Measurements of magnetic field alignment
نویسندگان
چکیده
منابع مشابه
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A long-standing solar problem has been to measure the coronal magnetic field. We believe it determines the coronal structure and dynamics from the upper chromosphere out into the heliospheric environment. It is only recently that Zeeman splitting observations of infrared coronal emission lines have been successfully used to deduce the coronal magnetic flux density. Here we extend this technique...
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ژورنال
عنوان ژورنال: IEEE Transactions on Magnetics
سال: 1988
ISSN: 0018-9464
DOI: 10.1109/20.11384