Solar Particle Radiation Storms Forecasting and Analysis : : The HESPERIA HORIZON 2020 Project and Beyond.
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Superior document: | Astrophysics and Space Science Library ; v.444 |
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Place / Publishing House: | Cham : : Springer International Publishing AG,, 2018. ©2018. |
Year of Publication: | 2018 |
Edition: | 1st ed. |
Language: | English |
Series: | Astrophysics and Space Science Library
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Physical Description: | 1 online resource (210 pages) |
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Malandraki, Olga E. Solar Particle Radiation Storms Forecasting and Analysis : The HESPERIA HORIZON 2020 Project and Beyond. 1st ed. Cham : Springer International Publishing AG, 2018. ©2018. 1 online resource (210 pages) text txt rdacontent computer c rdamedia online resource cr rdacarrier Astrophysics and Space Science Library ; v.444 Intro -- Preface -- Acknowledgements -- Contents -- List of Abbreviations -- 1 Solar Energetic Particles and Space Weather: Science and Applications -- 1.1 Science -- 1.1.1 Historical Perspective of Solar Energetic Particle (SEP) Events -- 1.1.2 Large Gradual SEP Events -- 1.1.3 Ground Level Enhancement (GLE) Events -- 1.1.4 Multi-Spacecraft Observations of SEP Events -- 1.1.5 Particle Acceleration -- 1.1.6 Key Open Questions and Future Missions -- 1.2 Applications -- 1.2.1 Why Study SEP Events? -- 1.2.2 SEP Effects on Technology -- 1.2.3 SEPs and Human Health Effects -- 1.2.4 Mitigating the Effects of SEPs -- 1.2.4.1 Hazard Assessment -- 1.2.4.2 Mitigation Procedures -- References -- 2 Eruptive Activity Related to Solar Energetic Particle Events -- 2.1 Introduction -- 2.2 The Scene -- 2.3 Solar Flares: Energy Release and Radiative Signatures of Charged Particle Acceleration -- 2.3.1 Emission Processes -- 2.3.1.1 Bremsstrahlung -- 2.3.1.2 Gyrosynchrotron Radiation -- 2.3.1.3 Plasma Emission from Electron Beams -- 2.3.1.4 Gamma-Rays from Accelerated Protons and Ions -- 2.3.2 Where Are Electrons Accelerated in Solar Flares? -- 2.3.3 A Qualitative View of Acceleration Processes -- 2.4 What Is a Coronal Mass Ejection? -- 2.4.1 CME Magnetic Structure and Eruption -- 2.4.2 Shock Waves and Particle Acceleration at CMEs -- 2.5 Summary and Conclusion -- References -- 3 Particle Acceleration Mechanisms -- 3.1 Introduction -- 3.2 Acceleration Mechanisms -- 3.2.1 Large-Scale Electric Field Acceleration -- 3.2.2 Resonant Wave Acceleration -- 3.2.3 Shock Acceleration -- 3.2.4 Compressional Acceleration and Collapsing Magnetic Traps -- 3.2.5 Stochastic Acceleration -- 3.3 Concluding Remarks -- References -- 4 Charged Particle Transport in the Interplanetary Medium -- 4.1 Introduction -- 4.1.1 Energetic Particles in the Solar System. 4.1.2 The Interplanetary Magnetic Field -- 4.1.3 Motion of Charged Particles. First Adiabatic Invariant -- 4.2 Particle Transport -- 4.2.1 Particle Transport Equations -- 4.2.2 Focused Transport -- 4.2.3 Diffusive Transport -- 4.3 Application: Description of Solar Energetic Particle Events -- 4.3.1 Numerical Techniques -- 4.3.2 Observations -- 4.3.3 Inferring Transport Conditions -- 4.4 Concluding Remarks -- References -- 5 Cosmic Ray Particle Transport in the Earth's Magnetosphere -- 5.1 Introduction -- 5.2 Motion of Charged Particles in a Magnetic Field: Lorentz Force -- 5.3 Earth's Magnetic Field -- 5.3.1 The Magnetic Field of the Earth as a Dipole Field -- 5.3.2 Magnetic Field Model Due to Internal Sources: IGRF -- 5.3.3 Contributions to the Earth's Magnetic Field by Magnetospheric Electric Currents -- 5.3.4 Magnetic Field Models of the External Sources -- 5.4 Computation of the Propagation of Cosmic Ray Particles in the Earth's Magnetosphere -- 5.5 The Concept of Cutoff Rigidities and Asymptotic Directions -- References -- 6 Ground-Based Measurements of Energetic