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Defining and Characterising Heliospheric Weather and Climate

Published online by Cambridge University Press:  24 July 2018

Mauro Messerotti*
Affiliation:
INAF-Astronomical Observatory of Trieste, Loc. Basovizza 302, 34149, Trieste, Italy email: [email protected] Dept. of Physics, Trieste University, Via A. Valerio 2, 34127 Trieste, Italy email: [email protected]
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Abstract

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At large distance scales, space exploration in the last decades has significantly helped in better locating the boundaries of the Heliosphere and outlining its shape as well as in probing the various plasma domains that separate the inner heliospheric region from the interstellar one. At shorter distance scales, a fleet of spacecraft has been probing the outer and inner Solar System plasma with a high level of detail.

This monitoring, complemented by space- and ground-based observations of processes relevant to the Heliosphere, has pointed out a series both of intrinsic and extrinsic perturbations that characterise the physical state of heliospheric plasmas both at small and large spatial scales and on short and long temporal scales.

By means of concept maps that schematise the association among concepts, in this work we will present a new domain ontology for the definition and characterisation of Heliospheric Weather and Climate.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

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