SDO HMI 2014-01-09 07:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.37 | 16.01 | 0.70 | 8.59 | -18.72 | 66.54 | -13.76 | 144.52 | 0.3561 | -478.2 | -343.1 | |
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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 | 0.85 | 0.00 | 0.43 | -13.80 | 80.07 | -0.22 | 178.75 | 0.1718 | -809.0 | -599.9 | |
| 0.00 | 1.28 | 0.00 | 0.64 | -14.48 | 78.46 | -1.83 | 170.37 | 0.1862 | -885.0 | -705.4 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -19.85 | 74.56 | -5.73 | 161.11 | 0.2912 | 794.0 | 624.8 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -18.14 | 74.25 | -6.04 | 157.83 | 0.2663 | 898.0 | 646.0 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -17.80 | 74.14 | -6.15 | 156.94 | 0.2618 | 1058.0 | 861.2 | |
| 0.43 | 3.91 | 0.22 | 2.01 | -18.19 | 73.00 | -7.29 | 153.93 | 0.2756 | -1095.4 | -835.7 | |
| 0.94 | -6.00 | 0.48 | -6.00 | -18.28 | 72.84 | -7.45 | 153.59 | 0.2782 | -1015.3 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.44 | -15.12 | 69.29 | -11.01 | 136.61 | 0.2695 | -876.0 | -620.3 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -2.82 | 63.01 | -17.28 | 86.79 | 0.2985 | -784.0 | -652.9 | |
| 0.00 | 0.34 | 0.00 | 0.20 | -23.94 | 53.38 | -26.91 | 130.13 | 0.5432 | -720.0 | -729.0 | |
| 0.00 | 0.94 | 0.00 | 0.55 | -24.44 | 53.27 | -27.03 | 130.79 | 0.5485 | -782.0 | -631.6 | |
| 0.00 | 1.02 | 0.00 | 0.60 | -23.99 | 53.01 | -27.29 | 129.86 | 0.5478 | -766.0 | -520.2 | |
| 0.00 | 1.28 | 0.00 | 0.75 | -23.80 | 52.83 | -27.46 | 129.41 | 0.5482 | -765.0 | -636.1 | |
| 0.00 | 0.77 | 0.00 | 0.52 | -30.70 | 44.90 | -35.39 | 132.79 | 0.6810 | -553.0 | -440.4 | |
| 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. | |