SDO HMI 2014-09-13 01:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.78 | 22.06 | 1.47 | 17.44 | -20.16 | 105.62 | 43.86 | 236.62 | 0.7799 | 77.9 | 90.9 | |
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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 |
| 0.98 | 3.20 | 0.84 | 2.76 | -19.87 | 110.31 | 48.55 | 239.47 | 0.8205 | 468.3 | 298.5 | |
| 0.00 | 2.05 | 0.00 | 1.74 | -21.95 | 108.53 | 46.77 | 236.29 | 0.8146 | 16.0 | 67.7 | |
| 0.00 | 1.16 | 0.00 | 0.95 | -20.71 | 107.28 | 45.51 | 236.99 | 0.7980 | 517.0 | 469.6 | |
| 0.00 | 1.33 | 0.00 | 1.10 | -21.27 | 107.17 | 45.41 | 236.31 | 0.7998 | 567.0 | 468.7 | |
| 0.00 | 0.27 | 0.00 | 0.21 | -19.22 | 105.65 | 43.89 | 237.80 | 0.7759 | 586.0 | 543.3 | |
| 0.80 | 3.38 | 0.63 | 2.67 | -19.83 | 105.82 | 44.05 | 237.18 | 0.7806 | 681.3 | 537.9 | |
| 0.00 | 0.44 | 0.00 | 0.35 | -20.33 | 105.72 | 43.96 | 236.57 | 0.7822 | 463.0 | 472.6 | |
| 0.00 | 1.69 | 0.00 | 1.33 | -20.51 | 105.47 | 43.71 | 236.23 | 0.7809 | 497.0 | 497.1 | |
| 0.00 | 0.89 | 0.00 | 0.69 | -20.42 | 104.91 | 43.15 | 236.00 | 0.7753 | 676.0 | 537.1 | |
| 0.00 | 0.89 | 0.00 | 0.65 | -17.01 | 102.45 | 40.69 | 238.53 | 0.7332 | -530.0 | -463.8 | |
| 0.00 | 1.42 | 0.00 | 1.06 | -19.12 | 102.79 | 41.03 | 236.23 | 0.7485 | -435.0 | -382.9 | |
| 0.00 | 0.80 | 0.00 | 0.59 | -19.07 | 102.61 | 40.85 | 236.17 | 0.7464 | -409.0 | -434.7 | |
| 0.00 | 2.31 | 0.00 | 1.70 | -19.12 | 102.03 | 40.27 | 235.75 | 0.7412 | -546.0 | -518.6 | |
| 0.00 | 1.16 | 0.00 | 0.85 | -18.84 | 101.87 | 40.11 | 235.97 | 0.7379 | -773.0 | -565.2 | |
| 0.00 | 1.07 | 0.00 | 0.79 | -24.04 | 99.29 | 37.53 | 228.32 | 0.7473 | -325.0 | -358.9 | |
| 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. | |