Abstract
Several advantages of near infrared spectral lines for magnetic field measurements are listed. In particular, the 10830 Å multiplet of HeI is well suited for observations of chromospheric magnetic fields.
New photoelectric spectroheliograms made with the 10830 A line reveal a large amount of filamentary fine structure in active regions. This fine structure has important consequences on the interpretation of 10830 Å magnetograms. Except for an association of 10830 Å disk filaments with polarity reversals there is little correlation between absorption features and the 10830 Å longitudinal field. Comparisons of chromospheric and photo spheric observations show that the chromospheric field is spatially more diffuse and weaker than the photospheric field.
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Harvey, J., Hall, D. (1971). Magnetic Fields Measured with the 10 830 Å Hei Line. In: Howard, R. (eds) Solar Magnetic Fields. International Astronomical Union / Union Astronomique Internationale, vol 43. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3117-2_38
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DOI: https://doi.org/10.1007/978-94-010-3117-2_38
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