The evolution of the charged particles are followed during contraction of a model of an interstellar cloud, with initial density number of n = 10 cmV3. The contraction is followed up to density increase by five orders of magnitude. Special care is given to the details of the negative ions. In addit
β¦ LIBER β¦
Evolution of extended clouds of particles near the sun and stars
β Scribed by V. A. Antonov; A. S. Baranov
- Publisher
- Springer
- Year
- 2009
- Tongue
- English
- Weight
- 178 KB
- Volume
- 52
- Category
- Article
- ISSN
- 0571-7256
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## Abstract During an investigation into convective cloud at a single temperature level near β6Β°C, observations by aircraft have found ice crystal concentrations significantly in excess (up to 600 L^β1^) of those to be expected from primary ice formation (i.e. ice multiplication). Despite the fact