Sigmoid Eruption Associated with the X9.3 Flare from AR 12673 Drives the Gradual Solar Energetic Particle Event on 2017 September 6

Autor: Stephanie L. Yardley, David H. Brooks

Publikováno v: The Astrophysical Journal, Vol 976, Iss 2, p 152 (2024)

Large gradual solar energetic particle (SEP) events can pose a radiation risk to crewed spaceflight and a significant threat to near-Earth satellites; however, the origin of the SEP seed particle population, and how these particles are released, acce

Externí odkaz: https://doaj.org/article/5f80916148cc480b84a67f543acb817b

Slow Solar Wind Connection Science during Solar Orbiter’s First Close Perihelion Passage

Autor: Stephanie L. Yardley, Christopher J. Owen, David M. Long, Deborah Baker, David H. Brooks, Vanessa Polito, Lucie M. Green, Sarah Matthews, Mathew Owens, Mike Lockwood, David Stansby, Alexander W. James, Gherardo Valori, Alessandra Giunta, Miho Janvier, Nawin Ngampoopun, Teodora Mihailescu, Andy S. H. To, Lidia van Driel-Gesztelyi, Pascal Démoulin, Raffaella D’Amicis, Ryan J. French, Gabriel H. H. Suen, Alexis P. Rouillard, Rui F. Pinto, Victor Réville, Christopher J. Watson, Andrew P. Walsh, Anik De Groof, David R. Williams, Ioannis Zouganelis, Daniel Müller, David Berghmans, Frédéric Auchère, Louise Harra, Udo Schuehle, Krysztof Barczynski, Éric Buchlin, Regina Aznar Cuadrado, Emil Kraaikamp, Sudip Mandal, Susanna Parenti, Hardi Peter, Luciano Rodriguez, Conrad Schwanitz, Phil Smith, Luca Teriaca, Cis Verbeeck, Andrei N. Zhukov, Bart De Pontieu, Tim Horbury, Sami K. Solanki, Jose Carlos del Toro Iniesta, Joachim Woch, Achim Gandorfer, Johann Hirzberger, David Orozco Súarez, Thierry Appourchaux, Daniele Calchetti, Jonas Sinjan, Fatima Kahil, Kinga Albert, Reiner Volkmer, Mats Carlsson, Andrzej Fludra, Don Hassler, Martin Caldwell, Terje Fredvik, Tim Grundy, Steve Guest, Margit Haberreiter, Sarah Leeks, Gabriel Pelouze, Joseph Plowman, Werner Schmutz, Sunil Sidher, William T. Thompson, Philippe Louarn, Andrei Federov

Publikováno v: The Astrophysical Journal Supplement Series, Vol 267, Iss 1, p 11 (2023)

The Slow Solar Wind Connection Solar Orbiter Observing Plan (Slow Wind SOOP) was developed to utilize the extensive suite of remote-sensing and in situ instruments on board the ESA/NASA Solar Orbiter mission to answer significant outstanding question

Externí odkaz: https://doaj.org/article/0066ae64811043d48a0175ce81e45182

Investigating Remote-Sensing Techniques to Reveal Stealth Coronal Mass Ejections

Autor: Erika Palmerio, Nariaki V. Nitta, Tamitha Mulligan, Marilena Mierla, Jennifer O’Kane, Ian G. Richardson, Suvadip Sinha, Nandita Srivastava, Stephanie L. Yardley, Andrei N. Zhukov

Publikováno v: Frontiers in Astronomy and Space Sciences, Vol 8 (2021)

Eruptions of coronal mass ejections (CMEs) from the Sun are usually associated with a number of signatures that can be identified in solar disc imagery. However, there are cases in which a CME that is well observed in coronagraph data is missing a cl

Externí odkaz: https://doaj.org/article/1a0995f474ab42109c86e8f5dab2e5d1

Signature and escape of highly fractionated plasma in an active region

Autor: Stephanie L. Yardley, David H. Brooks

Accurate forecasting of space weather requires knowledge of the source regions where solar energetic particles (SEP) and eruptive events originate. Recent work has linked several major SEP events in 2014, January, to specific features in the host act

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e793b60f448f4a9291360665b6540b0
http://arxiv.org/abs/2109.11157

Decoding the Pre-Eruptive Magnetic Field Configurations of Coronal Mass Ejections

Autor: Jie Zhang, P. Syntelis, Tibor Torok, Ronald L. Moore, Georgios Chintzoglou, Spiros Patsourakos, Guillaume Aulanier, Manolis K. Georgoulis, Stephanie L. Yardley, Alexander Nindos, Vasilis Archontis, James E. Leake, Spiro K. Antiochos, Lucie M. Green, Vasyl Yurchyshyn, Angelos Vourlidas, Bernhard Kliem, Xin Cheng

Publikováno v: Space Science Reviews. 216

A clear understanding of the nature of the pre-eruptive magnetic field configurations of Coronal Mass Ejections (CMEs) is required for understanding and eventually predicting solar eruptions. Only two, but seemingly disparate, magnetic configurations

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b44d53e4ab4143bfcf6c2a134ff18aa2
https://doi.org/10.1007/s11214-020-00757-9