SDO HMI 2014-12-11 05:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.96 | 289.87 | 31.00 | 176.25 | -3.95 | 1.17 | 35.37 | 263.76 | 0.5831 | 914.5 | 365.7 | |
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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 | 0.77 | 0.00 | 0.48 | -5.85 | 3.87 | 38.06 | 261.06 | 0.6231 | 665.0 | 497.0 | |
| 34.35 | 265.33 | 20.96 | 161.51 | -4.11 | 1.42 | 35.61 | 263.51 | 0.5868 | 1096.3 | 377.5 | |
| 0.00 | 2.81 | 0.00 | 1.71 | -1.45 | 1.33 | 35.52 | 268.06 | 0.5834 | -951.0 | -694.2 | |
| 12.61 | -2.00 | 7.64 | -2.00 | -3.88 | 0.82 | 35.02 | 263.83 | 0.5781 | 1259.5 | 999999 | |
| 2.81 | 10.31 | 1.70 | 6.23 | -2.87 | 0.75 | 34.94 | 265.57 | 0.5760 | 780.4 | 554.6 | |
| 0.00 | 1.36 | 0.00 | 0.82 | -1.84 | 0.21 | 34.41 | 267.33 | 0.5676 | -824.0 | -580.2 | |
| 0.00 | 1.28 | 0.00 | 0.77 | -4.83 | 0.33 | 34.52 | 262.10 | 0.5724 | 376.0 | 387.5 | |
| 0.00 | 1.11 | 0.00 | 0.66 | -2.82 | 359.67 | 33.86 | 265.55 | 0.5604 | 613.0 | 564.0 | |
| 0.00 | 1.02 | 0.00 | 0.61 | -2.64 | 359.02 | 33.22 | 265.80 | 0.5509 | 642.0 | 597.2 | |
| 0.00 | 2.47 | 0.00 | 1.46 | -1.99 | 358.83 | 33.02 | 266.97 | 0.5476 | 970.0 | 793.9 | |
| 0.00 | 0.68 | 0.00 | 0.40 | -4.06 | 358.83 | 33.02 | 263.19 | 0.5496 | 787.0 | 653.0 | |
| 1.19 | 2.73 | 0.70 | 1.60 | -3.32 | 358.09 | 32.29 | 264.43 | 0.5380 | -774.9 | -652.2 | |
| 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. | |