SDO HMI 2014-08-14 14:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.47 | 40.00 | 11.08 | 51.62 | 16.06 | 22.66 | -68.30 | 75.30 | 0.9241 | 136.7 | 33.7 | |
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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 | 4.51 | 0.00 | 5.14 | 16.53 | 25.89 | -65.07 | 74.80 | 0.9026 | -585.0 | -472.7 | |
| 0.00 | 1.62 | 0.00 | 1.88 | 16.77 | 25.43 | -65.53 | 74.54 | 0.9059 | -503.0 | -427.4 | |
| 0.00 | 1.17 | 0.00 | 1.37 | 16.67 | 25.11 | -65.85 | 74.65 | 0.9082 | -380.0 | -300.6 | |
| 0.72 | 2.25 | 0.85 | 2.65 | 16.17 | 25.12 | -65.83 | 75.20 | 0.9081 | -235.8 | -104.9 | |
| 0.00 | 0.99 | 0.00 | 1.19 | 16.79 | 24.47 | -66.49 | 74.52 | 0.9127 | -57.0 | -63.7 | |
| 0.00 | 3.07 | 0.00 | 3.71 | 17.03 | 24.30 | -66.66 | 74.26 | 0.9138 | -205.0 | -51.2 | |
| 0.00 | 1.44 | 0.00 | 1.73 | 15.44 | 24.49 | -66.47 | 76.00 | 0.9125 | -224.0 | -163.0 | |
| 0.00 | 1.35 | 0.00 | 1.63 | 15.59 | 24.39 | -66.57 | 75.84 | 0.9132 | 327.0 | 259.5 | |
| 0.90 | 2.34 | 1.13 | 2.94 | 16.58 | 23.30 | -67.66 | 74.76 | 0.9205 | -229.2 | -130.3 | |
| 5.59 | 8.47 | 7.26 | 11.02 | 15.45 | 22.48 | -68.48 | 75.97 | 0.9258 | 474.5 | 281.6 | |
| 0.00 | 2.70 | 0.00 | 3.86 | 16.32 | 20.25 | -70.70 | 75.00 | 0.9392 | 414.0 | 364.2 | |
| 0.00 | 2.43 | 0.00 | 3.46 | 15.86 | 20.35 | -70.61 | 75.49 | 0.9388 | 494.0 | 453.0 | |
| 0.00 | 2.34 | 0.00 | 3.29 | 15.23 | 20.65 | -70.31 | 76.17 | 0.9371 | 388.0 | 310.8 | |
| 1.26 | 3.79 | 1.84 | 5.53 | 16.23 | 19.74 | -71.22 | 75.08 | 0.9422 | 173.2 | 127.5 | |
| 0.00 | 1.53 | 0.00 | 2.22 | 15.72 | 19.97 | -70.99 | 75.63 | 0.9409 | 45.0 | 18.1 | |
| 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. | |