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Highly structured slow solar wind emerging from an equatorial coronal hole.
Bale SD, Badman ST, Bonnell JW, Bowen TA, Burgess D, Case AW, Cattell CA, Chandran BDG, Chaston CC, Chen CHK, Drake JF, de Wit TD, Eastwood JP, Ergun RE, Farrell WM, Fong C, Goetz K, Goldstein M, Goodrich KA, Harvey PR, Horbury TS, Howes GG, Kasper JC, Kellogg PJ, Klimchuk JA, Korreck KE, Krasnoselskikh VV, Krucker S, Laker R, Larson DE, MacDowall RJ, Maksimovic M, Malaspina DM, Martinez-Oliveros J, McComas DJ, Meyer-Vernet N, Moncuquet M, Mozer FS, Phan TD, Pulupa M, Raouafi NE, Salem C, Stansby D, Stevens M, Szabo A, Velli M, Woolley T, Wygant JR. Bale SD, et al. Among authors: phan td. Nature. 2019 Dec;576(7786):237-242. doi: 10.1038/s41586-019-1818-7. Epub 2019 Dec 4. Nature. 2019. PMID: 31802007
Observations of turbulence generated by magnetic reconnection.
Eastwood JP, Phan TD, Bale SD, Tjulin A. Eastwood JP, et al. Among authors: phan td. Phys Rev Lett. 2009 Jan 23;102(3):035001. doi: 10.1103/PhysRevLett.102.035001. Epub 2009 Jan 20. Phys Rev Lett. 2009. PMID: 19257361 Free article.
120 results