Particles by Neutron Monitors -- 6.1 Introduction -- 6.2 History -- 6.3 Transport of Cosmic Ray Particles in the Earth's Atmosphere -- 6.3.1 Model of the Earth's Atmosphere -- 6.3.2 Particle Cascade in the Atmosphere -- 6.4 Neutron Monitor Detector -- 6.4.1 Components of a Neutron Monitor -- 6.4.2 Neutron Monitor Yield Function -- 6.4.3 Atmospheric Effects -- 6.5 Worldwide Network of Neutron Monitor Stations as a Giant Spectrometer -- 6.6 Neutron Monitor Database: NMDB -- References -- 7 HESPERIA Forecasting Tools: Real-Time and Post-Event -- 7.1 Introduction -- 7.2 Predicting SEP Event Onsets from Historical Microwave Data by Using the UMASEP Scheme -- 7.3 Predicting SEP Energy Spectra from Historical Microwave Data -- 7.4 Predicting 30-50 MeV SEP Events by Using the RELeASE Scheme. 7.5 Predicting > -- 500 MeV SEP Events by Using the UMASEP Scheme -- 7.6 Concluding Remarks -- References -- 8 X-Ray, Radio and SEP Observations of Relativistic Gamma-Ray Events -- 8.1 Introduction -- 8.2 Theory and Early Observations of Gamma-Ray Emission at Photon Energies > -- 60MeV -- 8.2.1 Pion-Decay γ-Ray Emission -- 8.2.2 Long-Duration γ-Ray Events -- 8.3 New Insights of Sustained Emission Events from Fermi Observations -- 8.4 Multiwavelength Observations of Fermi/LAT γ-Ray Events -- 8.4.1 Impulsive and Early Post-impulsive γ-Ray Emission -- 8.4.2 Long-Duration γ-Ray Events -- 8.4.3 Soft X-Ray Bursts and γ-Ray Events -- 8.4.4 Coronal Shock Waves and γ-Ray Events -- 8.5 Solar Energetic Particle Events Associated with Fermi/LAT Gamma-Ray Events -- 8.5.1 SEP Characteristics and Association with Fermi/LAT -- 8.5.2 SEP Spectra -- 8.6 Summary and Discussion -- References -- 9 Modelling of Shock-Accelerated Gamma-Ray Events -- 9.1 Introduction -- 9.2 Model Description -- 9.2.1 Shock and Particle Model -- 9.2.2 Coronal Shock Acceleration Model -- 9.2.3 DownStream Propagation Model -- 9.3 Results -- 9.3.1 2012 May 17 Event -- 9.3.1.1 Modelling of the SEP Event -- 9.3.1.2 Simulations of Proton Acceleration at the Shock -- 9.3.1.3 Modelling of the Proton Transport Back to the Sun -- 9.3.2 2012 January 23 Event -- 9.3.2.1 Modelling of the SEP Event -- 9.3.2.2 Simulation of Proton Acceleration at the Shock -- 9.3.2.3 Modelling of the Proton Transport Back to the Sun -- 9.4 Discussion and Conclusions -- References -- 10 Inversion Methodology of Ground Level Enhancements -- 10.1 Introduction -- 10.2 Space and Ground Based Measurements of GLEs -- 10.2.1 dE/dx-dE/dx-Method -- 10.2.2 dE/dx - C -- 10.2.3 Magnet Spectrometer -- 10.3 Forward Modeling from the Sun to the Observer at Ground. 10.3.1 Interplanetary Particle Transport: From the Sun to the Magnetosphere -- 10.3.2 From the Interplanetary Particle Distribution to Neutron Monitor Measurements - Magneto- and Atmospheric Transport of Charged Energetic Particles -- 10.3.3 Combined Greens-Function -- 10.4 Inversion Methodology -- 10.4.1 Inversion of Spacecraft Data to the Sun -- 10.4.2 Inversion of NM Data to the Border of the Earth's Magnetosphere -- 10.4.3 The HESPERIA Approach -- 10.5 Results and Validation -- 10.6 Concluding Remarks -- References -- Index. Description based on publisher supplied metadata and other sources. Electronic reproduction. Ann Arbor, Michigan : ProQuest Ebook Central, 2024. Available via World Wide Web. Access may be limited to ProQuest Ebook Central affiliated libraries. Electronic books. Crosby, Norma B. Print version: Malandraki, Olga E. Solar Particle Radiation Storms Forecasting and Analysis Cham : Springer International Publishing AG,c2018 9783319600505 ProQuest (Firm) Astrophysics and Space Science Library https://ebookcentral.proquest.com/lib/oeawat/detail.action?docID=5591474 Click to View |
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Malandraki, Olga E. |
