ICME Evolution in the Inner Heliosphere
Author:
Funder
National Aeronautics and Space Administration
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://link.springer.com/content/pdf/10.1007/s11207-020-01624-0.pdf
Reference263 articles.
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2. Al-Haddad, N., Poedts, S., Roussev, I., Farrugia, C.J., Yu, W., Lugaz, N.: 2019, The magnetic morphology of magnetic clouds: multi-spacecraft investigation of twisted and writhed coronal mass ejections. Astrophys. J.870, 100. DOI .
3. Arge, C.N., Pizzo, V.J.: 2000, Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates. J. Geophys. Res.105, 10469.
4. Attrill, G.D.R., Harra, L.K., van Driel-Gesztelyi, L., Démoulin, P.: 2007, Coronal “wave”: magnetic footprint of a coronal mass ejection? Astrophys. J. Lett.656, L101.
5. Bain, H.M., Mays, M.L., Luhmann, J.G., Li, Y., Jian, L.K., Odstrcil, D.: 2016, Shock connectivity in the August 2010 and July 2012 solar energetic particle events inferred from observations and ENLIL modeling. Astrophys. J.825, 1. DOI .
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