SDO HMI 2014-11-26 03:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.72 | 310.07 | 94.03 | 830.72 | -15.52 | 242.56 | 77.99 | 253.81 | 0.9802 | -392.1 | -62.3 | |
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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 | 11.22 | 0.00 | 105.81 | -12.63 | 250.96 | 86.39 | 257.26 | 0.9987 | -40.0 | -47.6 | |
| 0.00 | 3.43 | 0.00 | 30.04 | -13.54 | 250.92 | 86.35 | 256.35 | 0.9987 | 179.0 | 157.4 | |
| 0.00 | 1.54 | 0.00 | 3.67 | -11.89 | 242.00 | 77.42 | 257.50 | 0.9792 | 193.0 | 132.8 | |
| 0.00 | 1.37 | 0.00 | 3.14 | -12.85 | 241.40 | 76.83 | 256.48 | 0.9773 | -329.0 | -268.8 | |
| 6.17 | 291.65 | 14.12 | 686.24 | -14.47 | 241.19 | 76.62 | 254.81 | 0.9771 | -460.4 | -75.3 | |
| 3.00 | -5.00 | 7.43 | -5.00 | -15.51 | 242.15 | 77.58 | 253.83 | 0.9807 | -194.0 | 999999 | |
| 3.34 | -5.00 | 7.50 | -5.00 | -14.86 | 240.96 | 76.38 | 254.39 | 0.9764 | -577.7 | 999999 | |
| 0.00 | 0.86 | 0.00 | 1.82 | -14.81 | 240.13 | 75.55 | 254.37 | 0.9732 | -342.0 | -353.6 | |
| 5.39 | -5.00 | 11.95 | -5.00 | -15.69 | 240.71 | 76.13 | 253.53 | 0.9757 | -377.5 | 999999 | |
| 8.31 | -5.00 | 20.22 | -5.00 | -17.02 | 241.84 | 77.27 | 252.27 | 0.9801 | -53.5 | 999999 | |
| 4.20 | -5.00 | 9.63 | -5.00 | -16.75 | 241.21 | 76.63 | 252.48 | 0.9779 | -561.7 | 999999 | |
| 1.46 | -5.00 | 3.16 | -5.00 | -16.98 | 240.30 | 75.72 | 252.17 | 0.9747 | -287.2 | 999999 | |
| 9.85 | -5.00 | 20.02 | -5.00 | -16.73 | 239.39 | 74.82 | 252.33 | 0.9711 | -714.5 | 999999 | |
| 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. | |