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Malandraki, Olga E. Solar Particle Radiation Storms Forecasting and Analysis : The HESPERIA HORIZON 2020 Project and Beyond. Astrophysics and Space Science Library ; Intro -- Preface -- Acknowledgements -- Contents -- List of Abbreviations -- 1 Solar Energetic Particles and Space Weather: Science and Applications -- 1.1 Science -- 1.1.1 Historical Perspective of Solar Energetic Particle (SEP) Events -- 1.1.2 Large Gradual SEP Events -- 1.1.3 Ground Level Enhancement (GLE) Events -- 1.1.4 Multi-Spacecraft Observations of SEP Events -- 1.1.5 Particle Acceleration -- 1.1.6 Key Open Questions and Future Missions -- 1.2 Applications -- 1.2.1 Why Study SEP Events? -- 1.2.2 SEP Effects on Technology -- 1.2.3 SEPs and Human Health Effects -- 1.2.4 Mitigating the Effects of SEPs -- 1.2.4.1 Hazard Assessment -- 1.2.4.2 Mitigation Procedures -- References -- 2 Eruptive Activity Related to Solar Energetic Particle Events -- 2.1 Introduction -- 2.2 The Scene -- 2.3 Solar Flares: Energy Release and Radiative Signatures of Charged Particle Acceleration -- 2.3.1 Emission Processes -- 2.3.1.1 Bremsstrahlung -- 2.3.1.2 Gyrosynchrotron Radiation -- 2.3.1.3 Plasma Emission from Electron Beams -- 2.3.1.4 Gamma-Rays from Accelerated Protons and Ions -- 2.3.2 Where Are Electrons Accelerated in Solar Flares? -- 2.3.3 A Qualitative View of Acceleration Processes -- 2.4 What Is a Coronal Mass Ejection? -- 2.4.1 CME Magnetic Structure and Eruption -- 2.4.2 Shock Waves and Particle Acceleration at CMEs -- 2.5 Summary and Conclusion -- References -- 3 Particle Acceleration Mechanisms -- 3.1 Introduction -- 3.2 Acceleration Mechanisms -- 3.2.1 Large-Scale Electric Field Acceleration -- 3.2.2 Resonant Wave Acceleration -- 3.2.3 Shock Acceleration -- 3.2.4 Compressional Acceleration and Collapsing Magnetic Traps -- 3.2.5 Stochastic Acceleration -- 3.3 Concluding Remarks -- References -- 4 Charged Particle Transport in the Interplanetary Medium -- 4.1 Introduction -- 4.1.1 Energetic Particles in the Solar System. 4.1.2 The Interplanetary Magnetic Field -- 4.1.3 Motion of Charged Particles. First Adiabatic Invariant -- 4.2 Particle Transport -- 4.2.1 Particle Transport Equations -- 4.2.2 Focused Transport -- 4.2.3 Diffusive Transport -- 4.3 Application: Description of Solar Energetic Particle Events -- 4.3.1 Numerical Techniques -- 4.3.2 Observations -- 4.3.3 Inferring Transport Conditions -- 4.4 Concluding Remarks -- References -- 5 Cosmic Ray Particle Transport in the Earth's Magnetosphere -- 5.1 Introduction -- 5.2 Motion of Charged Particles in a Magnetic Field: Lorentz Force -- 5.3 Earth's Magnetic Field -- 5.3.1 The Magnetic Field of the Earth as a Dipole Field -- 5.3.2 Magnetic Field Model Due to Internal Sources: IGRF -- 5.3.3 Contributions to the Earth's Magnetic Field by Magnetospheric Electric Currents -- 5.3.4 Magnetic Field Models of the External Sources -- 5.4 Computation of the Propagation of Cosmic Ray Particles in the Earth's Magnetosphere -- 5.5 The Concept of Cutoff Rigidities and Asymptotic Directions -- References -- 6 Ground-Based Measurements of Energetic Particles by Neutron Monitors -- 6.1 Introduction -- 6.2 History -- 6.3 Transport of Cosmic Ray Particles in the Earth's Atmosphere -- 6.3.1 Model of the Earth's Atmosphere -- 6.3.2 Particle Cascade in the Atmosphere -- 6.4 Neutron Monitor Detector -- 6.4.1 Components of a Neutron Monitor -- 6.4.2 Neutron Monitor Yield Function -- 6.4.3 Atmospheric Effects -- 6.5 Worldwide Network of Neutron Monitor Stations as a Giant Spectrometer -- 6.6 Neutron Monitor Database: NMDB -- References -- 7 HESPERIA Forecasting Tools: Real-Time and Post-Event -- 7.1 Introduction -- 7.2 Predicting SEP Event Onsets from Historical Microwave Data by Using the UMASEP Scheme -- 7.3 Predicting SEP Energy Spectra from Historical Microwave Data -- 7.4 Predicting 30-50 MeV SEP Events by Using the RELeASE Scheme. 