Abstract
We compare high resolution observations of a Solar Active Region (A.R. 7530) performed with the Westerbork Synthesis Radio Telescope, at 5000 MHz (λ = 6 cm), with images obtained with the SXT onboard the Yohkoh satellite and with the coronal magnetic field, extrapolated from Marshall Space Flight Center (MSFC) photospheric magnetograms.
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References
Alissandrakis, C.E. (1981) Astron. Astrophys. 100, 197
Alissandrakis, C.E. and Chiuderi Drago, F. (1994) Astrophys. J. Letters 426, L72
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© 1996 Kluwer Academic Publishers
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Drago, F.C., Borgioli, F., Alissandrakis, C.E., Hagyard, M., Shibasaki, K. (1996). Coronal Magnetic Fields from Polarization Observations at Microwaves. In: Uchida, Y., Kosugi, T., Hudson, H.S. (eds) Magnetodynamic Phenomena in the Solar Atmosphere. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0315-9_88
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DOI: https://doi.org/10.1007/978-94-009-0315-9_88
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6627-3
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