SDO HMI 2014-09-07 14:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.30 | 35.22 | 8.19 | 35.02 | -20.48 | 79.58 | -54.28 | 118.71 | 0.8683 | 104.1 | 48.7 | |
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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 | 0.71 | 0.00 | 0.62 | -18.60 | 84.53 | -49.33 | 118.74 | 0.8220 | 440.0 | 407.8 | |
| 0.80 | 4.28 | 0.74 | 3.96 | -20.61 | 82.55 | -51.31 | 120.06 | 0.8462 | 561.7 | 428.6 | |
| 1.52 | 2.85 | 1.42 | 2.68 | -20.54 | 81.90 | -51.96 | 119.70 | 0.8512 | 240.2 | 204.0 | |
| 0.00 | 1.96 | 0.00 | 1.83 | -20.26 | 82.04 | -51.82 | 119.46 | 0.8491 | 542.0 | 497.9 | |
| 0.00 | 0.80 | 0.00 | 0.72 | -17.93 | 82.65 | -51.21 | 117.16 | 0.8357 | 440.0 | 385.7 | |
| 0.00 | 1.61 | 0.00 | 1.55 | -21.24 | 80.96 | -52.90 | 120.06 | 0.8610 | 494.0 | 347.2 | |
| 0.00 | 0.62 | 0.00 | 0.60 | -20.71 | 81.18 | -52.68 | 119.59 | 0.8575 | 338.0 | 307.4 | |
| 0.00 | 2.14 | 0.00 | 2.12 | -21.41 | 80.05 | -53.81 | 119.86 | 0.8684 | 588.0 | 481.0 | |
| 2.77 | 4.73 | 2.73 | 4.67 | -21.00 | 80.05 | -53.81 | 119.43 | 0.8671 | 348.4 | 213.9 | |
| 0.00 | 1.34 | 0.00 | 1.34 | -20.00 | 79.08 | -54.78 | 117.96 | 0.8712 | -540.0 | -505.7 | |
| 0.00 | 0.27 | 0.00 | 0.27 | -20.19 | 78.86 | -55.00 | 118.08 | 0.8734 | -478.0 | -481.7 | |
| 0.00 | 0.71 | 0.00 | 0.73 | -20.56 | 78.55 | -55.31 | 118.36 | 0.8768 | -348.0 | -284.4 | |
| 3.21 | 10.35 | 3.30 | 10.59 | -19.93 | 78.15 | -55.71 | 117.53 | 0.8779 | -393.4 | -449.9 | |
| 0.00 | 0.80 | 0.00 | 0.84 | -19.09 | 77.09 | -56.77 | 116.24 | 0.8832 | -254.0 | -258.6 | |
| 0.00 | 2.05 | 0.00 | 2.50 | -22.37 | 73.54 | -60.32 | 118.44 | 0.9155 | 366.0 | 234.7 | |
| 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. | |