SDO HMI 2014-05-26 07:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.11 | 193.83 | 92.09 | 435.03 | -18.71 | 150.13 | 76.78 | 251.05 | 0.9733 | 56.1 | -15.3 | |
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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 |
| 0.00 | 3.16 | 0.00 | 8.30 | -17.42 | 152.34 | 78.99 | 252.52 | 0.9828 | 343.0 | 296.0 | |
| 12.00 | 75.41 | 36.31 | 233.64 | -18.44 | 153.84 | 80.49 | 251.53 | 0.9872 | 79.7 | -15.1 | |
| 0.00 | 2.16 | 0.00 | 5.34 | -17.50 | 151.64 | 78.29 | 252.41 | 0.9806 | 402.0 | 362.9 | |
| 0.00 | 4.06 | 0.00 | 8.37 | -17.23 | 149.23 | 75.88 | 252.58 | 0.9718 | 408.0 | 321.1 | |
| 0.00 | 1.53 | 0.00 | 3.16 | -17.52 | 149.20 | 75.85 | 252.28 | 0.9718 | -363.0 | -200.9 | |
| 0.00 | 0.63 | 0.00 | 1.31 | -17.64 | 149.36 | 76.00 | 252.16 | 0.9724 | 49.0 | -52.1 | |
| 0.00 | 1.08 | 0.00 | 1.90 | -17.54 | 146.66 | 73.31 | 252.11 | 0.9610 | 119.0 | 169.8 | |
| 3.70 | 30.85 | 6.20 | 51.60 | -17.47 | 145.71 | 72.35 | 252.12 | 0.9564 | -317.4 | -248.8 | |
| 3.16 | -8.00 | 5.23 | -8.00 | -17.76 | 145.57 | 72.22 | 251.81 | 0.9559 | -305.6 | 999999 | |
| 1.17 | -8.00 | 1.92 | -8.00 | -17.96 | 145.24 | 71.89 | 251.58 | 0.9543 | -391.2 | 999999 | |
| 2.62 | 5.05 | 4.44 | 8.57 | -19.97 | 145.82 | 72.47 | 249.52 | 0.9579 | -298.2 | -144.1 | |
| 11.01 | 31.39 | 17.57 | 50.38 | -19.28 | 144.64 | 71.29 | 250.14 | 0.9519 | 424.5 | 325.1 | |
| 0.00 | 1.35 | 0.00 | 2.09 | -18.68 | 144.04 | 70.69 | 250.72 | 0.9485 | 546.0 | 521.6 | |
| 3.61 | 20.75 | 5.89 | 33.53 | -20.15 | 144.96 | 71.61 | 249.26 | 0.9539 | -614.8 | -451.6 | |
| 8.84 | 15.24 | 14.53 | 25.05 | -21.22 | 145.03 | 71.68 | 248.15 | 0.9548 | 191.2 | 130.9 | |
| 0.00 | 1.17 | 0.00 | 1.79 | -20.11 | 143.61 | 70.26 | 249.18 | 0.9470 | 239.0 | 264.0 | |
| 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. | |