a region of enhanced particle pressure inside the heliosheath. The Suprathermal Time Of Flight (HSTOF) instrument on the Solar and Heliospheric Observatory (SOHO) also provided information of 58-88 keV ENAs from the heliosphere. In this chapter we provide a brief discussion for the contribution of the Voyager 1 and 2 Low Energy Charged Particle (LECP) observations that provided "ground truth" to the ENA images from Cassini/INCA towards addressing fundamental questions for the heliosphere's interaction with the Very Local Interstellar Medium.