| The
EVLA (Phase 1) |
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| How does it compare with FASR? |
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| The
good news: |
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| The
EVLA will be will be significantly more sensitive than FASR for |
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| quiet
Sun studies. |
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| The
bad news: |
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| • | No frequency agility |
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| • | Restricted FOV |
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| • | Non-optimum configurations |
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| • | Limited access (~3%/yr) |
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