دورية أكاديمية
Magnetic energy powers the corona: how we can understand its 3D storage & release
| العنوان: | Magnetic energy powers the corona: how we can understand its 3D storage & release |
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| المؤلفون: | Caspi, A., Seaton, D., Casini, R., Downs, C., Gibson, S., Gilbert, H., Glesener, L., Guidoni, S., Hughes, J.M., McKenzie, D., Plowman, J., Reeves, K., Saint-Hilaire, P., Shih, A.Y., West, M., Alaoui, M., Alexander, D., Allred, J.C., Antiochos, S., Ashfield, W., Ballai, I., Barata, T., Barta, M., Benz, A.O., Berlicki, A., Bradshaw, S.J., Bröse, M., Buitrago-Casas, J.C., Cassak, P., Chamberlin, P., Che, H., Chen, T.Y., Chen, B., Cheng, X., Christe, S., Comisso, L., Dahlin, J., Nolfo, G.D., Dennis, B., Dickson, E.C.M., Drake, J., Dudík, J., Dzifcakova, E., Emslie, G., Erdelyi, R., Farid, S., Fleishman, G., French, R., Gallagher, P.T., Gan, W., Gary, D., Guo, F., Hayes, L.A., Hudson, H., Ji, H., Jones, A.R., Kansabanik, D., Kawate, T., Kerr, G.S., Keshav, A., Knuth, T., Kobelski, A., Kooi, J., Kumari, A., Lee, J., Li, Y., Longo, F., Maharana, A., Mandrini, C.H., Oliveros, J.C.M., Mason, J.P., Mason, E.I., Massone, A.M., McAteer, R.T.J., McConnell, M., McTiernan, J., Mitchell, J.G., Mohan, A., Motorina, G., Mrozek, T., Musset, S., Narukage, N., Nayak, S.S., Nitta, N., Panesar, N., Pariat, E., Piana, M., Pohjolainen, S., Qiu, J., Reale, F., Rivera, Y., Rozelot, J.P., Sarkar, R., Setterberg, W., Shaik, S.B., Shaikh, Z., Sharma, R., Skokic, I., Stores, M., Struminsky, A., Sylwester, J., Takahashi, T., Tiwari, S., Tsiklauri, D., Vievering, J.T., Warmuth, A., White, S., Zimovets, I.V. |
| بيانات النشر: | American Astronomical Society |
| سنة النشر: | 2023 |
| المجموعة: | White Rose Research Online (Universities of Leeds, Sheffield & York) |
| الوصف: | The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. It is, however, still poorly observed and understood. We highlight key questions related to magnetic energy storage, release, and transport in the solar corona, and their relationship to these important problems. We advocate for new and multi-point co-optimized measurements, sensitive to magnetic field and other plasma parameters, spanning from optical to γ-ray wavelengths, to bring closure to these long-standing and fundamental questions. We discuss how our approach can fully describe the 3D magnetic field, embedded plasma, particle energization, and their joint evolution to achieve these objectives. |
| نوع الوثيقة: | article in journal/newspaper |
| وصف الملف: | text |
| اللغة: | English |
| العلاقة: | https://eprints.whiterose.ac.uk/203430/1/21692975172443.pdfTest; Caspi, A. orcid.org/0000-0001-8702-8273 , Seaton, D. orcid.org/0000-0002-0494-2025 , Casini, R. orcid.org/0000-0001-6990-513X et al. (105 more authors) (2023) Magnetic energy powers the corona: how we can understand its 3D storage & release. Bulletin of the American Astronomical Society, 55 (3). |
| DOI: | 10.3847/25c2cfeb.1dbfea1f |
| الإتاحة: | https://doi.org/10.3847/25c2cfeb.1dbfea1fTest https://eprints.whiterose.ac.uk/203430Test/ https://eprints.whiterose.ac.uk/203430/1/21692975172443.pdfTest |
| حقوق: | cc_by_4 |
| رقم الانضمام: | edsbas.9C67B4B3 |
| قاعدة البيانات: | BASE |
| DOI: | 10.3847/25c2cfeb.1dbfea1f |
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