SDO HMI 2014-07-13 01:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.72 | 343.09 | 171.04 | 1049.34 | -7.35 | 241.46 | 80.11 | 261.85 | 0.9858 | -14.2 | 96.0 | |
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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 |
| 16.70 | 167.96 | 70.42 | 694.83 | -7.34 | 243.83 | 82.48 | 262.09 | 0.9933 | 344.7 | 185.8 | |
| 4.90 | -1.00 | 21.65 | -1.00 | -8.84 | 244.03 | 82.68 | 260.60 | 0.9939 | 232.6 | 999999 | |
| 0.00 | 5.45 | 0.00 | 14.91 | -4.85 | 240.56 | 79.20 | 264.30 | 0.9845 | 443.0 | 255.3 | |
| 0.00 | 1.45 | 0.00 | 3.25 | -4.40 | 238.13 | 76.77 | 264.54 | 0.9760 | -160.0 | -151.1 | |
| 1.27 | 4.45 | 2.77 | 9.67 | -4.83 | 237.74 | 76.38 | 264.06 | 0.9747 | -143.1 | -125.9 | |
| 8.44 | 64.64 | 18.19 | 134.64 | -6.60 | 237.41 | 76.06 | 262.22 | 0.9741 | -489.7 | 63.2 | |
| 4.27 | -6.00 | 8.82 | -6.00 | -5.55 | 236.97 | 75.61 | 263.25 | 0.9719 | 302.2 | 999999 | |
| 14.25 | 67.00 | 30.19 | 140.91 | -8.00 | 237.11 | 75.75 | 260.75 | 0.9735 | -535.7 | -238.8 | |
| 9.17 | 25.15 | 14.72 | 40.10 | -4.92 | 232.91 | 71.56 | 263.47 | 0.9527 | -454.7 | -337.8 | |
| 0.00 | 0.27 | 0.00 | 0.44 | -5.96 | 232.72 | 71.36 | 262.36 | 0.9522 | -346.0 | -330.7 | |
| 2.72 | 6.72 | 4.28 | 10.59 | -5.63 | 232.43 | 71.07 | 262.67 | 0.9505 | -518.6 | -277.6 | |
| 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. | |