7.5 Predicting > -- 500 MeV SEP Events by Using the UMASEP Scheme -- 7.6 Concluding Remarks -- References -- 8 X-Ray, Radio and SEP Observations of Relativistic Gamma-Ray Events -- 8.1 Introduction -- 8.2 Theory and Early Observations of Gamma-Ray Emission at Photon Energies > -- 60MeV -- 8.2.1 Pion-Decay γ-Ray Emission -- 8.2.2 Long-Duration γ-Ray Events -- 8.3 New Insights of Sustained Emission Events from Fermi Observations -- 8.4 Multiwavelength Observations of Fermi/LAT γ-Ray Events -- 8.4.1 Impulsive and Early Post-impulsive γ-Ray Emission -- 8.4.2 Long-Duration γ-Ray Events -- 8.4.3 Soft X-Ray Bursts and γ-Ray Events -- 8.4.4 Coronal Shock Waves and γ-Ray Events -- 8.5 Solar Energetic Particle Events Associated with Fermi/LAT Gamma-Ray Events -- 8.5.1 SEP Characteristics and Association with Fermi/LAT -- 8.5.2 SEP Spectra -- 8.6 Summary and Discussion -- References -- 9 Modelling of Shock-Accelerated Gamma-Ray Events -- 9.1 Introduction -- 9.2 Model Description -- 9.2.1 Shock and Particle Model -- 9.2.2 Coronal Shock Acceleration Model -- 9.2.3 DownStream Propagation Model -- 9.3 Results -- 9.3.1 2012 May 17 Event -- 9.3.1.1 Modelling of the SEP Event -- 9.3.1.2 Simulations of Proton Acceleration at the Shock -- 9.3.1.3 Modelling of the Proton Transport Back to the Sun -- 9.3.2 2012 January 23 Event -- 9.3.2.1 Modelling of the SEP Event -- 9.3.2.2 Simulation of Proton Acceleration at the Shock -- 9.3.2.3 Modelling of the Proton Transport Back to the Sun -- 9.4 Discussion and Conclusions -- References -- 10 Inversion Methodology of Ground Level Enhancements -- 10.1 Introduction -- 10.2 Space and Ground Based Measurements of GLEs -- 10.2.1 dE/dx-dE/dx-Method -- 10.2.2 dE/dx - C -- 10.2.3 Magnet Spectrometer -- 10.3 Forward Modeling from the Sun to the Observer at Ground. 10.3.1 Interplanetary Particle Transport: From the Sun to the Magnetosphere -- 10.3.2 From the Interplanetary Particle Distribution to Neutron Monitor Measurements - Magneto- and Atmospheric Transport of Charged Energetic Particles -- 10.3.3 Combined Greens-Function -- 10.4 Inversion Methodology -- 10.4.1 Inversion of Spacecraft Data to the Sun -- 10.4.2 Inversion of NM Data to the Border of the Earth's Magnetosphere -- 10.4.3 The HESPERIA Approach -- 10.5 Results and Validation -- 10.6 Concluding Remarks -- References -- Index. |
author_facet |
Malandraki, Olga E. Crosby, Norma B. |
author_variant |
o e m oe oem |
author2 |
Crosby, Norma B. |
author2_variant |
n b c nb nbc |
author2_role |
TeilnehmendeR |
author_sort |
Malandraki, Olga E. |
title |
Solar Particle Radiation Storms Forecasting and Analysis : The HESPERIA HORIZON 2020 Project and Beyond. |
title_sub |
The HESPERIA HORIZON 2020 Project and Beyond. |
title_full |
Solar Particle Radiation Storms Forecasting and Analysis : The HESPERIA HORIZON 2020 Project and Beyond. |
title_fullStr |
Solar Particle Radiation Storms Forecasting and Analysis : The HESPERIA HORIZON 2020 Project and Beyond. |
title_full_unstemmed |
Solar Particle Radiation Storms Forecasting and Analysis : The HESPERIA HORIZON 2020 Project and Beyond. |
title_auth |
Solar Particle Radiation Storms Forecasting and Analysis : The HESPERIA HORIZON 2020 Project and Beyond. |
title_new |
Solar Particle Radiation Storms Forecasting and Analysis : |
title_sort |
solar particle radiation storms forecasting and analysis : the hesperia horizon 2020 project and beyond. |
series |
Astrophysics and Space Science Library ; |
series2 |
Astrophysics and Space Science Library ; |
publisher |
Springer International Publishing AG, |
publishDate |
2018 |
physical |
1 online resource (210 pages) |
edition |
1st ed. |
contents |
