SDO HMI 2014-12-01 09:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.73 | 24.53 | 4.90 | 23.14 | -15.17 | 38.75 | -56.65 | 108.57 | 0.8514 | 182.5 | -80.6 | |
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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 |
| 2.65 | 9.23 | 2.26 | 7.90 | -16.32 | 42.89 | -52.51 | 110.83 | 0.8169 | 811.0 | 532.9 | |
| 3.08 | -1.00 | 2.64 | -1.00 | -16.48 | 42.78 | -52.62 | 110.99 | 0.8184 | 683.2 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.84 | -15.48 | 40.72 | -54.68 | 109.29 | 0.8353 | 496.0 | 409.4 | |
| 0.00 | 1.03 | 0.00 | 0.94 | -15.89 | 40.01 | -55.39 | 109.61 | 0.8424 | 439.0 | 389.8 | |
| 0.00 | 1.03 | 0.00 | 0.94 | -15.34 | 39.75 | -55.65 | 108.90 | 0.8438 | 543.0 | 401.5 | |
| 0.00 | 0.85 | 0.00 | 0.84 | -15.25 | 37.30 | -58.10 | 108.28 | 0.8647 | 336.0 | 298.7 | |
| 0.00 | 1.54 | 0.00 | 1.48 | -14.05 | 37.75 | -57.65 | 106.99 | 0.8590 | 333.0 | 259.1 | |
| 0.00 | 0.51 | 0.00 | 0.52 | -14.65 | 36.32 | -59.08 | 107.41 | 0.8719 | -532.0 | -544.8 | |
| 0.00 | 4.44 | 0.00 | 4.59 | -15.40 | 35.49 | -59.91 | 108.10 | 0.8796 | -672.0 | -531.4 | |
| 0.00 | 0.26 | 0.00 | 0.26 | -14.63 | 35.85 | -59.55 | 107.30 | 0.8757 | -418.0 | -443.0 | |
| 0.00 | 1.11 | 0.00 | 1.13 | -14.38 | 35.90 | -59.50 | 107.03 | 0.8749 | -540.0 | -485.6 | |
| 0.00 | 2.74 | 0.00 | 2.81 | -12.71 | 35.26 | -60.14 | 105.03 | 0.8780 | -554.0 | -458.8 | |
| 0.00 | 0.85 | 0.00 | 0.89 | -12.83 | 34.96 | -60.44 | 105.13 | 0.8805 | -165.0 | -125.3 | |
| 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. | |