SDO HMI 2014-09-26 20:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.76 | 0.00 | 9.84 | 7.24 | 207.06 | -32.66 | 87.43 | 0.5379 | 343.9 | 170.6 | |
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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 | 1.41 | 0.00 | 0.80 | 6.64 | 210.47 | -29.25 | 88.77 | 0.4875 | -809.0 | -688.4 | |
| 0.00 | 0.35 | 0.00 | 0.20 | 6.43 | 210.48 | -29.24 | 89.20 | 0.4874 | -788.0 | -735.8 | |
| 0.00 | 3.62 | 0.00 | 2.08 | 6.31 | 208.98 | -30.73 | 89.30 | 0.5100 | -825.0 | -622.4 | |
| 0.00 | 0.97 | 0.00 | 0.57 | 5.39 | 206.76 | -32.96 | 90.78 | 0.5438 | 641.0 | 516.5 | |
| 0.00 | 0.53 | 0.00 | 0.31 | 7.36 | 206.51 | -33.21 | 87.13 | 0.5459 | 543.0 | 589.5 | |
| 0.00 | 1.06 | 0.00 | 0.63 | 7.49 | 206.28 | -33.44 | 86.87 | 0.5492 | 755.0 | 582.9 | |
| 0.00 | 0.79 | 0.00 | 0.47 | 8.06 | 206.20 | -33.52 | 85.83 | 0.5504 | 977.0 | 870.6 | |
| 0.00 | 1.06 | 0.00 | 0.63 | 8.21 | 206.15 | -33.57 | 85.56 | 0.5511 | 868.0 | 733.6 | |
| 0.00 | 0.44 | 0.00 | 0.26 | 8.08 | 206.01 | -33.71 | 85.80 | 0.5531 | 520.0 | 439.4 | |
| 0.00 | 0.79 | 0.00 | 0.47 | 7.65 | 205.94 | -33.78 | 86.57 | 0.5541 | 523.0 | 455.8 | |
| 0.00 | 1.68 | 0.00 | 1.00 | 7.44 | 205.89 | -33.83 | 86.95 | 0.5550 | 701.0 | 485.7 | |
| 0.00 | 1.24 | 0.00 | 0.74 | 6.92 | 205.75 | -33.97 | 87.89 | 0.5572 | 424.0 | 381.8 | |
| 0.00 | 1.41 | 0.00 | 0.84 | 8.98 | 205.56 | -34.16 | 84.17 | 0.5597 | 686.0 | 597.9 | |
| 0.00 | 1.41 | 0.00 | 0.84 | 7.95 | 205.40 | -34.32 | 86.02 | 0.5619 | 598.0 | 424.6 | |
| 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. | |