SDO HMI 2014-06-01 00:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.53 | 36.93 | 9.89 | 20.75 | -9.08 | 24.68 | 26.87 | 251.71 | 0.4720 | 634.1 | 535.2 | |
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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 | 1.90 | 0.00 | 1.08 | -8.59 | 26.61 | 28.80 | 253.76 | 0.4982 | 779.0 | 607.4 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -8.80 | 26.63 | 28.82 | 253.35 | 0.4992 | 631.0 | 481.9 | |
| 17.53 | 23.85 | 9.89 | 13.46 | -8.78 | 25.37 | 27.56 | 252.76 | 0.4807 | 970.7 | 730.8 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -9.92 | 24.56 | 26.76 | 249.99 | 0.4739 | 415.0 | 443.0 | |
| 0.00 | 3.52 | 0.00 | 1.97 | -9.98 | 23.95 | 26.14 | 249.46 | 0.4652 | 881.0 | 733.5 | |
| 0.00 | 1.81 | 0.00 | 1.01 | -10.05 | 23.57 | 25.77 | 249.08 | 0.4601 | 847.0 | 668.0 | |
| 0.00 | 0.63 | 0.00 | 0.35 | -10.11 | 22.22 | 24.41 | 247.97 | 0.4407 | 757.0 | 569.9 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -9.13 | 21.06 | 23.26 | 249.26 | 0.4186 | -657.0 | -585.3 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -14.12 | 20.45 | 22.64 | 238.03 | 0.4419 | 774.0 | 507.5 | |
| 0.00 | 0.36 | 0.00 | 0.19 | -5.38 | 17.94 | 20.13 | 256.49 | 0.3539 | -734.0 | -643.8 | |
| 0.00 | 0.90 | 0.00 | 0.47 | -6.85 | 16.31 | 18.50 | 251.12 | 0.3344 | -681.0 | -487.3 | |
| 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. | |