SDO HMI 2014-09-07 16:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.82 | 34.15 | 9.47 | 33.07 | -20.65 | 79.54 | -53.22 | 119.31 | 0.8609 | 210.9 | 82.5 | |
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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 | 2.76 | 0.00 | 2.49 | -20.63 | 82.48 | -50.28 | 120.55 | 0.8380 | 642.0 | 565.5 | |
| 1.25 | 2.50 | 1.14 | 2.28 | -20.58 | 81.94 | -50.82 | 120.26 | 0.8422 | 311.7 | 246.7 | |
| 0.54 | 2.14 | 0.49 | 1.94 | -20.27 | 82.08 | -50.68 | 119.98 | 0.8398 | 620.0 | 516.6 | |
| 0.00 | 0.80 | 0.00 | 0.70 | -17.85 | 82.65 | -50.11 | 117.55 | 0.8259 | 520.0 | 419.8 | |
| 0.00 | 1.25 | 0.00 | 1.16 | -20.73 | 81.19 | -51.56 | 120.08 | 0.8487 | 473.0 | 361.7 | |
| 0.00 | 1.07 | 0.00 | 1.01 | -21.27 | 80.88 | -51.88 | 120.53 | 0.8532 | 557.0 | 532.2 | |
| 0.62 | 2.76 | 0.60 | 2.66 | -21.38 | 80.13 | -52.63 | 120.32 | 0.8594 | 605.1 | 487.2 | |
| 3.57 | 5.35 | 3.42 | 5.14 | -20.98 | 80.06 | -52.70 | 119.87 | 0.8585 | 387.0 | 216.8 | |
| 0.00 | 1.16 | 0.00 | 1.13 | -21.43 | 79.67 | -53.09 | 120.18 | 0.8630 | 230.0 | 238.8 | |
| 0.00 | 0.98 | 0.00 | 1.06 | -24.08 | 76.96 | -55.80 | 121.87 | 0.8910 | 413.0 | 344.6 | |
| 0.00 | 1.34 | 0.00 | 1.30 | -19.98 | 79.05 | -53.71 | 118.37 | 0.8629 | -623.0 | -607.9 | |
| 3.84 | 10.70 | 3.82 | 10.63 | -19.91 | 78.15 | -54.61 | 117.94 | 0.8696 | -440.4 | -490.7 | |
| 0.00 | 1.34 | 0.00 | 1.57 | -22.34 | 73.52 | -59.24 | 118.79 | 0.9086 | 400.0 | 239.0 | |
| 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. | |