SDO HMI 2014-11-27 08:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.18 | 42.21 | 14.88 | 39.28 | -23.81 | 94.96 | -53.70 | 119.47 | 0.8489 | 124.2 | -122.4 | |
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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 |
| 14.55 | 26.79 | 13.32 | 24.49 | -24.16 | 95.81 | -52.85 | 120.14 | 0.8431 | 511.8 | 199.0 | |
| 0.00 | 0.86 | 0.00 | 0.80 | -24.18 | 95.15 | -53.51 | 119.93 | 0.8485 | 116.0 | 148.2 | |
| 0.00 | 1.20 | 0.00 | 1.12 | -23.83 | 94.71 | -53.96 | 119.39 | 0.8511 | -186.0 | -170.6 | |
| 0.00 | 0.77 | 0.00 | 0.73 | -23.77 | 94.41 | -54.26 | 119.23 | 0.8533 | -265.0 | -247.4 | |
| 0.00 | 0.43 | 0.00 | 0.40 | -23.64 | 94.43 | -54.23 | 119.09 | 0.8527 | -26.0 | -63.4 | |
| 0.00 | 2.65 | 0.00 | 2.53 | -23.23 | 93.79 | -54.88 | 118.42 | 0.8567 | -431.0 | -519.4 | |
| 1.63 | 3.60 | 1.56 | 3.46 | -23.14 | 93.45 | -55.22 | 118.22 | 0.8592 | -674.8 | -596.1 | |
| 0.00 | 1.63 | 0.00 | 1.57 | -22.78 | 93.27 | -55.39 | 117.77 | 0.8597 | -555.0 | -434.8 | |
| 0.00 | 1.54 | 0.00 | 1.49 | -22.82 | 93.02 | -55.65 | 117.73 | 0.8618 | -556.0 | -483.8 | |
| 0.00 | 2.48 | 0.00 | 2.43 | -23.05 | 92.76 | -55.91 | 117.92 | 0.8644 | -517.0 | -406.2 | |
| 0.00 | 0.26 | 0.00 | 0.26 | -23.67 | 91.35 | -57.32 | 118.18 | 0.8766 | -378.0 | -359.7 | |
| 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. | |