Intro -- Preface -- Acknowledgements -- Contents -- List of Abbreviations -- 1 Solar Energetic Particles and Space Weather: Science and Applications -- 1.1 Science -- 1.1.1 Historical Perspective of Solar Energetic Particle (SEP) Events -- 1.1.2 Large Gradual SEP Events -- 1.1.3 Ground Level Enhancement (GLE) Events -- 1.1.4 Multi-Spacecraft Observations of SEP Events -- 1.1.5 Particle Acceleration -- 1.1.6 Key Open Questions and Future Missions -- 1.2 Applications -- 1.2.1 Why Study SEP Events? -- 1.2.2 SEP Effects on Technology -- 1.2.3 SEPs and Human Health Effects -- 1.2.4 Mitigating the Effects of SEPs -- 1.2.4.1 Hazard Assessment -- 1.2.4.2 Mitigation Procedures -- References -- 2 Eruptive Activity Related to Solar Energetic Particle Events -- 2.1 Introduction -- 2.2 The Scene -- 2.3 Solar Flares: Energy Release and Radiative Signatures of Charged Particle Acceleration -- 2.3.1 Emission Processes -- 2.3.1.1 Bremsstrahlung -- 2.3.1.2 Gyrosynchrotron Radiation -- 2.3.1.3 Plasma Emission from Electron Beams -- 2.3.1.4 Gamma-Rays from Accelerated Protons and Ions -- 2.3.2 Where Are Electrons Accelerated in Solar Flares? -- 2.3.3 A Qualitative View of Acceleration Processes -- 2.4 What Is a Coronal Mass Ejection? -- 2.4.1 CME Magnetic Structure and Eruption -- 2.4.2 Shock Waves and Particle Acceleration at CMEs -- 2.5 Summary and Conclusion -- References -- 3 Particle Acceleration Mechanisms -- 3.1 Introduction -- 3.2 Acceleration Mechanisms -- 3.2.1 Large-Scale Electric Field Acceleration -- 3.2.2 Resonant Wave Acceleration -- 3.2.3 Shock Acceleration -- 3.2.4 Compressional Acceleration and Collapsing Magnetic Traps -- 3.2.5 Stochastic Acceleration -- 3.3 Concluding Remarks -- References -- 4 Charged Particle Transport in the Interplanetary Medium -- 4.1 Introduction -- 4.1.1 Energetic Particles in the Solar System. 4.1.2 The Interplanetary Magnetic Field -- 4.1.3 Motion of Charged Particles. First Adiabatic Invariant -- 4.2 Particle Transport -- 4.2.1 Particle Transport Equations -- 4.2.2 Focused Transport -- 4.2.3 Diffusive Transport -- 4.3 Application: Description of Solar Energetic Particle Events -- 4.3.1 Numerical Techniques -- 4.3.2 Observations -- 4.3.3 Inferring Transport Conditions -- 4.4 Concluding Remarks -- References -- 5 Cosmic Ray Particle Transport in the Earth's Magnetosphere -- 5.1 Introduction -- 5.2 Motion of Charged Particles in a Magnetic Field: Lorentz Force -- 5.3 Earth's Magnetic Field -- 5.3.1 The Magnetic Field of the Earth as a Dipole Field -- 5.3.2 Magnetic Field Model Due to Internal Sources: IGRF -- 5.3.3 Contributions to the Earth's Magnetic Field by Magnetospheric Electric Currents -- 5.3.4 Magnetic Field Models of the External Sources -- 5.4 Computation of the Propagation of Cosmic Ray Particles in the Earth's Magnetosphere -- 5.5 The Concept of Cutoff Rigidities and Asymptotic Directions -- References -- 6 Ground-Based Measurements of Energetic Particles by Neutron Monitors -- 6.1 Introduction -- 6.2 History -- 6.3 Transport of Cosmic Ray Particles in the Earth's Atmosphere -- 6.3.1 Model of the Earth's Atmosphere -- 6.3.2 Particle Cascade in the Atmosphere -- 6.4 Neutron Monitor Detector -- 6.4.1 Components of a Neutron Monitor -- 6.4.2 Neutron Monitor Yield Function -- 6.4.3 Atmospheric Effects -- 6.5 Worldwide Network of Neutron Monitor Stations as a Giant Spectrometer -- 6.6 Neutron Monitor Database: NMDB -- References -- 7 HESPERIA Forecasting Tools: Real-Time and Post-Event -- 7.1 Introduction -- 7.2 Predicting SEP Event Onsets from Historical Microwave Data by Using the UMASEP Scheme -- 7.3 Predicting SEP Energy Spectra from Historical Microwave Data -- 7.4 Predicting 30-50 MeV SEP Events by Using the RELeASE Scheme. 