SDO HMI 2014-11-28 20:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.11 | 15.90 | 0.73 | 10.66 | -23.15 | 93.40 | -35.49 | 127.51 | 0.6746 | -12.2 | -93.5 | |
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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 |
| 0.68 | 2.05 | 0.44 | 1.31 | -23.32 | 97.63 | -31.27 | 130.85 | 0.6324 | 855.4 | 715.4 | |
| 0.00 | 1.11 | 0.00 | 0.71 | -23.10 | 96.74 | -32.15 | 129.84 | 0.6399 | 683.0 | 539.2 | |
| 0.00 | 0.68 | 0.00 | 0.45 | -23.35 | 95.01 | -33.88 | 128.84 | 0.6594 | 591.0 | 547.5 | |
| 0.00 | 1.03 | 0.00 | 0.68 | -23.90 | 94.73 | -34.16 | 129.35 | 0.6662 | 483.0 | 441.9 | |
| 0.00 | 0.94 | 0.00 | 0.62 | -23.61 | 94.74 | -34.15 | 128.98 | 0.6641 | 335.0 | 431.5 | |
| 0.43 | 1.71 | 0.29 | 1.15 | -24.05 | 93.38 | -35.51 | 128.57 | 0.6808 | -749.6 | -658.9 | |
| 0.00 | 0.60 | 0.00 | 0.40 | -22.52 | 93.38 | -35.51 | 126.61 | 0.6708 | -558.0 | -473.1 | |
| 0.00 | 1.11 | 0.00 | 0.76 | -24.48 | 92.72 | -36.18 | 128.66 | 0.6903 | -597.0 | -461.1 | |
| 0.00 | 1.45 | 0.00 | 0.96 | -21.14 | 93.54 | -35.35 | 124.90 | 0.6603 | -671.0 | -541.9 | |
| 0.00 | 1.97 | 0.00 | 1.31 | -20.55 | 92.45 | -36.44 | 123.39 | 0.6685 | -309.0 | -326.7 | |
| 0.00 | 3.25 | 0.00 | 2.31 | -24.23 | 89.64 | -39.26 | 126.38 | 0.7191 | -365.0 | -303.2 | |
| 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. | |