SDO HMI 2014-01-12 20:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.50 | 0.00 | 10.90 | -23.26 | 56.96 | 23.32 | 224.27 | 0.5321 | -436.0 | -380.2 | |
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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 | 0.67 | -10.87 | 74.44 | 40.80 | 258.36 | 0.6575 | -539.0 | -480.8 | |
| 0.00 | 1.02 | 0.00 | 0.66 | -7.92 | 73.99 | 40.34 | 262.83 | 0.6486 | -595.0 | -499.1 | |
| 0.00 | 0.85 | 0.00 | 0.56 | -21.03 | 72.81 | 39.16 | 242.75 | 0.6654 | 813.0 | 650.3 | |
| 0.00 | 2.12 | 0.00 | 1.39 | -22.98 | 71.03 | 37.39 | 239.11 | 0.6537 | 554.0 | 423.8 | |
| 0.00 | 0.59 | 0.00 | 0.37 | -15.37 | 68.75 | 35.10 | 249.70 | 0.5934 | -520.0 | -457.0 | |
| 0.00 | 1.19 | 0.00 | 0.70 | -16.55 | 65.03 | 31.39 | 245.98 | 0.5488 | -503.0 | -495.4 | |
| 0.00 | 1.02 | 0.00 | 0.57 | -18.96 | 58.14 | 24.49 | 236.51 | 0.4721 | -770.0 | -681.5 | |
| 0.00 | 1.10 | 0.00 | 0.62 | -25.78 | 53.10 | 19.45 | 219.03 | 0.4782 | -650.0 | -554.8 | |
| 0.00 | 3.23 | 0.00 | 1.79 | -24.60 | 51.88 | 18.23 | 219.08 | 0.4532 | -718.0 | -688.6 | |
| 0.00 | 1.78 | 0.00 | 1.04 | -33.31 | 47.53 | 13.88 | 202.39 | 0.5284 | -571.0 | -395.3 | |
| 0.00 | 1.10 | 0.00 | 0.62 | -30.56 | 45.81 | 12.17 | 202.24 | 0.4815 | -665.0 | -604.4 | |
| 0.00 | 1.27 | 0.00 | 0.67 | -23.80 | 39.49 | 5.84 | 195.57 | 0.3483 | -795.0 | -585.1 | |
| 0.00 | 2.21 | 0.00 | 1.24 | -32.02 | 39.10 | 5.46 | 189.83 | 0.4742 | -709.0 | -631.5 | |
| 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. | |