7.5 Predicting > -- 500 MeV SEP Events by Using the UMASEP Scheme -- 7.6 Concluding Remarks -- References -- 8 X-Ray, Radio and SEP Observations of Relativistic Gamma-Ray Events -- 8.1 Introduction -- 8.2 Theory and Early Observations of Gamma-Ray Emission at Photon Energies > -- 60MeV -- 8.2.1 Pion-Decay γ-Ray Emission -- 8.2.2 Long-Duration γ-Ray Events -- 8.3 New Insights of Sustained Emission Events from Fermi Observations -- 8.4 Multiwavelength Observations of Fermi/LAT γ-Ray Events -- 8.4.1 Impulsive and Early Post-impulsive γ-Ray Emission -- 8.4.2 Long-Duration γ-Ray Events -- 8.4.3 Soft X-Ray Bursts and γ-Ray Events -- 8.4.4 Coronal Shock Waves and γ-Ray Events -- 8.5 Solar Energetic Particle Events Associated with Fermi/LAT Gamma-Ray Events -- 8.5.1 SEP Characteristics and Association with Fermi/LAT -- 8.5.2 SEP Spectra -- 8.6 Summary and Discussion -- References -- 9 Modelling of Shock-Accelerated Gamma-Ray Events -- 9.1 Introduction -- 9.2 Model Description -- 9.2.1 Shock and Particle Model -- 9.2.2 Coronal Shock Acceleration Model -- 9.2.3 DownStream Propagation Model -- 9.3 Results -- 9.3.1 2012 May 17 Event -- 9.3.1.1 Modelling of the SEP Event -- 9.3.1.2 Simulations of Proton Acceleration at the Shock -- 9.3.1.3 Modelling of the Proton Transport Back to the Sun -- 9.3.2 2012 January 23 Event -- 9.3.2.1 Modelling of the SEP Event -- 9.3.2.2 Simulation of Proton Acceleration at the Shock -- 9.3.2.3 Modelling of the Proton Transport Back to the Sun -- 9.4 Discussion and Conclusions -- References -- 10 Inversion Methodology of Ground Level Enhancements -- 10.1 Introduction -- 10.2 Space and Ground Based Measurements of GLEs -- 10.2.1 dE/dx-dE/dx-Method -- 10.2.2 dE/dx - C -- 10.2.3 Magnet Spectrometer -- 10.3 Forward Modeling from the Sun to the Observer at Ground. 10.3.1 Interplanetary Particle Transport: From the Sun to the Magnetosphere -- 10.3.2 From the Interplanetary Particle Distribution to Neutron Monitor Measurements - Magneto- and Atmospheric Transport of Charged Energetic Particles -- 10.3.3 Combined Greens-Function -- 10.4 Inversion Methodology -- 10.4.1 Inversion of Spacecraft Data to the Sun -- 10.4.2 Inversion of NM Data to the Border of the Earth's Magnetosphere -- 10.4.3 The HESPERIA Approach -- 10.5 Results and Validation -- 10.6 Concluding Remarks -- References -- Index. |
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Electronic books. |
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Electronic books. |
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1076261138 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>07872nam a22004453i 4500</leader><controlfield tag="001">5005591474</controlfield><controlfield tag="003">MiAaPQ</controlfield><controlfield tag="005">20240229073831.0</controlfield><controlfield tag="006">m o d | </controlfield><controlfield tag="007">cr cnu||||||||</controlfield><controlfield tag="008">240229s2018 xx o ||||0 eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9783319600512</subfield><subfield code="q">(electronic bk.)</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="z">9783319600505</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(MiAaPQ)5005591474</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(Au-PeEL)EBL5591474</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)1076261138</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">MiAaPQ</subfield><subfield code="b">eng</subfield><subfield code="e">rda</subfield><subfield code="e">pn</subfield><subfield code="c">MiAaPQ</subfield><subfield code="d">MiAaPQ</subfield></datafield><datafield tag="050" ind1=" " ind2="4"><subfield code="a">QB520-545</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Malandraki, Olga E.</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Solar Particle Radiation Storms Forecasting and Analysis :</subfield><subfield code="b">The HESPERIA HORIZON 2020 Project and Beyond.</subfield></datafield><datafield tag="250" ind1=" " ind2=" "><subfield code="a">1st ed.</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Cham :</subfield><subfield code="b">Springer International Publishing AG,</subfield><subfield code="c">2018.</subfield></datafield><datafield tag="264" ind1=" " ind2="4"><subfield code="c">©2018.