SDO HMI 2014-03-09 23:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.78 | 30.67 | 0.39 | 15.26 | -11.10 | 13.68 | -0.86 | 176.78 | 0.0847 | 291.6 | 141.8 | |
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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 | 1.13 | 0.00 | 0.56 | -9.43 | 19.37 | 4.83 | 245.11 | 0.0920 | 955.0 | 831.4 | |
| 0.00 | 1.56 | 0.00 | 0.77 | -9.12 | 17.56 | 3.01 | 237.73 | 0.0617 | 1006.0 | 810.2 | |
| 0.00 | 2.77 | 0.00 | 1.38 | -9.99 | 16.50 | 1.96 | 215.20 | 0.0588 | 990.0 | 777.8 | |
| 0.78 | 3.46 | 0.39 | 1.72 | -10.91 | 16.05 | 1.51 | 202.08 | 0.0693 | 1116.9 | 951.3 | |
| 0.00 | 2.25 | 0.00 | 1.12 | -10.23 | 16.02 | 1.48 | 206.07 | 0.0581 | 792.0 | 628.2 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -11.48 | 15.27 | 0.73 | 189.55 | 0.0751 | 574.0 | 542.5 | |
| 0.00 | 3.90 | 0.00 | 1.93 | -10.73 | 15.08 | 0.54 | 188.71 | 0.0618 | 922.0 | 809.6 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -11.27 | 15.05 | 0.51 | 187.14 | 0.0710 | 914.0 | 705.4 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -11.85 | 10.92 | -3.62 | 142.44 | 0.1019 | -1029.0 | -818.0 | |
| 0.00 | 1.39 | 0.00 | 0.69 | -8.57 | 10.69 | -3.85 | 109.33 | 0.0707 | 977.0 | 766.8 | |
| 0.00 | 5.89 | 0.00 | 2.94 | -12.20 | 10.52 | -4.02 | 141.63 | 0.1110 | -633.0 | -844.4 | |
| 0.00 | 1.99 | 0.00 | 0.99 | -12.47 | 10.42 | -4.12 | 142.46 | 0.1157 | -1083.0 | -892.4 | |
| 0.00 | 1.82 | 0.00 | 0.91 | -12.68 | 10.32 | -4.22 | 142.93 | 0.1195 | -937.0 | -815.7 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -13.12 | 9.49 | -5.05 | 140.14 | 0.1344 | -804.0 | -656.9 | |
| 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. | |