SDO HMI 2014-05-30 04:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.12 | 29.96 | 6.25 | 18.05 | -19.54 | 51.42 | 29.35 | 234.29 | 0.5672 | 306.4 | 116.0 | |
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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 | 0.27 | 0.00 | 0.18 | -22.83 | 58.31 | 36.25 | 235.38 | 0.6644 | 595.0 | 575.7 | |
| 0.00 | 0.99 | 0.00 | 0.63 | -19.63 | 55.96 | 33.89 | 238.37 | 0.6191 | 609.0 | 480.5 | |
| 4.97 | 14.54 | 3.07 | 8.98 | -19.51 | 54.39 | 32.32 | 237.48 | 0.5999 | 794.2 | 614.2 | |
| 5.15 | -3.00 | 3.18 | -3.00 | -19.67 | 54.31 | 32.25 | 237.18 | 0.6000 | 802.8 | 999999 | |
| 0.00 | 3.07 | 0.00 | 1.88 | -19.07 | 53.69 | 31.62 | 237.65 | 0.5887 | 863.0 | 673.4 | |
| 0.00 | 0.63 | 0.00 | 0.41 | -26.07 | 55.34 | 33.27 | 229.06 | 0.6547 | -517.0 | -454.0 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -14.80 | 52.57 | 30.50 | 243.73 | 0.5494 | 746.0 | 591.5 | |
| 0.00 | 1.17 | 0.00 | 0.70 | -17.07 | 52.84 | 30.77 | 240.17 | 0.5660 | 650.0 | 470.9 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -16.29 | 49.94 | 27.87 | 239.24 | 0.5243 | 429.0 | 457.8 | |
| 0.00 | 2.44 | 0.00 | 1.42 | -19.58 | 48.62 | 26.55 | 232.62 | 0.5320 | -980.0 | -814.7 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -20.47 | 44.39 | 22.32 | 226.65 | 0.4913 | -637.0 | -528.5 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -22.03 | 42.49 | 20.42 | 221.83 | 0.4869 | -750.0 | -662.9 | |
| 0.00 | 2.62 | 0.00 | 1.41 | -20.79 | 34.57 | 12.50 | 210.74 | 0.3977 | -714.0 | -651.7 | |
| 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. | |