SDO HMI 2014-05-29 22:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.36 | 181.86 | 12.69 | 91.08 | -9.09 | 24.94 | -0.44 | 177.64 | 0.1459 | 875.8 | 433.5 | |
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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 |
| 25.36 | 159.76 | 12.69 | 79.95 | -9.04 | 25.51 | 0.13 | 180.90 | 0.1414 | 1309.3 | 446.8 | |
| 0.00 | 1.08 | 0.00 | 0.54 | -10.64 | 24.33 | -1.05 | 173.90 | 0.1700 | 821.0 | 611.2 | |
| 0.00 | 2.53 | 0.00 | 1.26 | -8.86 | 23.48 | -1.90 | 166.59 | 0.1420 | 671.0 | 636.0 | |
| 0.00 | 1.90 | 0.00 | 0.95 | -9.38 | 23.26 | -2.12 | 166.01 | 0.1516 | 1094.0 | 919.3 | |
| 0.00 | 2.89 | 0.00 | 1.45 | -9.68 | 23.17 | -2.21 | 165.91 | 0.1572 | 763.0 | 764.7 | |
| 0.00 | 1.62 | 0.00 | 0.81 | -9.50 | 23.08 | -2.31 | 165.05 | 0.1545 | 1056.0 | 894.2 | |
| 0.00 | 1.53 | 0.00 | 0.77 | -10.11 | 23.01 | -2.37 | 165.64 | 0.1651 | 708.0 | 652.6 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -9.81 | 22.98 | -2.40 | 164.99 | 0.1601 | 896.0 | 669.0 | |
| 0.00 | 1.08 | 0.00 | 0.54 | -9.96 | 22.95 | -2.43 | 165.05 | 0.1628 | 850.0 | 757.2 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -14.10 | 20.05 | -5.33 | 158.39 | 0.2458 | 874.0 | 730.8 | |
| 0.00 | 2.08 | 0.00 | 1.04 | -8.85 | 20.12 | -5.26 | 146.61 | 0.1653 | -948.0 | -717.7 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -8.26 | 19.30 | -6.08 | 140.53 | 0.1657 | -850.0 | -645.6 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -2.22 | 15.40 | -9.98 | 97.33 | 0.1753 | 939.0 | 745.8 | |
| 0.00 | 2.53 | 0.00 | 1.31 | -11.90 | 12.99 | -12.39 | 132.19 | 0.2846 | -991.0 | -794.3 | |
| 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. | |