Only proposals for continuum observations in Bands 3, 5, 6 and 7 will be accepted. For the interferometric observations, these will be obtained using the low spectral resolution (TDM) mode, and the high spectral resolution (FDM) mode is not offered (please see Appendix Section "Solar Observations" in Cycle-10 Proposer's Guide).
Band | spw1 | spw2 | LO1 | spw3 | spw4 |
| (GHz) | (GHz) | (GHz) | (GHz) | (GHz) |
3 | 93.0 | 95.0 | 100.0 | 105.0 | 107.0 |
5 | 191.0 | 193.0 | 198.0 | 203.0 | 205.0 |
6 | 230.0 | 232.0 | 239.0 | 246.0 | 248.0 |
7 | 339.6 | 341.6 | 346.6 | 351.6 | 353.6 |
Observing frequencies for Cycle 10 solar observations. This table assumes that each baseband is populated with a single spectral window (spw) centered on the baseband frequency.