SDO HMI 2014-12-10 21:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.43 | 324.57 | 33.76 | 187.69 | -3.81 | 1.10 | 30.90 | 263.17 | 0.5182 | 888.6 | 371.3 | |
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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 | 0.94 | 0.00 | 0.58 | -2.49 | 7.28 | 37.08 | 266.32 | 0.6058 | 591.0 | 495.9 | |
| 34.07 | 304.20 | 19.77 | 176.09 | -4.07 | 1.39 | 31.19 | 262.73 | 0.5229 | 1166.2 | 392.3 | |
| 1.70 | 3.83 | 0.98 | 2.21 | -1.38 | 1.18 | 30.98 | 267.88 | 0.5170 | -893.3 | -670.8 | |
| 3.07 | -2.00 | 1.77 | -2.00 | -2.89 | 0.97 | 30.77 | 264.93 | 0.5150 | 750.6 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.44 | -1.68 | 0.91 | 30.71 | 267.29 | 0.5131 | -713.0 | -529.0 | |
| 14.57 | -2.00 | 8.40 | -2.00 | -3.86 | 0.83 | 30.63 | 263.01 | 0.5142 | 1298.2 | 999999 | |
| 1.70 | -2.00 | 0.98 | -2.00 | -2.62 | 0.76 | 30.56 | 265.42 | 0.5116 | 750.6 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.64 | -2.00 | 0.43 | 30.23 | 266.61 | 0.5062 | -559.0 | -438.5 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -2.98 | 359.43 | 29.23 | 264.52 | 0.4920 | 774.0 | 614.6 | |
| 0.00 | 3.07 | 0.00 | 1.74 | -2.18 | 359.08 | 28.88 | 266.10 | 0.4857 | 962.0 | 804.9 | |
| 0.00 | 1.45 | 0.00 | 0.82 | -1.92 | 359.00 | 28.80 | 266.64 | 0.4844 | 1016.0 | 859.4 | |
| 0.00 | 0.77 | 0.00 | 0.43 | -3.93 | 358.45 | 28.25 | 262.37 | 0.4784 | 739.0 | 530.2 | |
| 3.32 | 7.07 | 1.86 | 3.97 | -3.25 | 358.13 | 27.93 | 263.72 | 0.4724 | -936.4 | -744.0 | |
| 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. | |