SDO HMI 2014-04-14 21:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.36 | 407.74 | 33.98 | 218.48 | 11.78 | 274.84 | 14.02 | 321.49 | 0.3822 | -948.0 | -369.3 | |
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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 |
| 63.36 | 385.75 | 33.98 | 206.84 | 11.71 | 275.19 | 14.37 | 320.57 | 0.3841 | -1392.6 | -429.4 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 9.95 | 273.56 | 12.74 | 320.83 | 0.3453 | -860.0 | -692.4 | |
| 0.00 | 1.06 | 0.00 | 0.57 | 13.96 | 272.11 | 11.29 | 330.35 | 0.3857 | -759.0 | -639.1 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 15.45 | 271.18 | 10.35 | 334.21 | 0.3998 | -634.0 | -497.1 | |
| 0.00 | 1.41 | 0.00 | 0.75 | 12.92 | 270.59 | 9.76 | 332.46 | 0.3591 | 822.0 | 635.7 | |
| 0.00 | 3.18 | 0.00 | 1.69 | 13.07 | 270.22 | 9.39 | 333.55 | 0.3586 | 927.0 | 731.3 | |
| 0.00 | 1.59 | 0.00 | 0.84 | 13.12 | 269.63 | 8.80 | 335.07 | 0.3552 | 1000.0 | 887.7 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 14.71 | 268.94 | 8.11 | 338.53 | 0.3745 | 811.0 | 674.7 | |
| 0.00 | 1.33 | 0.00 | 0.71 | 14.80 | 268.16 | 7.33 | 340.51 | 0.3713 | 743.0 | 591.9 | |
| 0.00 | 1.86 | 0.00 | 0.99 | 14.44 | 268.11 | 7.29 | 340.28 | 0.3657 | 905.0 | 703.9 | |
| 0.00 | 1.94 | 0.00 | 1.03 | 13.64 | 267.80 | 6.98 | 340.29 | 0.3517 | 854.0 | 652.6 | |
| 0.00 | 6.98 | 0.00 | 3.64 | 11.76 | 265.99 | 5.17 | 343.56 | 0.3128 | 872.0 | 676.3 | |
| 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. | |