SDO HMI 2011-10-16 14:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 126.98 | 693.59 | 66.44 | 362.88 | -12.19 | 49.08 | 4.59 | 194.01 | 0.3234 | -29.9 | -91.8 | |
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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 |
| 21.82 | 265.55 | 11.47 | 139.50 | -11.79 | 53.12 | 8.63 | 206.04 | 0.3362 | 1214.4 | 381.4 | |
| 27.23 | -1.00 | 14.29 | -1.00 | -11.81 | 52.44 | 7.96 | 204.21 | 0.3318 | 1286.1 | 999999 | |
| 12.39 | 22.43 | 6.48 | 11.73 | -11.85 | 50.78 | 6.30 | 199.54 | 0.3222 | 1103.6 | 600.0 | |
| 0.00 | 1.13 | 0.00 | 0.61 | -15.56 | 50.88 | 6.40 | 196.46 | 0.3805 | 698.0 | 560.8 | |
| 0.00 | 3.49 | 0.00 | 1.83 | -12.70 | 50.58 | 6.10 | 198.14 | 0.3344 | 676.0 | 597.2 | |
| 0.00 | 2.44 | 0.00 | 1.27 | -11.41 | 50.40 | 5.92 | 198.91 | 0.3132 | 911.0 | 709.6 | |
| 0.00 | 0.70 | 0.00 | 0.36 | -12.24 | 48.12 | 3.64 | 191.34 | 0.3166 | -816.0 | -601.8 | |
| 0.00 | 1.31 | 0.00 | 0.69 | -14.51 | 47.57 | 3.08 | 188.54 | 0.3521 | -674.0 | -556.9 | |
| 2.09 | 393.58 | 1.09 | 205.33 | -11.98 | 47.11 | 2.62 | 188.35 | 0.3096 | -957.0 | -434.8 | |
| 13.70 | -9.00 | 7.18 | -9.00 | -13.11 | 46.84 | 2.36 | 187.06 | 0.3276 | -1064.5 | 999999 | |
| 3.49 | -9.00 | 1.82 | -9.00 | -12.42 | 46.74 | 2.26 | 187.03 | 0.3160 | -1014.0 | 999999 | |
| 22.08 | -9.00 | 11.50 | -9.00 | -12.07 | 46.50 | 2.01 | 186.39 | 0.3098 | -1414.1 | 999999 | |
| 14.14 | -9.00 | 7.38 | -9.00 | -12.61 | 46.44 | 1.95 | 186.03 | 0.3185 | -1068.8 | 999999 | |
| 10.04 | -9.00 | 5.23 | -9.00 | -12.26 | 45.98 | 1.49 | 184.70 | 0.3120 | -1166.0 | 999999 | |
| 0.00 | 1.83 | 0.00 | 0.97 | -14.82 | 43.55 | -0.93 | 177.44 | 0.3538 | -920.0 | -735.9 | |
| 0.00 | 1.13 | 0.00 | 0.59 | -11.70 | 42.80 | -1.68 | 174.53 | 0.3029 | -752.0 | -606.1 | |
| 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. | |