Abstract
AbstractAt 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.
Publisher
Cambridge University Press (CUP)
Subject
Astronomy and Astrophysics,Space and Planetary Science
Cited by
2 articles.
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1. Solar radio emission surveillance by the Trieste Solar Radio System 2.0;2020 XXXIIIrd General Assembly and Scientific Symposium of the International Union of Radio Science;2020-08
2. Radio Observations for Space Weather;2019 URSI Asia-Pacific Radio Science Conference (AP-RASC);2019-03