SDO HMI 2014-10-04 16:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.52 | 0.00 | 11.03 | -18.21 | 102.28 | -34.08 | 127.39 | 0.6699 | -102.8 | -115.3 | |
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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 | 1.41 | 0.00 | 0.87 | -22.66 | 113.38 | -22.98 | 143.08 | 0.6020 | 624.0 | 558.4 | |
| 0.00 | 1.32 | 0.00 | 0.84 | -22.53 | 110.48 | -25.89 | 139.69 | 0.6256 | 403.0 | 396.1 | |
| 0.00 | 0.97 | 0.00 | 0.59 | -17.03 | 108.52 | -27.84 | 130.93 | 0.5933 | 663.0 | 553.9 | |
| 0.00 | 1.49 | 0.00 | 0.92 | -16.88 | 108.33 | -28.03 | 130.54 | 0.5940 | 668.0 | 553.0 | |
| 0.00 | 1.41 | 0.00 | 0.87 | -15.08 | 105.76 | -30.60 | 125.70 | 0.6075 | 695.0 | 577.4 | |
| 0.00 | 0.35 | 0.00 | 0.24 | -17.70 | 98.99 | -37.37 | 123.88 | 0.6988 | -501.0 | -422.2 | |
| 0.00 | 1.49 | 0.00 | 1.03 | -17.27 | 99.06 | -37.30 | 123.39 | 0.6955 | -684.0 | -632.8 | |
| 0.00 | 1.41 | 0.00 | 0.97 | -17.54 | 98.91 | -37.45 | 123.63 | 0.6987 | -722.0 | -668.4 | |
| 0.00 | 2.11 | 0.00 | 1.46 | -17.53 | 98.64 | -37.72 | 123.43 | 0.7014 | -651.0 | -562.6 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -17.76 | 98.18 | -38.18 | 123.41 | 0.7076 | -221.0 | -307.3 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -17.66 | 98.17 | -38.20 | 123.28 | 0.7071 | -489.0 | -505.0 | |
| 0.00 | 1.32 | 0.00 | 0.94 | -18.95 | 97.66 | -38.70 | 124.51 | 0.7200 | -124.0 | -201.1 | |
| 0.00 | 1.49 | 0.00 | 1.04 | -16.86 | 98.00 | -38.36 | 122.17 | 0.7040 | -595.0 | -465.5 | |
| 0.00 | 1.23 | 0.00 | 0.90 | -19.06 | 95.77 | -40.59 | 123.44 | 0.7393 | -505.0 | -429.3 | |
| 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. | |