Editorial: Earth-affecting Solar Transients
- Autores
- Zhang, Jiaen; Blanco Cano, Xochitl Guillermina; Nitta, Nariaki; Srivastava, Nandita; Mandrini, Cristina Hemilse
- Año de publicación
- 2018
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- This Topical Collection (TC) is devoted to the recent advancement in the study of Earth-affecting solar transients. Earth-affecting solar transients encompass a broad range of phenomena, including major solar flares, coronal mass ejections (CMEs), interplanetary CMEs (ICMEs), solar energetic particle (SEP) events, and corotating interaction regions (CIRs). In the past decade, nearly continuous observations of the Sun and the inner heliosphere with an unprecedented wide spatial coverage from a fleet of spacecraft, including the Solar Terrestrial Relations ObservatoryAhead/Behind (STEREO A/B), the Solar Dynamics Observatory (SDO), the Solar and Heliospheric Observatory (SOHO), the Mercury Surface, Space Environment, Geochemistry, and Ranging (MESSENGER) spacecraft, Venus Express (VEX), the Advance Composition Explorer (ACE), and Wind, in combination with a significant development and improvement of global magnetohydrodynamics (MHD) numerical simulations and theoretical analyses, have greatly improved our understanding of solar transients and the prediction of their potential impact on Earth.
Fil: Zhang, Jiaen. George Mason University; Estados Unidos
Fil: Blanco Cano, Xochitl Guillermina. Universidad Nacional Autónoma de México; México
Fil: Nitta, Nariaki. Lockheed Martin Corporation;
Fil: Srivastava, Nandita. Physical Research Laboratory India; India. Center Of Excellence In Space Sciences India; India
Fil: Mandrini, Cristina Hemilse. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Universidad de Buenos Aires; Argentina - Materia
-
Sun: Coronal Mass Ejections
Sun: Flares
Interplanetary Coronal Mass Ejections
Space Weather - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/80659
Ver los metadatos del registro completo
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Editorial: Earth-affecting Solar TransientsZhang, JiaenBlanco Cano, Xochitl GuillerminaNitta, NariakiSrivastava, NanditaMandrini, Cristina HemilseSun: Coronal Mass EjectionsSun: FlaresInterplanetary Coronal Mass EjectionsSpace Weatherhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1This Topical Collection (TC) is devoted to the recent advancement in the study of Earth-affecting solar transients. Earth-affecting solar transients encompass a broad range of phenomena, including major solar flares, coronal mass ejections (CMEs), interplanetary CMEs (ICMEs), solar energetic particle (SEP) events, and corotating interaction regions (CIRs). In the past decade, nearly continuous observations of the Sun and the inner heliosphere with an unprecedented wide spatial coverage from a fleet of spacecraft, including the <em class="EmphasisTypeItalic ">Solar Terrestrial Relations Observatory</em><em class="EmphasisTypeItalic ">Ahead</em>/<em class="EmphasisTypeItalic ">Behind</em> (STEREO A/B), the <em class="EmphasisTypeItalic ">Solar Dynamics Observatory</em> (SDO), the <em class="EmphasisTypeItalic ">Solar and Heliospheric Observatory</em> (SOHO), the <em class="EmphasisTypeItalic ">Mercury Surface, Space Environment, Geochemistry, and Ranging</em> (MESSENGER) spacecraft, <em class="EmphasisTypeItalic ">Venus Express</em> (VEX), the <em class="EmphasisTypeItalic ">Advance Composition Explorer</em> (ACE), and <em class="EmphasisTypeItalic ">Wind</em>, in combination with a significant development and improvement of global magnetohydrodynamics (MHD) numerical simulations and theoretical analyses, have greatly improved our understanding of solar transients and the prediction of their potential impact on Earth.Fil: Zhang, Jiaen. George Mason University; Estados UnidosFil: Blanco Cano, Xochitl Guillermina. Universidad Nacional Autónoma de México; MéxicoFil: Nitta, Nariaki. Lockheed Martin Corporation;Fil: Srivastava, Nandita. Physical Research Laboratory India; India. Center Of Excellence In Space Sciences India; IndiaFil: Mandrini, Cristina Hemilse. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Universidad de Buenos Aires; ArgentinaSpringer2018-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/80659Zhang, Jiaen; Blanco Cano, Xochitl Guillermina; Nitta, Nariaki; Srivastava, Nandita; Mandrini, Cristina Hemilse; Editorial: Earth-affecting Solar Transients; Springer; Solar Physics; 293; 5; 5-2018; 1-60038-0938CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1007/s11207-018-1302-9info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:13:33Zoai:ri.conicet.gov.ar:11336/80659instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:13:34.205CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Editorial: Earth-affecting Solar Transients |
title |
Editorial: Earth-affecting Solar Transients |
spellingShingle |
Editorial: Earth-affecting Solar Transients Zhang, Jiaen Sun: Coronal Mass Ejections Sun: Flares Interplanetary Coronal Mass Ejections Space Weather |
title_short |
Editorial: Earth-affecting Solar Transients |
title_full |
Editorial: Earth-affecting Solar Transients |
