SDO HMI 2011-11-28 10:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.53 | 89.55 | 31.11 | 128.77 | 7.63 | 129.84 | -69.90 | 82.33 | 0.9401 | -139.4 | -113.0 | |
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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 |
| 10.18 | 61.32 | 13.84 | 83.26 | 7.52 | 131.08 | -68.66 | 82.41 | 0.9331 | -576.2 | -232.9 | |
| 0.94 | -1.00 | 1.30 | -1.00 | 7.49 | 130.75 | -68.98 | 82.46 | 0.9351 | 149.6 | 999999 | |
| 0.00 | 1.03 | 0.00 | 1.42 | 6.86 | 130.71 | -69.02 | 83.13 | 0.9353 | 42.0 | 28.2 | |
| 0.00 | 2.65 | 0.00 | 3.80 | 7.23 | 129.98 | -69.75 | 82.75 | 0.9397 | -176.0 | -123.1 | |
| 0.00 | 0.43 | 0.00 | 0.60 | 5.66 | 130.21 | -69.52 | 84.43 | 0.9382 | -370.0 | -393.2 | |
| 0.00 | 0.86 | 0.00 | 1.26 | 7.16 | 129.30 | -70.43 | 82.85 | 0.9437 | -291.0 | -220.4 | |
| 0.00 | 2.14 | 0.00 | 3.26 | 7.87 | 128.75 | -70.98 | 82.11 | 0.9469 | 18.0 | -27.5 | |
| 2.14 | 3.16 | 3.21 | 4.76 | 6.91 | 128.93 | -70.80 | 83.12 | 0.9458 | -188.5 | 50.9 | |
| 1.03 | 2.22 | 1.60 | 3.47 | 8.13 | 128.27 | -71.46 | 81.85 | 0.9496 | 91.8 | -64.4 | |
| 0.00 | 4.62 | 0.00 | 7.36 | 8.48 | 127.82 | -71.91 | 81.49 | 0.9520 | 627.0 | 456.6 | |
| 0.00 | 1.37 | 0.00 | 2.19 | 8.20 | 127.75 | -71.98 | 81.78 | 0.9524 | 425.0 | 363.6 | |
| 2.05 | 3.25 | 3.57 | 5.64 | 8.18 | 126.33 | -73.40 | 81.84 | 0.9596 | 499.8 | 467.6 | |
| 2.91 | 6.50 | 5.24 | 11.75 | 7.95 | 125.68 | -74.05 | 82.09 | 0.9626 | 226.4 | 186.9 | |
| 1.28 | -13.00 | 2.35 | -13.00 | 8.04 | 125.42 | -74.32 | 82.00 | 0.9639 | -136.5 | 999999 | |
| 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. | |