On a numerical model for extracting TKE dissipation rate from very high frequency (VHF) radar spectral width
Abstract The standard model (e.g., Hocking in Earth Planets Space 51:525–541, 1999), $$\varepsilon = c_{0} \sigma^{2} N$$ ε=c0σ2N , (where $$\sigma$$ σ is the radar spectral width assumed to be equal to vertical turbulence velocity fluctuation $$\sqrt {\overline{{w^{2} }} }$$ w2¯ , N is the buoyancy...
| Main Authors: | , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
SpringerOpen
2018-12-01
|
| Series: | Earth, Planets and Space |
| Subjects: | |
| Online Access: | http://link.springer.com/article/10.1186/s40623-018-0957-7 |