Abstract
The International Solar Polar Mission (ISPM) will, for the first time, allow exploration of the heliosphere within a few astronomical units of the Sun over the full range of heliographic latitudes. The prime mission objective is to study, as a function of solar latitude, the properties of the interplanetary medium and solar corona. The scientific instrumentation is designed to explore, in the third heliospheric dimension, the properties of the solar wind, the Sun/wind interface, the heliospheric magnetic field, solar radio bursts and plasma waves, solar X-rays, solar and galactic cosmic rays, and interplanetary/interstellar neutral gas and dust. ISPM will also detect cosmic gamma-ray bursts and search for gravitational waves.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
Editor information
Rights and permissions
Copyright information
© 1984 Springer-Verlag Berlin Heidelberg
About this chapter
Cite this chapter
Böhme, S. et al. (1984). Space Research. In: Böhme, S., et al. Astronomy and Astrophysics Abstracts. Astronomy and Astrophysics Abstracts, vol 34. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-12340-9_8
Download citation
DOI: https://doi.org/10.1007/978-3-662-12340-9_8
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-662-12342-3
Online ISBN: 978-3-662-12340-9
eBook Packages: Springer Book Archive