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Knowledgebase: Project Planning
Which frequency setup is possible for solar observations?
Posted by Misato Fukagawa, Last modified by Sarah Wood on 19 March 2018 05:40 PM
The LO1 frequency for solar observations is fixed to 100 GHz for Band 3 and 239 GHz for Band 6. Only proposals for continuum observations 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 Proposer's Guide).
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