SDO HMI 2014-08-13 06:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.00 | 35.90 | 11.93 | 32.81 | -18.60 | 160.60 | 52.02 | 242.81 | 0.8420 | 286.1 | 295.3 | |
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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 |
| 3.16 | 9.02 | 2.98 | 8.49 | -16.26 | 162.83 | 54.26 | 246.30 | 0.8530 | 496.6 | 456.3 | |
| 1.90 | -1.00 | 1.78 | -1.00 | -16.39 | 162.56 | 53.98 | 246.05 | 0.8512 | 590.3 | 999999 | |
| 0.00 | 1.26 | 0.00 | 1.17 | -16.98 | 161.83 | 53.25 | 245.13 | 0.8468 | 303.0 | 267.7 | |
| 0.00 | 0.90 | 0.00 | 0.86 | -18.41 | 162.39 | 53.82 | 243.75 | 0.8560 | 470.0 | 384.5 | |
| 2.71 | 4.60 | 2.48 | 4.22 | -19.13 | 160.58 | 52.01 | 242.24 | 0.8435 | 607.8 | 516.8 | |
| 0.00 | 0.27 | 0.00 | 0.24 | -18.02 | 160.05 | 51.48 | 243.25 | 0.8352 | 461.0 | 383.0 | |
| 1.62 | 3.34 | 1.49 | 3.06 | -19.48 | 160.42 | 51.85 | 241.78 | 0.8434 | 499.0 | 407.3 | |
| 0.00 | 2.62 | 0.00 | 2.38 | -19.13 | 160.16 | 51.58 | 242.07 | 0.8400 | 787.0 | 733.1 | |
| 0.00 | 1.71 | 0.00 | 1.55 | -19.24 | 159.95 | 51.37 | 241.86 | 0.8386 | 672.0 | 574.1 | |
| 0.00 | 2.71 | 0.00 | 2.46 | -19.48 | 160.00 | 51.43 | 241.61 | 0.8399 | 630.0 | 504.3 | |
| 0.00 | 1.62 | 0.00 | 1.45 | -19.59 | 159.07 | 50.50 | 241.09 | 0.8325 | -406.0 | -302.7 | |
| 0.00 | 1.17 | 0.00 | 1.02 | -18.61 | 158.51 | 49.94 | 241.94 | 0.8241 | -487.0 | -358.3 | |
| 2.89 | 4.60 | 2.56 | 4.08 | -20.39 | 158.61 | 50.03 | 240.00 | 0.8317 | -453.7 | -200.9 | |
| 0.72 | 2.08 | 0.64 | 1.83 | -20.55 | 158.17 | 49.60 | 239.63 | 0.8287 | -542.4 | -482.5 | |
| 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. | |