Coronal magnetic fields inferred from IR wavelength and comparison with EUV observations
Spectropolarimetry using IR wavelength of 1075 nm has been proved to be a powerful tool for directly mapping solar coronal magnetic fields including transverse component directions and line-of-sight component intensities. Solar tomography, or stereoscopy based on EUV observations, can supply 3-D...
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| Format: | Article |
| Language: | English |
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Copernicus Publications
2009-07-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/27/2771/2009/angeo-27-2771-2009.pdf |