SDO HMI 2014-10-12 02:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.86 | 0.00 | 11.10 | 13.91 | 58.36 | 19.87 | 294.23 | 0.3615 | -45.6 | 28.4 | |
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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 | 1.14 | 0.00 | 0.64 | 11.66 | 67.05 | 28.56 | 283.16 | 0.4828 | -597.0 | -460.9 | |
| 0.00 | 2.10 | 0.00 | 1.18 | 11.98 | 66.63 | 28.14 | 283.96 | 0.4774 | -681.0 | -626.4 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 12.96 | 66.33 | 27.84 | 286.11 | 0.4757 | -693.0 | -579.4 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 18.08 | 60.79 | 22.30 | 300.81 | 0.4217 | -611.0 | -533.9 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 18.27 | 60.78 | 22.29 | 301.21 | 0.4229 | -497.0 | -506.0 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 15.27 | 60.11 | 21.62 | 295.11 | 0.3942 | -784.0 | -660.9 | |
| 0.00 | 2.19 | 0.00 | 1.17 | 15.74 | 58.96 | 20.47 | 297.32 | 0.3805 | -839.0 | -625.3 | |
| 0.00 | 2.89 | 0.00 | 1.51 | 13.65 | 55.24 | 16.75 | 295.86 | 0.3127 | 720.0 | 692.3 | |
| 0.00 | 2.98 | 0.00 | 1.55 | 13.15 | 55.08 | 16.59 | 294.54 | 0.3070 | 136.0 | 309.9 | |
| 0.00 | 1.58 | 0.00 | 0.82 | 13.37 | 54.64 | 16.15 | 295.75 | 0.3019 | 882.0 | 727.1 | |
| 0.00 | 1.23 | 0.00 | 0.63 | 13.45 | 52.93 | 14.44 | 298.40 | 0.2769 | 796.0 | 681.1 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 14.55 | 52.43 | 13.94 | 302.75 | 0.2784 | 608.0 | 518.1 | |
| 0.00 | 1.49 | 0.00 | 0.76 | 11.83 | 51.26 | 12.77 | 295.34 | 0.2405 | 967.0 | 737.6 | |
| 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. | |