Emitted cyclotron frequency, magnetopause size, and co-latitude of the polar cap of HD189733b, calculated for different planetary magnetic field strengths. These values only vary by small amounts through the orbit and between each epoch.
| Bp . | fc . | Rm . | α0 . |
|---|---|---|---|
| (G) . | (MHz) . | (Rp) . | (°) . |
| 1 | 2 | 1.6 | 53 |
| 5 | 12 | 2.7 | 38 |
| 10 | 25 | 3.3 | 33 |
| Bp . | fc . | Rm . | α0 . |
|---|---|---|---|
| (G) . | (MHz) . | (Rp) . | (°) . |
| 1 | 2 | 1.6 | 53 |
| 5 | 12 | 2.7 | 38 |
| 10 | 25 | 3.3 | 33 |
Emitted cyclotron frequency, magnetopause size, and co-latitude of the polar cap of HD189733b, calculated for different planetary magnetic field strengths. These values only vary by small amounts through the orbit and between each epoch.
| Bp . | fc . | Rm . | α0 . |
|---|---|---|---|
| (G) . | (MHz) . | (Rp) . | (°) . |
| 1 | 2 | 1.6 | 53 |
| 5 | 12 | 2.7 | 38 |
| 10 | 25 | 3.3 | 33 |
| Bp . | fc . | Rm . | α0 . |
|---|---|---|---|
| (G) . | (MHz) . | (Rp) . | (°) . |
| 1 | 2 | 1.6 | 53 |
| 5 | 12 | 2.7 | 38 |
| 10 | 25 | 3.3 | 33 |
This PDF is available to Subscribers Only
View Article Abstract & Purchase OptionsFor full access to this pdf, sign in to an existing account, or purchase an annual subscription.
