SDO HMI 2014-11-27 09:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.83 | 47.26 | 17.13 | 43.56 | -23.74 | 94.79 | -53.33 | 119.52 | 0.8457 | 192.3 | -151.7 | |
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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 | 0.94 | 0.00 | 0.85 | -24.67 | 96.09 | -52.03 | 121.01 | 0.8380 | 466.0 | 398.5 | |
| 2.48 | 24.91 | 2.24 | 22.45 | -24.44 | 96.01 | -52.11 | 120.72 | 0.8379 | 733.0 | 283.3 | |
| 8.56 | -2.00 | 7.73 | -2.00 | -24.18 | 95.90 | -52.22 | 120.39 | 0.8380 | 659.3 | 999999 | |
| 5.05 | -2.00 | 4.56 | -2.00 | -23.83 | 95.73 | -52.39 | 119.92 | 0.8383 | 249.3 | 999999 | |
| 0.00 | 1.46 | 0.00 | 1.33 | -24.20 | 95.30 | -52.82 | 120.19 | 0.8429 | 131.0 | 28.1 | |
| 0.00 | 1.03 | 0.00 | 0.96 | -24.05 | 94.30 | -53.82 | 119.69 | 0.8506 | -435.0 | -420.2 | |
| 0.00 | 0.43 | 0.00 | 0.39 | -23.10 | 94.81 | -53.31 | 118.78 | 0.8437 | 275.0 | 216.2 | |
| 0.00 | 1.28 | 0.00 | 1.20 | -23.86 | 94.36 | -53.76 | 119.49 | 0.8495 | -545.0 | -349.1 | |
| 0.00 | 0.86 | 0.00 | 0.81 | -24.22 | 93.86 | -54.26 | 119.73 | 0.8546 | 485.0 | 400.8 | |
| 2.74 | 9.93 | 2.60 | 9.39 | -23.16 | 93.51 | -54.61 | 118.43 | 0.8544 | -662.7 | -548.1 | |
| 0.00 | 1.71 | 0.00 | 1.63 | -22.77 | 93.30 | -54.82 | 117.93 | 0.8551 | -509.0 | -487.5 | |
| 0.00 | 0.26 | 0.00 | 0.25 | -22.84 | 92.97 | -55.15 | 117.91 | 0.8579 | -473.0 | -497.3 | |
| 0.00 | 4.45 | 0.00 | 4.30 | -23.08 | 92.66 | -55.46 | 118.07 | 0.8610 | -521.0 | -368.1 | |
| 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. | |