SDO HMI 2014-10-12 03:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.65 | 0.00 | 10.14 | 13.52 | 60.70 | 22.76 | 290.70 | 0.4025 | -162.6 | -134.8 | |
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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 | 0.35 | 0.00 | 0.20 | 11.72 | 67.00 | 29.06 | 283.14 | 0.4904 | -597.0 | -579.5 | |
| 0.00 | 2.63 | 0.00 | 1.49 | 11.98 | 66.64 | 28.70 | 283.78 | 0.4857 | -730.0 | -565.4 | |
| 0.00 | 0.96 | 0.00 | 0.55 | 13.59 | 66.43 | 28.49 | 287.13 | 0.4871 | -632.0 | -537.8 | |
| 0.00 | 0.70 | 0.00 | 0.39 | 11.09 | 63.86 | 25.92 | 282.80 | 0.4418 | -678.0 | -544.1 | |
| 0.00 | 1.23 | 0.00 | 0.68 | 14.38 | 63.34 | 25.40 | 290.33 | 0.4450 | -675.0 | -513.7 | |
| 0.00 | 2.19 | 0.00 | 1.21 | 14.59 | 63.26 | 25.32 | 290.84 | 0.4448 | -651.0 | -551.4 | |
| 0.00 | 2.80 | 0.00 | 1.50 | 12.74 | 59.87 | 21.93 | 288.68 | 0.3862 | 790.0 | 551.1 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 17.37 | 60.38 | 22.44 | 299.13 | 0.4189 | -562.0 | -464.1 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 15.30 | 60.10 | 22.16 | 294.73 | 0.4022 | -805.0 | -689.9 | |
| 0.00 | 1.49 | 0.00 | 0.80 | 15.80 | 58.95 | 21.01 | 296.95 | 0.3887 | -844.0 | -724.8 | |
| 0.00 | 1.31 | 0.00 | 0.68 | 12.58 | 55.20 | 17.26 | 292.09 | 0.3138 | 834.0 | 647.5 | |
| 0.00 | 0.70 | 0.00 | 0.37 | 13.78 | 55.19 | 17.25 | 295.66 | 0.3209 | 695.0 | 650.8 | |
| 0.00 | 1.40 | 0.00 | 0.73 | 13.38 | 53.39 | 15.45 | 296.73 | 0.2916 | 748.0 | 574.1 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 11.84 | 51.28 | 13.34 | 294.51 | 0.2492 | 830.0 | 679.2 | |
| 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. | |