SDO HMI 2014-11-06 21:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.34 | 0.00 | 8.60 | -23.06 | 78.04 | 19.70 | 215.09 | 0.5644 | 491.8 | 367.5 | |
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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 |
| 0.00 | 1.73 | 0.00 | 1.11 | -27.05 | 84.34 | 25.99 | 217.60 | 0.6421 | -735.0 | -536.7 | |
| 0.00 | 1.73 | 0.00 | 1.03 | -19.79 | 82.62 | 24.27 | 224.42 | 0.5547 | 789.0 | 715.2 | |
| 0.00 | 1.21 | 0.00 | 0.72 | -20.43 | 82.51 | 24.17 | 223.44 | 0.5601 | 786.0 | 674.9 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -19.81 | 82.38 | 24.03 | 224.11 | 0.5526 | 783.0 | 711.1 | |
| 0.00 | 0.78 | 0.00 | 0.47 | -21.60 | 82.26 | 23.91 | 221.65 | 0.5693 | 672.0 | 477.6 | |
| 0.00 | 0.78 | 0.00 | 0.46 | -20.77 | 80.53 | 22.18 | 220.64 | 0.5441 | 675.0 | 566.7 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -21.22 | 80.39 | 22.04 | 219.90 | 0.5476 | 559.0 | 488.3 | |
| 0.00 | 1.38 | 0.00 | 0.81 | -21.05 | 80.23 | 21.88 | 219.90 | 0.5443 | 810.0 | 680.4 | |
| 0.00 | 1.81 | 0.00 | 1.04 | -21.22 | 76.35 | 18.00 | 214.45 | 0.5113 | 762.0 | 507.5 | |
| 0.00 | 1.12 | 0.00 | 0.66 | -23.70 | 76.45 | 18.10 | 211.80 | 0.5420 | 753.0 | 582.5 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -21.92 | 75.57 | 17.22 | 212.48 | 0.5134 | 608.0 | 506.5 | |
| 0.00 | 1.04 | 0.00 | 0.68 | -36.35 | 49.87 | -8.48 | 169.55 | 0.6575 | -561.0 | -483.4 | |
| 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. | |