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Solar particle radiation storms fore...

Crosby, Norma B.

Solar particle radiation storms forecasting and analysisthe HESPERIA HORIZON 2020 Project and beyond /

Record Type:	Electronic resources : Monograph/item
Title/Author:	Solar particle radiation storms forecasting and analysisedited by Olga E. Malandraki, Norma B. Crosby.
Reminder of title:	the HESPERIA HORIZON 2020 Project and beyond /
other author:	Malandraki, Olga E.
Published:	Cham :Springer International Publishing :2018.
Description:	xiii, 203 p. :ill. (some col.), digital ;24 cm.
Contained By:	Springer eBooks
Subject:	Solar energetic particles.
Online resource:	http://dx.doi.org/10.1007/978-3-319-60051-2
ISBN:	9783319600512$q(electronic bk.)

Solar particle radiation storms forecasting and analysisthe HESPERIA HORIZON 2020 Project and beyond /
Solar particle radiation storms forecasting and analysisthe HESPERIA HORIZON 2020 Project and beyond /[electronic resource] :edited by Olga E. Malandraki, Norma B. Crosby. - Cham :Springer International Publishing :2018. - xiii, 203 p. :ill. (some col.), digital ;24 cm. - Astrophysics and space science library,0067-0057. - Astrophysics and space science library..

Open access.

Solar energetic particles (SEPs) emitted from the Sun are a major space weather hazard motivating the development of predictive capabilities. This book presents the results and findings of the HESPERIA (High Energy Solar Particle Events forecasting and Analysis) project of the EU HORIZON 2020 programme. It discusses the forecasting operational tools developed within the project, and presents progress to SEP research contributed by HESPERIA both from the observational as well as the SEP modelling perspective. Using multi-frequency observational data and simulations HESPERIA investigated the chain of processes from particle acceleration in the corona, particle transport in the magnetically complex corona and interplanetary space, to the detection near 1 AU. The book also elaborates on the unique software that has been constructed for inverting observations of relativistic SEPs to physical parameters that can be compared with spac e-borne measurements at lower energies. Introductory and pedagogical material included in the book make it accessible to students at graduate level and will be useful as background material for Space Physics and Space Weather courses with emphasis on Solar Energetic Particle Event Forecasting and Analysis. This book is published with open access under a CC BY 4.0 license.

ISBN: 9783319600512$q(electronic bk.)

Standard No.: 10.1007/978-3-319-60051-2doiSubjects--Topical Terms:

776214
Solar energetic particles.

LC Class. No.: QB526.S65

Dewey Class. No.: 539.7223

Solar particle radiation storms forecasting and analysisthe HESPERIA HORIZON 2020 Project and beyond /
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520 $a Solar energetic particles (SEPs) emitted from the Sun are a major space weather hazard motivating the development of predictive capabilities. This book presents the results and findings of the HESPERIA (High Energy Solar Particle Events forecasting and Analysis) project of the EU HORIZON 2020 programme. It discusses the forecasting operational tools developed within the project, and presents progress to SEP research contributed by HESPERIA both from the observational as well as the SEP modelling perspective. Using multi-frequency observational data and simulations HESPERIA investigated the chain of processes from particle acceleration in the corona, particle transport in the magnetically complex corona and interplanetary space, to the detection near 1 AU. The book also elaborates on the unique software that has been constructed for inverting observations of relativistic SEPs to physical parameters that can be compared with spac e-borne measurements at lower energies. Introductory and pedagogical material included in the book make it accessible to students at graduate level and will be useful as background material for Space Physics and Space Weather courses with emphasis on Solar Energetic Particle Event Forecasting and Analysis. This book is published with open access under a CC BY 4.0 license.
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