Future Instrumentation for Solar and Stellar Research at Radio ...

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Strawman FASR Specifications Frequency range Frequency resolution Time resolution Number antennas Size antennas Polarization Angular resolution Field of View ~0.1 – 30 GHz
FASR Science • Nature & Evolution of Coronal Magnetic Fields Measurement of coronal magnetic fields Temporal & spatial evolution of fields Role of electric currents in corona • Coronal Mass Ejections Birth Acceleration B, n rl , n th Prominence eruptions • Flares Energy release Plasma heating Electron acceleration and transport
Page 1 and 2: Future Instrumentation for Solar an
Page 3 and 4: And Beyond … •SKA - Square Kilo
Page 5 and 6: By deploying N antennas over a two
Page 7: The EVLAThe EVLA (Phase 1) Point so
Page 10 and 11: Configurations Nested rings with di
Page 12 and 13: from R. Simon
Page 14 and 15: CARMA Combine the six 10.4 m antenn
Page 16 and 17: The Frequency Agile Solar Radiotele
Page 20 and 21: from J. Lee
Page 22 and 23: FASR Science • Nature & Evolution
Page 24 and 25: Noise storm Bastian et al. (2001)
Page 26 and 27: from Aschwanden & Benz 1997
Page 28 and 29: Status and Plans The NAS/NRC Astron
Page 30 and 31: The ATA The ATA is a project of the
Page 32 and 33: 6.1 m x 7.0 m Primary Log-periodic
Page 34 and 35: ATA Science • SETI - 100,000 FGK
Page 36 and 37: SM146 Concept (VLA Scientific Memor
Page 38 and 39: SM146 CAPABILITY SM146 SM146 SM146
Page 40 and 41: SKA Finally, it is worth mentioning
Page 42 and 43: Originally conceived as a “red sh

Future Instrumentation for Solar and Stellar Research at Radio ...

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