SDO HMI 2014-07-09 20:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.60 | 162.84 | 36.75 | 195.15 | -11.97 | 267.84 | 64.02 | 255.00 | 0.9120 | -19.1 | -89.1 | |
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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 | 1.27 | 0.00 | 1.68 | -12.36 | 270.28 | 66.45 | 255.04 | 0.9285 | 379.0 | 395.6 | |
| 14.80 | 78.07 | 18.61 | 98.53 | -10.57 | 269.38 | 65.56 | 256.80 | 0.9209 | 577.8 | 126.9 | |
| 0.91 | -2.00 | 1.15 | -2.00 | -11.02 | 269.50 | 65.67 | 256.34 | 0.9221 | 364.7 | 999999 | |
| 0.00 | 1.09 | 0.00 | 1.23 | -8.32 | 266.74 | 62.91 | 258.82 | 0.8998 | 535.0 | 501.9 | |
| 0.00 | 0.82 | 0.00 | 0.98 | -12.09 | 267.96 | 64.14 | 254.92 | 0.9130 | 214.0 | 212.3 | |
| 0.00 | 0.54 | 0.00 | 0.66 | -12.21 | 267.95 | 64.12 | 254.78 | 0.9130 | 285.0 | 242.8 | |
| 0.00 | 1.27 | 0.00 | 1.41 | -8.51 | 266.25 | 62.42 | 258.53 | 0.8963 | 423.0 | 358.1 | |
| 0.00 | 1.09 | 0.00 | 1.30 | -13.94 | 267.34 | 63.51 | 252.79 | 0.9111 | -376.0 | -214.5 | |
| 14.89 | 73.89 | 16.99 | 84.00 | -13.46 | 266.20 | 62.38 | 253.08 | 0.9024 | -753.9 | -370.2 | |
| 0.00 | 1.45 | 0.00 | 1.69 | -14.28 | 266.52 | 62.70 | 252.27 | 0.9059 | -154.0 | -171.7 | |
| 0.00 | 1.54 | 0.00 | 1.74 | -15.02 | 265.59 | 61.77 | 251.26 | 0.9004 | -278.0 | -178.8 | |
| 0.00 | 1.54 | 0.00 | 1.67 | -15.83 | 264.22 | 60.40 | 250.05 | 0.8917 | -486.0 | -383.4 | |
| 0.00 | 0.27 | 0.00 | 0.26 | -10.32 | 261.52 | 57.70 | 255.60 | 0.8605 | 201.0 | 269.7 | |
| 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. | |