SDO HMI 2014-12-11 02:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.68 | 308.73 | 33.80 | 184.04 | -3.92 | 1.13 | 33.68 | 263.51 | 0.5590 | 866.2 | 362.5 | |
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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 | -5.93 | 3.72 | 36.27 | 260.55 | 0.5988 | 623.0 | 576.5 | |
| 37.84 | 290.07 | 22.64 | 173.10 | -4.10 | 1.39 | 33.94 | 263.24 | 0.5630 | 1059.1 | 375.5 | |
| 0.60 | 3.49 | 0.36 | 2.08 | -1.47 | 1.27 | 33.83 | 267.93 | 0.5590 | -839.3 | -686.6 | |
| 2.73 | -2.00 | 1.62 | -2.00 | -2.89 | 0.84 | 33.40 | 265.34 | 0.5538 | 731.8 | 999999 | |
| 13.46 | -2.00 | 8.00 | -2.00 | -3.86 | 0.81 | 33.36 | 263.57 | 0.5544 | 1244.5 | 999999 | |
| 0.00 | 1.19 | 0.00 | 0.70 | -1.85 | 0.32 | 32.88 | 267.17 | 0.5454 | -597.0 | -534.9 | |
| 0.00 | 1.11 | 0.00 | 0.66 | -6.71 | 0.16 | 32.72 | 258.29 | 0.5504 | 565.0 | 513.8 | |
| 0.00 | 0.77 | 0.00 | 0.45 | -2.83 | 359.78 | 32.34 | 265.32 | 0.5382 | 652.0 | 508.1 | |
| 0.00 | 0.68 | 0.00 | 0.40 | -5.73 | 359.57 | 32.12 | 259.90 | 0.5395 | 685.0 | 541.2 | |
| 0.00 | 2.81 | 0.00 | 1.64 | -2.80 | 359.15 | 31.71 | 265.29 | 0.5289 | 598.0 | 590.9 | |
| 0.00 | 2.73 | 0.00 | 1.58 | -1.97 | 358.93 | 31.48 | 266.84 | 0.5248 | 795.0 | 772.0 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -4.07 | 358.78 | 31.34 | 262.81 | 0.5250 | 782.0 | 610.8 | |
| 2.05 | 3.58 | 1.18 | 2.06 | -3.28 | 358.06 | 30.62 | 264.22 | 0.5131 | -855.8 | -726.1 | |
| 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. | |