SDO HMI 2014-12-11 08:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.77 | 291.49 | 33.40 | 180.94 | -3.92 | 1.08 | 36.91 | 264.04 | 0.6047 | 830.8 | 308.0 | |
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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 |
| 1.36 | 2.73 | 0.85 | 1.70 | -1.49 | 1.38 | 37.21 | 268.09 | 0.6072 | -749.7 | -589.2 | |
| 33.75 | 277.86 | 21.03 | 172.67 | -4.12 | 1.37 | 37.20 | 263.75 | 0.6089 | 1096.4 | 332.8 | |
| 14.40 | -2.00 | 8.91 | -2.00 | -3.92 | 0.80 | 36.63 | 264.01 | 0.6008 | 1243.5 | 999999 | |
| 3.15 | -2.00 | 1.94 | -2.00 | -2.82 | 0.64 | 36.47 | 265.82 | 0.5975 | 789.2 | 999999 | |
| 0.00 | 0.34 | 0.00 | 0.21 | -5.82 | 0.51 | 36.34 | 260.80 | 0.5995 | 380.0 | 541.8 | |
| 0.00 | 0.68 | 0.00 | 0.42 | -1.82 | 0.14 | 35.97 | 267.48 | 0.5898 | -710.0 | -579.1 | |
| 0.00 | 0.85 | 0.00 | 0.52 | -3.42 | 359.31 | 35.14 | 264.66 | 0.5793 | 716.0 | 635.3 | |
| 0.34 | 1.28 | 0.21 | 0.77 | -3.54 | 359.14 | 34.97 | 264.44 | 0.5769 | 703.2 | 699.7 | |
| 0.77 | 1.79 | 0.46 | 1.08 | -2.00 | 358.76 | 34.59 | 267.08 | 0.5703 | 896.0 | 767.9 | |
| 0.00 | 1.02 | 0.00 | 0.62 | -2.80 | 358.68 | 34.51 | 265.67 | 0.5696 | -610.0 | -427.9 | |
| 0.00 | 1.02 | 0.00 | 0.61 | -2.51 | 358.63 | 34.46 | 266.19 | 0.5688 | -272.0 | -267.6 | |
| 0.00 | 0.77 | 0.00 | 0.46 | -2.65 | 358.56 | 34.39 | 265.92 | 0.5679 | -609.0 | -545.4 | |
| 0.00 | 3.15 | 0.00 | 1.88 | -3.34 | 358.09 | 33.92 | 264.66 | 0.5616 | -859.0 | -690.7 | |
| 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. | |