SDO HMI 2014-08-19 08:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.92 | 98.33 | 25.76 | 93.87 | -9.52 | 331.57 | -56.60 | 105.54 | 0.8564 | 586.6 | 259.2 | |
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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 | 1.17 | 0.00 | 0.98 | -10.15 | 337.13 | -51.04 | 107.99 | 0.8069 | 489.0 | 383.3 | |
| 0.00 | 2.25 | 0.00 | 1.86 | -9.32 | 337.26 | -50.91 | 107.04 | 0.8033 | 685.0 | 539.8 | |
| 0.00 | 1.44 | 0.00 | 1.26 | -7.14 | 334.29 | -53.87 | 103.53 | 0.8265 | 456.0 | 341.8 | |
| 22.15 | 70.24 | 21.08 | 66.79 | -9.52 | 331.67 | -56.50 | 105.56 | 0.8557 | 753.9 | 285.1 | |
| 0.00 | 2.61 | 0.00 | 2.54 | -9.87 | 331.01 | -57.16 | 105.77 | 0.8621 | -330.0 | -272.6 | |
| 0.00 | 1.71 | 0.00 | 1.72 | -11.22 | 330.20 | -57.97 | 107.05 | 0.8717 | 319.0 | 237.2 | |
| 4.77 | 12.52 | 4.68 | 12.33 | -9.38 | 330.57 | -57.60 | 105.10 | 0.8648 | 532.5 | 237.8 | |
| 0.00 | 2.25 | 0.00 | 2.20 | -9.16 | 330.57 | -57.60 | 104.85 | 0.8644 | 553.0 | 447.4 | |
| 0.00 | 2.25 | 0.00 | 2.21 | -9.02 | 330.43 | -57.74 | 104.65 | 0.8652 | 537.0 | 436.3 | |
| 0.00 | 0.81 | 0.00 | 0.84 | -11.12 | 328.98 | -59.19 | 106.60 | 0.8813 | -277.0 | -260.1 | |
| 0.00 | 1.08 | 0.00 | 1.14 | -10.94 | 328.61 | -59.56 | 106.30 | 0.8838 | -426.0 | -399.0 | |
| 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. | |