SDO HMI 2014-04-13 11:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.40 | 414.14 | 30.37 | 215.53 | 11.44 | 274.77 | -4.77 | 15.36 | 0.3075 | -975.4 | -422.5 | |
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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 |
| 58.40 | 398.40 | 30.37 | 207.16 | 11.36 | 274.96 | -4.58 | 14.92 | 0.3052 | -1505.0 | -454.9 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 10.35 | 273.04 | -6.50 | 21.94 | 0.2992 | 615.0 | 498.8 | |
| 0.00 | 1.59 | 0.00 | 0.84 | 13.73 | 272.53 | -7.01 | 19.63 | 0.3546 | -738.0 | -651.1 | |
| 0.00 | 0.80 | 0.00 | 0.41 | 8.06 | 272.17 | -7.37 | 28.14 | 0.2706 | -794.0 | -661.3 | |
| 0.00 | 0.71 | 0.00 | 0.37 | 13.39 | 271.67 | -7.87 | 22.19 | 0.3544 | -544.0 | -446.6 | |
| 0.00 | 1.24 | 0.00 | 0.64 | 9.12 | 271.69 | -7.85 | 27.85 | 0.2901 | -790.0 | -598.1 | |
| 0.00 | 0.62 | 0.00 | 0.33 | 13.10 | 270.46 | -9.08 | 25.55 | 0.3580 | 700.0 | 577.0 | |
| 0.00 | 0.62 | 0.00 | 0.33 | 15.74 | 269.53 | -10.01 | 24.65 | 0.4029 | 599.0 | 561.9 | |
| 0.00 | 1.24 | 0.00 | 0.66 | 14.49 | 269.49 | -10.05 | 26.15 | 0.3850 | 949.0 | 752.4 | |
| 0.00 | 2.56 | 0.00 | 1.37 | 13.88 | 269.52 | -10.02 | 26.82 | 0.3761 | 587.0 | 595.9 | |
| 0.00 | 1.15 | 0.00 | 0.61 | 12.54 | 268.35 | -11.19 | 31.29 | 0.3663 | 781.0 | 601.2 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 14.26 | 268.11 | -11.43 | 29.46 | 0.3921 | 711.0 | 530.7 | |
| 0.00 | 0.97 | 0.00 | 0.54 | 18.39 | 267.77 | -11.77 | 25.45 | 0.4522 | 619.0 | 482.6 | |
| 0.00 | 1.94 | 0.00 | 1.05 | 14.81 | 267.93 | -11.61 | 29.16 | 0.4012 | 707.0 | 592.8 | |
| 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. | |