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
✦ LIBER ✦
Dust blobs in the solar nebula — primary distended atmosphere
✍ Scribed by Sho Sasaki
- Publisher
- Springer Netherlands
- Year
- 1994
- Tongue
- English
- Weight
- 487 KB
- Volume
- 212
- Category
- Article
- ISSN
- 0004-640X
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