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TWO-FLUID MODEL FOR HEATING OF THE SOLAR CORONA AND ACCELERATION OF THE SOLAR WIND BY HIGH-FREQUENCY ALFVÉN WAVES

✍ Scribed by C.-Y. Tu; E. Marsch

Book ID
110217768
Publisher
Springer
Year
1997
Tongue
English
Weight
292 KB
Volume
171
Category
Article
ISSN
0038-0938

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Comment on the paper ‘Two-Fluid Model of
Comment on the paper ‘Two-Fluid Model of the Solar Corona’ by J. W. Knight, C. E. Newman, and P. A. Sturrock
✍ Donald E. Billings 📂 Article 📅 1975 🏛 Springer 🌐 English ⚖ 138 KB

Observational line width evidence for a possible discrepancy between ion and electron temperature in the corona is reviewed for comparison with the conclusions of Knight et al. We note that the high line-width temperatures extend much higher in the corona than the high ion temperatures computed by K