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- W1645533835 abstract "Abstract : This contract was a study of possible variations in the observed flux from coronal holes over a solar cycle and their relationship to solar magnetic fields. The variation of X-ray emission from coronal holes was measured and compared with data on photospheric magnetic field strength and models of open field structures from holes. The data set consisted of reduced X-ray images from ASE (2) the particular holes that we measured were typical of those at each phase of the cycle in terms of their evolutionary and interplanetary characteristics; and (3) the X-ray hole emission followed a similar trend in Harvey et al.'s (1982) data whereby the photospheric field strength of near-equatorial holes increased systematically by a factor of three between 1975 and 1980. Further, our own measurements of field strengths within the X-ray hole boundaries were sparse but generally in agreement with the Harvey et al. trend. Keywords include: Coronal Holes; Solar cycle variations; Solar X-ray; Coronal images." @default.
- W1645533835 created "2016-06-24" @default.
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- W1645533835 date "1984-12-01" @default.
- W1645533835 modified "2023-09-27" @default.
- W1645533835 title "A Study of the Cyclical Variations of Coronal Holes and Their Relation to Open Magnetic Fields." @default.
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