SDO HMI 2014-01-12 01:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.32 | 0.00 | 9.70 | -19.46 | 65.39 | 21.33 | 230.17 | 0.4601 | -430.7 | -322.2 | |
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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 | 1.53 | 0.00 | 0.94 | -12.30 | 79.65 | 35.59 | 254.87 | 0.5912 | -699.0 | -608.2 | |
| 0.00 | 1.02 | 0.00 | 0.60 | -19.33 | 74.37 | 30.31 | 240.46 | 0.5496 | 379.0 | 388.6 | |
| 0.00 | 0.93 | 0.00 | 0.53 | -14.57 | 72.63 | 28.57 | 247.89 | 0.5017 | -721.0 | -575.7 | |
| 0.00 | 2.21 | 0.00 | 1.30 | -21.40 | 72.38 | 28.32 | 235.52 | 0.5379 | 566.0 | 417.7 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -23.29 | 70.80 | 26.74 | 231.09 | 0.5333 | 711.0 | 563.7 | |
| 0.00 | 2.55 | 0.00 | 1.38 | -15.53 | 65.43 | 21.37 | 240.24 | 0.4062 | -827.0 | -678.1 | |
| 0.00 | 1.10 | 0.00 | 0.60 | -15.06 | 64.96 | 20.90 | 240.80 | 0.3963 | -697.0 | -468.5 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -16.95 | 62.74 | 18.68 | 233.85 | 0.3810 | -694.0 | -547.3 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -17.08 | 62.56 | 18.49 | 233.32 | 0.3798 | -606.0 | -588.2 | |
| 0.00 | 1.70 | 0.00 | 0.89 | -18.01 | 58.23 | 14.16 | 224.10 | 0.3359 | -701.0 | -675.3 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -24.95 | 52.02 | 7.96 | 199.52 | 0.3775 | -815.0 | -633.9 | |
| 0.00 | 1.44 | 0.00 | 0.81 | -30.81 | 52.19 | 8.12 | 195.16 | 0.4661 | -747.0 | -601.2 | |
| 0.00 | 0.68 | 0.00 | 0.37 | -29.43 | 42.40 | -1.66 | 176.61 | 0.4282 | -748.0 | -621.2 | |
| 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. | |