SDO HMI 2014-09-07 18:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.37 | 36.92 | 8.76 | 34.64 | -20.46 | 79.63 | -52.02 | 119.62 | 0.8511 | 174.0 | 41.4 | |
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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 |
| 0.89 | 3.48 | 0.78 | 3.06 | -20.61 | 82.54 | -49.11 | 121.07 | 0.8283 | 664.7 | 512.9 | |
| 1.16 | 2.32 | 1.03 | 2.06 | -20.63 | 81.98 | -49.67 | 120.84 | 0.8331 | 245.7 | 211.8 | |
| 0.00 | 1.78 | 0.00 | 1.58 | -20.31 | 82.12 | -49.53 | 120.55 | 0.8306 | 621.0 | 537.2 | |
| 0.00 | 1.34 | 0.00 | 1.14 | -17.76 | 82.71 | -48.94 | 117.98 | 0.8153 | 167.0 | 269.1 | |
| 0.00 | 1.07 | 0.00 | 0.98 | -21.20 | 81.00 | -50.65 | 121.01 | 0.8432 | 604.0 | 456.6 | |
| 0.00 | 1.16 | 0.00 | 1.05 | -20.75 | 81.17 | -50.48 | 120.59 | 0.8402 | 468.0 | 338.6 | |
| 0.00 | 1.43 | 0.00 | 1.34 | -21.39 | 80.13 | -51.52 | 120.82 | 0.8509 | 620.0 | 523.6 | |
| 0.00 | 1.25 | 0.00 | 1.17 | -21.31 | 79.96 | -51.69 | 120.66 | 0.8519 | 540.0 | 429.5 | |
| 0.00 | 0.80 | 0.00 | 0.76 | -21.45 | 79.89 | -51.76 | 120.78 | 0.8529 | 222.0 | 212.1 | |
| 3.57 | 5.26 | 3.33 | 4.91 | -20.96 | 80.09 | -51.57 | 120.33 | 0.8496 | 398.7 | 169.1 | |
| 0.00 | 1.25 | 0.00 | 1.18 | -21.41 | 79.65 | -52.00 | 120.63 | 0.8547 | 285.0 | 204.6 | |
| 0.00 | 2.23 | 0.00 | 2.11 | -19.92 | 79.06 | -52.60 | 118.77 | 0.8541 | -555.0 | -541.1 | |
| 3.75 | 10.97 | 3.62 | 10.58 | -19.89 | 78.16 | -53.49 | 118.36 | 0.8610 | -520.7 | -463.0 | |
| 0.00 | 0.80 | 0.00 | 0.83 | -22.02 | 76.45 | -55.20 | 119.95 | 0.8806 | 299.0 | 273.6 | |
| 0.00 | 0.89 | 0.00 | 0.88 | -19.18 | 77.25 | -54.41 | 117.24 | 0.8658 | -275.0 | -283.5 | |
| 0.00 | 0.89 | 0.00 | 1.01 | -22.34 | 73.56 | -58.09 | 119.19 | 0.9013 | 402.0 | 234.6 | |
| 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. | |