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Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME

Remotely sensed interplanetary scintillation (IPS) data from the Institute for Space-Earth Environmental Research (ISEE), Japan, allows a determination of solar-wind parameters throughout the inner heliosphere. We show the 3D analysis technique developed for these data sets that forecast plasma velo...

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Autores principales: Jackson, Bernard V., Tokumaru, Munetoshi, Iwai, Kazumasa, Bracamontes, Matthew T., Buffington, Andrew, Fujiki, Ken’ichi, Murakami, Go, Heyner, Daniel, Sanchez-Cano, Beatriz, Rojo, Mathias, Aizawa, Sae, Andre, Nicolas, Barthe, Alain, Penou, Emmanuel, Fedorov, Andrei, Sauvaud, Jean-Andre, Yokota, Shoichiro, Saito, Yoshifumi
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Netherlands 2023
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10229700/
https://www.ncbi.nlm.nih.gov/pubmed/37266352
http://dx.doi.org/10.1007/s11207-023-02169-8
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author Jackson, Bernard V.
Tokumaru, Munetoshi
Iwai, Kazumasa
Bracamontes, Matthew T.
Buffington, Andrew
Fujiki, Ken’ichi
Murakami, Go
Heyner, Daniel
Sanchez-Cano, Beatriz
Rojo, Mathias
Aizawa, Sae
Andre, Nicolas
Barthe, Alain
Penou, Emmanuel
Fedorov, Andrei
Sauvaud, Jean-Andre
Yokota, Shoichiro
Saito, Yoshifumi
author_facet Jackson, Bernard V.
Tokumaru, Munetoshi
Iwai, Kazumasa
Bracamontes, Matthew T.
Buffington, Andrew
Fujiki, Ken’ichi
Murakami, Go
Heyner, Daniel
Sanchez-Cano, Beatriz
Rojo, Mathias
Aizawa, Sae
Andre, Nicolas
Barthe, Alain
Penou, Emmanuel
Fedorov, Andrei
Sauvaud, Jean-Andre
Yokota, Shoichiro
Saito, Yoshifumi
author_sort Jackson, Bernard V.
collection PubMed
description Remotely sensed interplanetary scintillation (IPS) data from the Institute for Space-Earth Environmental Research (ISEE), Japan, allows a determination of solar-wind parameters throughout the inner heliosphere. We show the 3D analysis technique developed for these data sets that forecast plasma velocity, density, and component magnetic fields at Earth, as well at the other inner heliospheric planets and spacecraft. One excellent coronal mass ejection (CME) example that occurred on the 10 March 2022 was viewed not only in the ISEE IPS analyses, but also by the spacecraft near Earth that measured the CME arrival at one AU. Solar Orbiter, that was nearly aligned along the Earth radial at 0.45 AU, also measured the CME in plasma density, velocity, and magnetic field. BepiColombo at 0.42 AU was also aligned with the STEREO A spacecraft, and viewed this CME. The instruments used here from BepiColombo include: 1) the European-Space-Agency Mercury-Planetary-Orbiter magnetic field measurements; 2) the Japan Aerospace Exploration Agency Mio spacecraft Solar Particle Monitor that viewed the CME Forbush decrease, and the Mercury Plasma Experiment/Mercury Electron Analyzer instruments that measured particles and solar-wind density from below the spacecraft protective sunshield covering. This article summarizes the analysis using ISEE, Japan real-time data for these forecasts: it provides a synopsis of the results and confirmation of the CME event morphology after its arrival, and discusses how future IPS analyses can augment these results.
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spelling pubmed-102297002023-06-01 Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME Jackson, Bernard V. Tokumaru, Munetoshi Iwai, Kazumasa Bracamontes, Matthew T. Buffington, Andrew Fujiki, Ken’ichi Murakami, Go Heyner, Daniel Sanchez-Cano, Beatriz Rojo, Mathias Aizawa, Sae Andre, Nicolas Barthe, Alain Penou, Emmanuel Fedorov, Andrei Sauvaud, Jean-Andre Yokota, Shoichiro Saito, Yoshifumi Sol Phys Research Remotely sensed interplanetary scintillation (IPS) data from the Institute for Space-Earth Environmental Research (ISEE), Japan, allows a determination of solar-wind parameters throughout the inner heliosphere. We show the 3D analysis technique developed for these data sets that forecast plasma velocity, density, and component magnetic fields at Earth, as well at the other inner heliospheric planets and spacecraft. One excellent coronal mass ejection (CME) example that occurred on the 10 March 2022 was viewed not only in the ISEE IPS analyses, but also by the spacecraft near Earth that measured the CME arrival at one AU. Solar Orbiter, that was nearly aligned along the Earth radial at 0.45 AU, also measured the CME in plasma density, velocity, and magnetic field. BepiColombo at 0.42 AU was also aligned with the STEREO A spacecraft, and viewed this CME. The instruments used here from BepiColombo include: 1) the European-Space-Agency Mercury-Planetary-Orbiter magnetic field measurements; 2) the Japan Aerospace Exploration Agency Mio spacecraft Solar Particle Monitor that viewed the CME Forbush decrease, and the Mercury Plasma Experiment/Mercury Electron Analyzer instruments that measured particles and solar-wind density from below the spacecraft protective sunshield covering. This article summarizes the analysis using ISEE, Japan real-time data for these forecasts: it provides a synopsis of the results and confirmation of the CME event morphology after its arrival, and discusses how future IPS analyses can augment these results. Springer Netherlands 2023-05-30 2023 /pmc/articles/PMC10229700/ /pubmed/37266352 http://dx.doi.org/10.1007/s11207-023-02169-8 Text en © The Author(s) 2023 https://creativecommons.org/licenses/by/4.0/Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) .
spellingShingle Research
Jackson, Bernard V.
Tokumaru, Munetoshi
Iwai, Kazumasa
Bracamontes, Matthew T.
Buffington, Andrew
Fujiki, Ken’ichi
Murakami, Go
Heyner, Daniel
Sanchez-Cano, Beatriz
Rojo, Mathias
Aizawa, Sae
Andre, Nicolas
Barthe, Alain
Penou, Emmanuel
Fedorov, Andrei
Sauvaud, Jean-Andre
Yokota, Shoichiro
Saito, Yoshifumi
Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME
title Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME
title_full Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME
title_fullStr Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME
title_full_unstemmed Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME
title_short Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME
title_sort forecasting heliospheric cme solar-wind parameters using the ucsd time-dependent tomography and isee interplanetary scintillation data: the 10 march 2022 cme
topic Research
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10229700/
https://www.ncbi.nlm.nih.gov/pubmed/37266352
http://dx.doi.org/10.1007/s11207-023-02169-8
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