</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 online resource (210 pages)</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">computer</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">online resource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="490" ind1="1" ind2=" "><subfield code="a">Astrophysics and Space Science Library ;</subfield><subfield code="v">v.444</subfield></datafield><datafield tag="505" ind1="0" ind2=" "><subfield code="a">Intro -- Preface -- Acknowledgements -- Contents -- List of Abbreviations -- 1 Solar Energetic Particles and Space Weather: Science and Applications -- 1.1 Science -- 1.1.1 Historical Perspective of Solar Energetic Particle (SEP) Events -- 1.1.2 Large Gradual SEP Events -- 1.1.3 Ground Level Enhancement (GLE) Events -- 1.1.4 Multi-Spacecraft Observations of SEP Events -- 1.1.5 Particle Acceleration -- 1.1.6 Key Open Questions and Future Missions -- 1.2 Applications -- 1.2.1 Why Study SEP Events? -- 1.2.2 SEP Effects on Technology -- 1.2.3 SEPs and Human Health Effects -- 1.2.4 Mitigating the Effects of SEPs -- 1.2.4.1 Hazard Assessment -- 1.2.4.2 Mitigation Procedures -- References -- 2 Eruptive Activity Related to Solar Energetic Particle Events -- 2.1 Introduction -- 2.2 The Scene -- 2.3 Solar Flares: Energy Release and Radiative Signatures of Charged Particle Acceleration -- 2.3.1 Emission Processes -- 2.3.1.1 Bremsstrahlung -- 2.3.1.2 Gyrosynchrotron Radiation -- 2.3.1.3 Plasma Emission from Electron Beams -- 2.3.1.4 Gamma-Rays from Accelerated Protons and Ions -- 2.3.2 Where Are Electrons Accelerated in Solar Flares? -- 2.3.3 A Qualitative View of Acceleration Processes -- 2.4 What Is a Coronal Mass Ejection? -- 2.4.1 CME Magnetic Structure and Eruption -- 2.4.2 Shock Waves and Particle Acceleration at CMEs -- 2.5 Summary and Conclusion -- References -- 3 Particle Acceleration Mechanisms -- 3.1 Introduction -- 3.2 Acceleration Mechanisms -- 3.2.1 Large-Scale Electric Field Acceleration -- 3.2.2 Resonant Wave Acceleration -- 3.2.3 Shock Acceleration -- 3.2.4 Compressional Acceleration and Collapsing Magnetic Traps -- 3.2.5 Stochastic Acceleration -- 3.3 Concluding Remarks -- References -- 4 Charged Particle Transport in the Interplanetary Medium -- 4.1 Introduction -- 4.1.1 Energetic Particles in the Solar System.</subfield></datafield><datafield tag="505" ind1="8" ind2=" "><subfield code="a">4.1.2 The Interplanetary Magnetic Field -- 4.1.3 Motion of Charged Particles. First Adiabatic Invariant -- 4.2 Particle Transport -- 4.2.1 Particle Transport Equations -- 4.2.2 Focused Transport -- 4.2.3 Diffusive Transport -- 4.3 Application: Description of Solar Energetic Particle Events -- 4.3.1 Numerical Techniques -- 4.3.2 Observations -- 4.3.3 Inferring Transport Conditions -- 4.4 Concluding Remarks -- References -- 5 Cosmic Ray Particle Transport in the Earth's Magnetosphere -- 5.1 Introduction -- 5.2 Motion of Charged Particles in a Magnetic Field: Lorentz Force -- 5.3 Earth's Magnetic Field -- 5.3.1 The Magnetic Field of the Earth as a Dipole Field -- 5.3.2 Magnetic Field Model Due to Internal Sources: IGRF -- 5.3.3 Contributions to the Earth's Magnetic Field by Magnetospheric Electric Currents -- 5.3.4 Magnetic Field Models of the External Sources -- 5.4 Computation of the Propagation of Cosmic Ray Particles in the Earth's Magnetosphere -- 5.5 The Concept of Cutoff Rigidities and Asymptotic Directions -- References -- 6 Ground-Based Measurements of Energetic Particles by Neutron Monitors -- 6.1 Introduction -- 6.2 History -- 6.3 Transport of Cosmic Ray Particles in the Earth's Atmosphere -- 6.3.1 Model of the Earth's Atmosphere -- 6.3.2 Particle Cascade in the Atmosphere -- 6.4 Neutron Monitor Detector -- 6.4.1 Components of a Neutron Monitor -- 6.4.2 Neutron Monitor Yield Function -- 6.4.3 Atmospheric Effects -- 6.5 Worldwide Network of Neutron Monitor Stations as a Giant Spectrometer -- 6.6 Neutron Monitor Database: NMDB -- References -- 7 HESPERIA Forecasting Tools: Real-Time and Post-Event -- 7.1 Introduction -- 7.2 Predicting SEP Event Onsets from Historical Microwave Data by Using the UMASEP Scheme -- 7.3 Predicting SEP Energy Spectra from Historical Microwave Data -- 7.4 Predicting 30-50 MeV SEP Events by Using the RELeASE Scheme.