title_fullStr |
Editorial: Earth-affecting Solar Transients |
title_full_unstemmed |
Editorial: Earth-affecting Solar Transients |
title_sort |
Editorial: Earth-affecting Solar Transients |
dc.creator.none.fl_str_mv |
Zhang, Jiaen Blanco Cano, Xochitl Guillermina Nitta, Nariaki Srivastava, Nandita Mandrini, Cristina Hemilse |
author |
Zhang, Jiaen |
author_facet |
Zhang, Jiaen Blanco Cano, Xochitl Guillermina Nitta, Nariaki Srivastava, Nandita Mandrini, Cristina Hemilse |
author_role |
author |
author2 |
Blanco Cano, Xochitl Guillermina Nitta, Nariaki Srivastava, Nandita Mandrini, Cristina Hemilse |
author2_role |
author author author author |
dc.subject.none.fl_str_mv |
Sun: Coronal Mass Ejections Sun: Flares Interplanetary Coronal Mass Ejections Space Weather |
topic |
Sun: Coronal Mass Ejections Sun: Flares Interplanetary Coronal Mass Ejections Space Weather |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
This Topical Collection (TC) is devoted to the recent advancement in the study of Earth-affecting solar transients. Earth-affecting solar transients encompass a broad range of phenomena, including major solar flares, coronal mass ejections (CMEs), interplanetary CMEs (ICMEs), solar energetic particle (SEP) events, and corotating interaction regions (CIRs). In the past decade, nearly continuous observations of the Sun and the inner heliosphere with an unprecedented wide spatial coverage from a fleet of spacecraft, including the <em class="EmphasisTypeItalic ">Solar Terrestrial Relations Observatory</em><em class="EmphasisTypeItalic ">Ahead</em>/<em class="EmphasisTypeItalic ">Behind</em> (STEREO A/B), the <em class="EmphasisTypeItalic ">Solar Dynamics Observatory</em> (SDO), the <em class="EmphasisTypeItalic ">Solar and Heliospheric Observatory</em> (SOHO), the <em class="EmphasisTypeItalic ">Mercury Surface, Space Environment, Geochemistry, and Ranging</em> (MESSENGER) spacecraft, <em class="EmphasisTypeItalic ">Venus Express</em> (VEX), the <em class="EmphasisTypeItalic ">Advance Composition Explorer</em> (ACE), and <em class="EmphasisTypeItalic ">Wind</em>, in combination with a significant development and improvement of global magnetohydrodynamics (MHD) numerical simulations and theoretical analyses, have greatly improved our understanding of solar transients and the prediction of their potential impact on Earth. Fil: Zhang, Jiaen. George Mason University; Estados Unidos Fil: Blanco Cano, Xochitl Guillermina. Universidad Nacional Autónoma de México; México Fil: Nitta, Nariaki. Lockheed Martin Corporation; Fil: Srivastava, Nandita. Physical Research Laboratory India; India. Center Of Excellence In Space Sciences India; India Fil: Mandrini, Cristina Hemilse. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Universidad de Buenos Aires; Argentina |
description |
This Topical Collection (TC) is devoted to the recent advancement in the study of Earth-affecting solar transients. Earth-affecting solar transients encompass a broad range of phenomena, including major solar flares, coronal mass ejections (CMEs), interplanetary CMEs (ICMEs), solar energetic particle (SEP) events, and corotating interaction regions (CIRs). In the past decade, nearly continuous observations of the Sun and the inner heliosphere with an unprecedented wide spatial coverage from a fleet of spacecraft, including the <em class="EmphasisTypeItalic ">Solar Terrestrial Relations Observatory</em><em class="EmphasisTypeItalic ">Ahead</em>/<em class="EmphasisTypeItalic ">Behind</em> (STEREO A/B), the <em class="EmphasisTypeItalic ">Solar Dynamics Observatory</em> (SDO), the <em class="EmphasisTypeItalic ">Solar and Heliospheric Observatory</em> (SOHO), the <em class="EmphasisTypeItalic ">Mercury Surface, Space Environment, Geochemistry, and Ranging</em> (MESSENGER) spacecraft, <em class="EmphasisTypeItalic ">Venus Express</em> (VEX), the <em class="EmphasisTypeItalic ">Advance Composition Explorer</em> (ACE), and <em class="EmphasisTypeItalic ">Wind</em>, in combination with a significant development and improvement of global magnetohydrodynamics (MHD) numerical simulations and theoretical analyses, have greatly improved our understanding of solar transients and the prediction of their potential impact on Earth. |
publishDate |
2018 |
dc.date.none.fl_str_mv |
2018-05 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/80659 Zhang, Jiaen; Blanco Cano, Xochitl Guillermina; Nitta, Nariaki; Srivastava, Nandita; Mandrini, Cristina Hemilse; Editorial: Earth-affecting Solar Transients; Springer; Solar Physics; 293; 5; 5-2018; 1-6 0038-0938 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/80659 |
identifier_str_mv |
Zhang, Jiaen; Blanco Cano, Xochitl Guillermina; Nitta, Nariaki; Srivastava, Nandita; Mandrini, Cristina Hemilse; Editorial: Earth-affecting Solar Transients; Springer; Solar Physics; 293; 5; 5-2018; 1-6 0038-0938 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1007/s11207-018-1302-9 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Springer |
publisher.none.fl_str_mv |
Springer |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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12.982451 |