SDO HMI 2014-04-06 08:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.85 | 22.35 | 0.92 | 11.16 | -8.34 | 7.50 | -6.08 | 113.82 | 0.1181 | -142.7 | -148.5 | |
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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 |
| 0.00 | 1.23 | 0.00 | 0.61 | -8.93 | 12.25 | -1.33 | 154.08 | 0.0525 | 919.0 | 759.9 | |
| 0.00 | 1.58 | 0.00 | 0.79 | -7.15 | 11.20 | -2.38 | 111.40 | 0.0444 | 993.0 | 757.8 | |
| 0.00 | 0.79 | 0.00 | 0.39 | -7.36 | 10.66 | -2.92 | 111.36 | 0.0545 | 864.0 | 737.0 | |
| 0.00 | 2.20 | 0.00 | 1.09 | -10.21 | 10.23 | -3.35 | 140.43 | 0.0906 | 995.0 | 821.1 | |
| 1.85 | 3.26 | 0.92 | 1.62 | -9.73 | 9.99 | -3.58 | 134.77 | 0.0872 | 1097.3 | 848.4 | |
| 0.00 | 1.23 | 0.00 | 0.62 | -14.03 | 6.61 | -6.97 | 139.21 | 0.1810 | 828.0 | 669.6 | |
| 0.00 | 1.23 | 0.00 | 0.62 | -7.55 | 6.00 | -7.57 | 100.35 | 0.1334 | -915.0 | -609.4 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -6.73 | 5.71 | -7.86 | 94.10 | 0.1369 | -1062.0 | -792.6 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -7.27 | 5.43 | -8.15 | 97.75 | 0.1426 | -934.0 | -826.7 | |
| 0.00 | 3.35 | 0.00 | 1.67 | -6.97 | 5.28 | -8.30 | 95.55 | 0.1446 | -814.0 | -805.7 | |
| 0.00 | 1.23 | 0.00 | 0.62 | -7.35 | 5.15 | -8.43 | 98.11 | 0.1475 | -1023.0 | -928.5 | |
| 0.00 | 1.14 | 0.00 | 0.57 | -7.23 | 4.88 | -8.70 | 97.07 | 0.1519 | -1018.0 | -867.0 | |
| 0.00 | 1.50 | 0.00 | 0.75 | -7.56 | 4.84 | -8.74 | 99.19 | 0.1532 | -947.0 | -748.9 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -7.44 | 4.72 | -8.86 | 98.30 | 0.1550 | -882.0 | -727.8 | |
| 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. | |