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Defining and Characterising Heliospheric Weather and Climate

Published online by Cambridge University Press:  24 July 2018

Mauro Messerotti Open the ORCID record for Mauro Messerotti [Opens in a new window]
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.

Keywords

Solar-terrestrial relationssolar system: generalGalaxy: generalgalaxies: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S335: Space Weather of the Heliosphere: Processes and Forecasts , July 2017 , pp. 226 - 231
Copyright
Copyright © International Astronomical Union 2018 

References

Lilensten, J., Sanahuja, B. & Messerotti, M. 2008, in: Lilensten, J., Belehaki, A., Messerotti, M., Vainio, R., Watermann, J. & Poedts, S. (eds.), Developing the scientific basis for monitoring, modelling and predicting Space Weather, COST 724 Final Report (Luxembourg: Office for the Official Publications of the European Communities), p. 298Google Scholar
Messerotti, M. 2002, in: Sawaya-Lacoste, H. (ed.), Proc. Second Solar Cycle and Space Weather Euroconference (Noordwijk: ESA Publications Division), p. 607Google Scholar
Messerotti, M. 2007, in: Lundstedt, H. (ed.), Solar Activity: Exploration, Understanding and Prediction, Proc. Lund Workshop (Noordwijk: ESA Publications Division), p. 11Google Scholar
Messerotti, M. 2008, in: Lilensten, J., Belehaki, A., Messerotti, M., Vainio, R., Watermann, J. & Poedts, S. (eds.), Developing the scientific basis for monitoring, modelling and predicting Space Weather, COST 724 Final Report (Luxembourg: Office for the Official Publications of the European Communities), p. 350Google Scholar
Messerotti, M., Zuccarello, F. & Lundstedt, H. 2008, in: Lilensten, J., Belehaki, A., Messerotti, M., Vainio, R., Watermann, J. & Poedts, S. (eds.), Developing the scientific basis for monitoring, modelling and predicting Space Weather, COST 724 Final Report (Luxembourg: Office for the Official Publications of the European Communities), p. 20Google Scholar
Messerotti, M., Zuccarello, F., Guglielmino, S., Bothmer, V., Lilensten, J., Noci, G., Storini, M. & Lundstedt, H. 2009, Space Sci. Revs, 147, 3–4, 121CrossRefGoogle Scholar
Messerotti, M. 2011, in: Miralles, M. P. & Almeida, J. Sánchez (eds.), The Sun, the Solar Wind and the Heliosphere, Proc. Sopron IAGA Conference (Berlin: Springer), p. 209CrossRefGoogle Scholar