SDO HMI 2014-05-26 21:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.25 | 85.81 | 39.98 | 140.53 | -14.27 | 137.56 | 71.93 | 255.42 | 0.9527 | 211.1 | 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 | 1.44 | 0.00 | 2.70 | -14.15 | 140.15 | 74.52 | 255.68 | 0.9656 | -350.0 | -335.2 | |
| 0.00 | 2.07 | 0.00 | 3.88 | -14.34 | 140.09 | 74.46 | 255.49 | 0.9653 | -389.0 | -366.2 | |
| 4.33 | 50.67 | 7.78 | 89.36 | -14.39 | 139.43 | 73.80 | 255.41 | 0.9624 | -10.6 | 109.5 | |
| 13.98 | -3.00 | 23.97 | -3.00 | -14.40 | 138.66 | 73.03 | 255.35 | 0.9588 | 644.4 | 999999 | |
| 0.00 | 0.63 | 0.00 | 1.06 | -14.98 | 138.18 | 72.55 | 254.72 | 0.9566 | 450.0 | 405.3 | |
| 0.00 | 1.35 | 0.00 | 1.99 | -13.96 | 135.62 | 69.99 | 255.63 | 0.9427 | 34.0 | 129.7 | |
| 0.00 | 1.98 | 0.00 | 2.88 | -13.75 | 135.38 | 69.75 | 255.84 | 0.9413 | -442.0 | -212.0 | |
| 2.34 | 4.06 | 3.28 | 5.68 | -13.45 | 134.56 | 68.93 | 256.11 | 0.9364 | -294.5 | -144.2 | |
| 1.26 | 12.26 | 1.80 | 17.72 | -14.48 | 134.97 | 69.33 | 255.04 | 0.9392 | -135.7 | 131.9 | |
| 0.00 | 0.99 | 0.00 | 1.36 | -13.21 | 134.15 | 68.52 | 256.34 | 0.9338 | -361.0 | -321.8 | |
| 0.00 | 1.53 | 0.00 | 2.11 | -13.43 | 134.20 | 68.56 | 256.11 | 0.9342 | -383.0 | -332.4 | |
| 1.26 | 2.52 | 1.71 | 3.43 | -13.65 | 133.90 | 68.27 | 255.84 | 0.9325 | -367.1 | -282.9 | |
| 0.00 | 0.63 | 0.00 | 0.84 | -13.38 | 133.40 | 67.77 | 256.10 | 0.9293 | -436.0 | -350.4 | |
| 1.08 | 4.69 | 1.44 | 6.25 | -13.69 | 133.50 | 67.87 | 255.77 | 0.9301 | -547.5 | -366.7 | |
| 0.00 | 0.99 | 0.00 | 1.27 | -14.25 | 132.36 | 66.73 | 255.08 | 0.9231 | -520.0 | -473.3 | |
| 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. | |