SDO HMI 2014-10-05 02:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.76 | 30.56 | 6.47 | 19.95 | 14.24 | 90.59 | -40.26 | 75.75 | 0.6479 | 269.0 | 157.0 | |
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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 | 0.70 | 0.00 | 0.41 | 10.61 | 99.85 | -30.99 | 80.23 | 0.5156 | -676.0 | -476.2 | |
| 0.00 | 1.05 | 0.00 | 0.61 | 12.60 | 99.28 | -31.56 | 76.55 | 0.5273 | -737.0 | -517.5 | |
| 0.00 | 1.05 | 0.00 | 0.62 | 12.47 | 98.98 | -31.87 | 76.89 | 0.5314 | -834.0 | -677.8 | |
| 0.00 | 1.93 | 0.00 | 1.15 | 14.38 | 97.51 | -33.33 | 73.80 | 0.5565 | -751.0 | -615.4 | |
| 0.00 | 1.67 | 0.00 | 0.99 | 7.86 | 97.10 | -33.74 | 85.62 | 0.5540 | -764.0 | -639.8 | |
| 0.00 | 1.58 | 0.00 | 1.01 | 23.24 | 93.75 | -37.10 | 60.88 | 0.6367 | 757.0 | 623.4 | |
| 0.00 | 1.14 | 0.00 | 0.70 | 12.39 | 95.32 | -35.52 | 77.79 | 0.5828 | -660.0 | -472.5 | |
| 0.00 | 0.70 | 0.00 | 0.47 | 16.29 | 89.38 | -41.47 | 72.80 | 0.6677 | 630.0 | 526.9 | |
| 9.76 | 15.56 | 6.47 | 10.31 | 13.24 | 89.09 | -41.76 | 77.40 | 0.6666 | 875.7 | 550.9 | |
| 0.00 | 1.05 | 0.00 | 0.70 | 13.37 | 88.77 | -42.07 | 77.25 | 0.6707 | 419.0 | 376.8 | |
| 0.00 | 1.41 | 0.00 | 0.96 | 15.01 | 87.07 | -43.77 | 75.08 | 0.6938 | 541.0 | 507.8 | |
| 0.00 | 0.79 | 0.00 | 0.55 | 14.58 | 86.66 | -44.18 | 75.76 | 0.6982 | 558.0 | 490.0 | |
| 0.00 | 1.49 | 0.00 | 1.12 | 22.14 | 82.91 | -47.93 | 66.16 | 0.7540 | 580.0 | 487.6 | |
| 0.00 | 0.44 | 0.00 | 0.35 | 20.32 | 79.91 | -50.93 | 69.12 | 0.7815 | 508.0 | 437.8 | |
| 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. | |