Solar bipolar magnetic fields (Yamamoto, 2012)

Details Solar bipolar magnetic fields (Yamamoto, 2012) Solar bipolar magnetic fields (Yamamoto, 2012)

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ycat..35399013y&link_type=abstract

VizieR On-line Data Catalog: J/A+A/539/A13. Originally published in: 2012A&A...539A..13Y

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Sun, Magnetic Fields

Scientific paper

'Table_3.dat' is the list of bipolar regions. The date (column 1-3), MDI daily number (column 4), field-weighted position (x, y), area, average field strengths of the positive field (column 5-8), and those of the negative field (column 9-12). Morphological parameters in our paper are derived from these values.
The field-weighted positions (x, y), area, average field strength of the positive and negative fields are derived from MDI longitudinal magnetograms.
We analyzed 96 minutes cadence data sets. In these data sets, we analyzed the magnetogram observed around 00:00 UT on each day. The pixel width of the magnetograms is 1.98 arcsec.
(1 data file).

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