Anticipating the results from the Rosetta magnetometer experiment, we present a theoretical study concerning the possible origin of a cometary magnetic field. Assuming the existence of a permanently magnetized iron dust fraction in the primordial solar nebula, we use a numerical model to investigate
β¦ LIBER β¦
Accretion of dust by chondrules in a MHD-turbulent solar nebula
β Scribed by Augusto Carballido
- Book ID
- 108138909
- Publisher
- Elsevier Science
- Year
- 2011
- Tongue
- English
- Weight
- 570 KB
- Volume
- 211
- Category
- Article
- ISSN
- 0019-1035
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