SDO HMI 2014-01-12 09:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.76 | 0.00 | 11.58 | -19.88 | 66.30 | 26.61 | 234.28 | 0.5260 | -417.4 | -248.9 | |
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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 | 1.45 | 0.00 | 0.95 | -12.63 | 80.28 | 40.59 | 255.62 | 0.6577 | -572.0 | -479.2 | |
| 0.00 | 1.45 | 0.00 | 0.99 | -19.20 | 81.68 | 41.98 | 246.43 | 0.6916 | 695.0 | 501.9 | |
| 0.00 | 0.94 | 0.00 | 0.60 | -11.57 | 79.15 | 39.45 | 257.00 | 0.6412 | -607.0 | -495.1 | |
| 0.00 | 1.19 | 0.00 | 0.73 | -21.25 | 72.64 | 32.94 | 239.12 | 0.5928 | 652.0 | 575.2 | |
| 0.00 | 0.77 | 0.00 | 0.44 | -14.32 | 69.75 | 30.05 | 249.22 | 0.5211 | -653.0 | -573.0 | |
| 0.00 | 3.15 | 0.00 | 1.92 | -23.18 | 70.99 | 31.29 | 235.03 | 0.5849 | 550.0 | 483.8 | |
| 0.00 | 1.11 | 0.00 | 0.62 | -16.31 | 65.12 | 25.42 | 242.40 | 0.4669 | -708.0 | -601.3 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -17.70 | 63.11 | 23.41 | 237.85 | 0.4490 | -743.0 | -544.0 | |
| 0.00 | 2.38 | 0.00 | 1.31 | -17.13 | 62.76 | 23.07 | 238.64 | 0.4404 | -883.0 | -701.9 | |
| 0.00 | 1.62 | 0.00 | 0.87 | -18.70 | 58.34 | 18.65 | 230.15 | 0.3962 | -764.0 | -623.4 | |
| 0.00 | 1.53 | 0.00 | 0.83 | -19.03 | 58.35 | 18.65 | 229.48 | 0.3995 | -808.0 | -688.6 | |
| 0.00 | 0.68 | 0.00 | 0.38 | -30.78 | 51.98 | 12.28 | 202.20 | 0.4856 | -703.0 | -630.2 | |
| 0.00 | 1.02 | 0.00 | 0.58 | -33.06 | 47.60 | 7.91 | 193.45 | 0.4978 | -540.0 | -536.3 | |
| 0.00 | 1.02 | 0.00 | 0.56 | -29.12 | 42.03 | 2.33 | 184.84 | 0.4235 | -759.0 | -581.9 | |
| 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. | |