</subfield></datafield><datafield tag="505" ind1="8" ind2=" "><subfield code="a">7.5 Predicting &gt -- 500 MeV SEP Events by Using the UMASEP Scheme -- 7.6 Concluding Remarks -- References -- 8 X-Ray, Radio and SEP Observations of Relativistic Gamma-Ray Events -- 8.1 Introduction -- 8.2 Theory and Early Observations of Gamma-Ray Emission at Photon Energies &gt -- 60MeV -- 8.2.1 Pion-Decay γ-Ray Emission -- 8.2.2 Long-Duration γ-Ray Events -- 8.3 New Insights of Sustained Emission Events from Fermi Observations -- 8.4 Multiwavelength Observations of Fermi/LAT γ-Ray Events -- 8.4.1 Impulsive and Early Post-impulsive γ-Ray Emission -- 8.4.2 Long-Duration γ-Ray Events -- 8.4.3 Soft X-Ray Bursts and γ-Ray Events -- 8.4.4 Coronal Shock Waves and γ-Ray Events -- 8.5 Solar Energetic Particle Events Associated with Fermi/LAT Gamma-Ray Events -- 8.5.1 SEP Characteristics and Association with Fermi/LAT -- 8.5.2 SEP Spectra -- 8.6 Summary and Discussion -- References -- 9 Modelling of Shock-Accelerated Gamma-Ray Events -- 9.1 Introduction -- 9.2 Model Description -- 9.2.1 Shock and Particle Model -- 9.2.2 Coronal Shock Acceleration Model -- 9.2.3 DownStream Propagation Model -- 9.3 Results -- 9.3.1 2012 May 17 Event -- 9.3.1.1 Modelling of the SEP Event -- 9.3.1.2 Simulations of Proton Acceleration at the Shock -- 9.3.1.3 Modelling of the Proton Transport Back to the Sun -- 9.3.2 2012 January 23 Event -- 9.3.2.1 Modelling of the SEP Event -- 9.3.2.2 Simulation of Proton Acceleration at the Shock -- 9.3.2.3 Modelling of the Proton Transport Back to the Sun -- 9.4 Discussion and Conclusions -- References -- 10 Inversion Methodology of Ground Level Enhancements -- 10.1 Introduction -- 10.2 Space and Ground Based Measurements of GLEs -- 10.2.1 dE/dx-dE/dx-Method -- 10.2.2 dE/dx - C -- 10.2.3 Magnet Spectrometer -- 10.3 Forward Modeling from the Sun to the Observer at Ground.</subfield></datafield><datafield tag="505" ind1="8" ind2=" "><subfield code="a">10.3.1 Interplanetary Particle Transport: From the Sun to the Magnetosphere -- 10.3.2 From the Interplanetary Particle Distribution to Neutron Monitor Measurements - Magneto- and Atmospheric Transport of Charged Energetic Particles -- 10.3.3 Combined Greens-Function -- 10.4 Inversion Methodology -- 10.4.1 Inversion of Spacecraft Data to the Sun -- 10.4.2 Inversion of NM Data to the Border of the Earth's Magnetosphere -- 10.4.3 The HESPERIA Approach -- 10.5 Results and Validation -- 10.6 Concluding Remarks -- References -- Index.</subfield></datafield><datafield tag="588" ind1=" " ind2=" "><subfield code="a">Description based on publisher supplied metadata and other sources.</subfield></datafield><datafield tag="590" ind1=" " ind2=" "><subfield code="a">Electronic reproduction. Ann Arbor, Michigan : ProQuest Ebook Central, 2024. Available via World Wide Web. Access may be limited to ProQuest Ebook Central affiliated libraries. </subfield></datafield><datafield tag="655" ind1=" " ind2="4"><subfield code="a">Electronic books.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Crosby, Norma B.</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Print version:</subfield><subfield code="a">Malandraki, Olga E.</subfield><subfield code="t">Solar Particle Radiation Storms Forecasting and Analysis</subfield><subfield code="d">Cham : Springer International Publishing AG,c2018</subfield><subfield code="z">9783319600505</subfield></datafield><datafield tag="797" ind1="2" ind2=" "><subfield code="a">ProQuest (Firm)</subfield></datafield><datafield tag="830" ind1=" " ind2="0"><subfield code="a">Astrophysics and Space Science Library</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://ebookcentral.proquest.com/lib/oeawat/detail.action?docID=5591474</subfield><subfield code="z">Click to View</subfield></datafield></record></collection> |