SDO HMI 2014-12-13 07:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.76 | 150.29 | 29.05 | 162.72 | -4.01 | 1.11 | 62.75 | 265.84 | 0.8911 | 550.5 | 149.0 | |
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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 | 1.36 | 0.00 | 1.59 | -3.39 | 3.21 | 64.84 | 266.57 | 0.9070 | -272.0 | -275.9 | |
| 0.00 | 0.68 | 0.00 | 0.76 | -1.69 | 1.82 | 63.46 | 268.45 | 0.8964 | 337.0 | 244.0 | |
| 0.43 | 1.36 | 0.47 | 1.50 | -2.04 | 1.64 | 63.28 | 268.05 | 0.8951 | 29.4 | 66.4 | |
| 0.00 | 0.60 | 0.00 | 0.65 | -1.87 | 1.57 | 63.20 | 268.25 | 0.8944 | 257.0 | 221.0 | |
| 26.33 | 136.49 | 28.58 | 148.27 | -4.18 | 1.21 | 62.85 | 265.65 | 0.8919 | 723.4 | 169.7 | |
| 0.00 | 1.19 | 0.00 | 1.23 | -2.54 | 359.69 | 61.33 | 267.48 | 0.8793 | 235.0 | 186.1 | |
| 0.00 | 3.92 | 0.00 | 4.03 | -1.92 | 359.58 | 61.22 | 268.18 | 0.8784 | -264.0 | -223.6 | |
| 0.00 | 1.45 | 0.00 | 1.47 | -1.98 | 359.22 | 60.86 | 268.11 | 0.8754 | -194.0 | -217.3 | |
| 0.00 | 1.11 | 0.00 | 1.10 | -2.87 | 358.56 | 60.19 | 267.07 | 0.8698 | 502.0 | 408.4 | |
| 0.00 | 1.02 | 0.00 | 1.02 | -2.75 | 358.55 | 60.18 | 267.21 | 0.8697 | 363.0 | 414.7 | |
| 0.00 | 1.11 | 0.00 | 1.10 | -1.72 | 358.36 | 60.00 | 268.40 | 0.8680 | -185.0 | -210.5 | |
| 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. | |