SDO HMI 2014-01-02 14:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.42 | 41.02 | 13.64 | 33.34 | -12.21 | 116.52 | -52.13 | 103.01 | 0.7922 | 332.0 | 150.7 | |
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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 | 1.02 | 0.00 | 0.70 | -14.74 | 125.87 | -42.78 | 108.10 | 0.6934 | 599.0 | 525.3 | |
| 0.00 | 1.02 | 0.00 | 0.79 | -14.58 | 118.73 | -49.92 | 106.31 | 0.7739 | 620.0 | 524.9 | |
| 9.69 | 19.88 | 7.41 | 15.19 | -11.38 | 119.23 | -49.42 | 102.24 | 0.7642 | 815.8 | 589.7 | |
| 0.85 | -3.00 | 0.65 | -3.00 | -11.49 | 119.02 | -49.63 | 102.36 | 0.7667 | 445.0 | 999999 | |
| 6.46 | 9.60 | 5.19 | 7.71 | -12.33 | 116.98 | -51.67 | 103.19 | 0.7894 | 629.4 | 318.6 | |
| 0.00 | 0.68 | 0.00 | 0.60 | -13.52 | 113.17 | -55.48 | 104.21 | 0.8285 | 265.0 | 219.4 | |
| 0.42 | 1.27 | 0.39 | 1.16 | -12.67 | 111.83 | -56.82 | 103.06 | 0.8404 | -569.0 | -524.6 | |
| 0.00 | 1.44 | 0.00 | 1.34 | -13.88 | 111.21 | -57.44 | 104.43 | 0.8470 | -531.0 | -426.5 | |
| 0.00 | 1.02 | 0.00 | 0.95 | -13.66 | 111.07 | -57.58 | 104.16 | 0.8481 | -418.0 | -402.2 | |
| 0.00 | 1.10 | 0.00 | 1.03 | -13.78 | 111.02 | -57.63 | 104.29 | 0.8486 | -251.0 | -226.6 | |
| 0.00 | 1.78 | 0.00 | 1.66 | -11.73 | 110.91 | -57.74 | 101.86 | 0.8482 | -515.0 | -393.2 | |
| 0.00 | 1.19 | 0.00 | 1.13 | -13.29 | 110.18 | -58.47 | 103.64 | 0.8557 | -292.0 | -241.2 | |
| 0.00 | 1.02 | 0.00 | 1.08 | -12.94 | 106.56 | -62.09 | 102.96 | 0.8857 | -439.0 | -414.1 | |
| 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. | |