SDO HMI 2014-12-08 13:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.98 | 358.61 | 28.78 | 178.02 | -3.82 | 1.23 | 0.26 | 183.66 | 0.0668 | 1219.1 | 420.8 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.68 | 0.00 | 0.34 | -4.27 | 6.15 | 5.18 | 230.77 | 0.1169 | 802.0 | 675.4 | |
| 0.00 | 1.11 | 0.00 | 0.55 | -5.07 | 5.27 | 4.30 | 220.48 | 0.1155 | 882.0 | 653.8 | |
| 0.00 | 0.68 | 0.00 | 0.34 | -5.48 | 5.00 | 4.03 | 216.48 | 0.1183 | 737.0 | 572.1 | |
| 0.00 | 2.13 | 0.00 | 1.06 | -4.71 | 3.93 | 2.96 | 212.35 | 0.0966 | 876.0 | 648.9 | |
| 33.00 | 341.05 | 16.38 | 169.28 | -3.91 | 1.47 | 0.50 | 187.39 | 0.0682 | 1472.1 | 418.2 | |
| 2.22 | -5.00 | 1.10 | -5.00 | -3.58 | 1.26 | 0.29 | 184.75 | 0.0621 | 1230.6 | 999999 | |
| 0.00 | 2.22 | 0.00 | 1.10 | -2.61 | 1.23 | 0.27 | 185.92 | 0.0451 | 944.0 | 778.8 | |
| 0.00 | 1.19 | 0.00 | 0.59 | -2.23 | 0.94 | -0.03 | 179.22 | 0.0381 | 902.0 | 813.4 | |
| 22.76 | -5.00 | 11.30 | -5.00 | -3.61 | 0.85 | -0.12 | 178.07 | 0.0625 | 1474.2 | 999999 | |
| 0.00 | 3.50 | 0.00 | 1.74 | -5.00 | 0.46 | -0.51 | 174.17 | 0.0872 | 1085.0 | 874.3 | |
| 0.00 | 2.81 | 0.00 | 1.40 | -4.94 | 0.11 | -0.86 | 170.03 | 0.0870 | 903.0 | 781.8 | |
| 0.00 | 0.94 | 0.00 | 0.47 | -5.80 | 359.13 | -1.84 | 162.28 | 0.1057 | -794.0 | -705.6 | |
| 0.00 | 2.30 | 0.00 | 1.15 | -5.51 | 359.07 | -1.90 | 160.83 | 0.1011 | -1184.0 | -918.9 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |