On the formation of Io’s inner torus
✍ Scribed by M.M. Cowee; Y.-L. Wang; C.T. Russell; D.A. Gurnett
- Publisher
- Elsevier Science
- Year
- 2005
- Tongue
- English
- Weight
- 410 KB
- Volume
- 36
- Category
- Article
- ISSN
- 0273-1177
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A radiative-thermal conduction model for the vertical thermal structure of Io's atmosphere is developed with solar heating by \(\mathrm{SO}_{2}\) absorption in UV and near-IR bands and non-LTE cooling by \(\mathrm{SO}_{2} \nu_{1}, \nu_{2}, \nu_{3}\), vibrational bands and rotational lines. The model
## Let be the set of finite, simple and nondirected graphs being not embeddable into the torus. Furthermore let >4 be a partial order-relation and M, (r) the minimal basis of I'. In this paper we determine three graphs of M, (r) being embeddable into the projective plane and containing the subgrap