Defining the Middle Corona

The middle corona, the region roughly spanning heliocentric distances from 1.5 to 6 solar radii, encompasses almost all of the influential physical transitions and processes that govern the behavior of coronal outflow into the heliosphere. The solar wind, eruptions, and flows pass through the region...

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Detalles Bibliográficos
Autores principales: West, Matthew J., Seaton, Daniel B., Wexler, David B., Raymond, John C., Del Zanna, Giulio, Rivera, Yeimy J., Kobelski, Adam R., Chen, Bin, DeForest, Craig, Golub, Leon, Caspi, Amir, Gilly, Chris R., Kooi, Jason E., Meyer, Karen A., Alterman, Benjamin L., Alzate, Nathalia, Andretta, Vincenzo, Auchère, Frédéric, Banerjee, Dipankar, Berghmans, David, Chamberlin, Phillip, Chitta, Lakshmi Pradeep, Downs, Cooper, Giordano, Silvio, Harra, Louise, Higginson, Aleida, Howard, Russell A., Kumar, Pankaj, Mason, Emily, Mason, James P., Morton, Richard J., Nykyri, Katariina, Patel, Ritesh, Rachmeler, Laurel, Reardon, Kevin P., Reeves, Katharine K., Savage, Sabrina, Thompson, Barbara J., Van Kooten, Samuel J., Viall, Nicholeen M., Vourlidas, Angelos, Zhukov, Andrei N.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Netherlands 2023
Materias:
Review
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10267282/
https://www.ncbi.nlm.nih.gov/pubmed/37325237
http://dx.doi.org/10.1007/s11207-023-02170-1

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