SDO HMI 2014-09-06 01:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.12 | 234.83 | 49.02 | 195.22 | -19.54 | 107.24 | -46.96 | 120.95 | 0.8052 | 746.6 | 329.7 | |
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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 |
| 0.63 | 8.75 | 0.53 | 7.48 | -22.55 | 107.55 | -46.65 | 124.43 | 0.8165 | 738.0 | 512.9 | |
| 0.27 | -1.00 | 0.23 | -1.00 | -22.45 | 107.50 | -46.71 | 124.30 | 0.8165 | 721.7 | 999999 | |
| 0.00 | 1.88 | 0.00 | 1.53 | -19.90 | 108.31 | -45.89 | 121.90 | 0.7975 | 609.0 | 572.7 | |
| 0.00 | 0.89 | 0.00 | 0.73 | -19.60 | 107.91 | -46.29 | 121.36 | 0.7997 | 430.0 | 428.2 | |
| 23.93 | 89.56 | 19.40 | 72.36 | -18.71 | 108.14 | -46.06 | 120.47 | 0.7935 | 932.9 | 482.3 | |
| 9.82 | 37.32 | 8.29 | 31.41 | -20.65 | 107.12 | -47.08 | 122.13 | 0.8114 | 703.2 | 362.0 | |
| 9.47 | 89.20 | 7.98 | 75.17 | -20.04 | 106.79 | -47.41 | 121.29 | 0.8115 | 865.9 | 220.4 | |
| 10.98 | -7.00 | 9.23 | -7.00 | -19.67 | 106.80 | -47.41 | 120.88 | 0.8098 | 870.4 | 999999 | |
| 4.02 | -7.00 | 3.36 | -7.00 | -19.11 | 106.73 | -47.47 | 120.21 | 0.8080 | 708.4 | 999999 | |
| 0.00 | 0.80 | 0.00 | 0.70 | -18.00 | 104.24 | -49.96 | 117.80 | 0.8252 | -279.0 | -195.6 | |
| 0.00 | 1.61 | 0.00 | 1.45 | -18.09 | 102.75 | -51.46 | 117.24 | 0.8383 | -599.0 | -538.7 | |
| 0.00 | 3.21 | 0.00 | 2.88 | -17.35 | 102.84 | -51.36 | 116.46 | 0.8350 | -443.0 | -342.1 | |
| 0.00 | 1.61 | 0.00 | 1.51 | -18.09 | 101.12 | -53.08 | 116.58 | 0.8518 | -424.0 | -316.0 | |
| 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. | |