SDO HMI 2014-09-03 02:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.84 | 0.00 | 10.12 | 9.66 | 182.42 | -10.85 | 80.01 | 0.1988 | -432.1 | -367.5 | |
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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 | 1.25 | 0.00 | 0.62 | 3.92 | 189.53 | -3.75 | 131.41 | 0.0873 | -863.0 | -595.1 | |
| 0.00 | 3.04 | 0.00 | 1.51 | 5.16 | 189.22 | -4.05 | 116.97 | 0.0794 | -846.0 | -633.2 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 11.66 | 186.27 | -7.00 | 56.77 | 0.1433 | -754.0 | -632.7 | |
| 0.00 | 1.61 | 0.00 | 0.81 | 11.78 | 185.87 | -7.41 | 57.53 | 0.1503 | -1068.0 | -946.5 | |
| 0.00 | 1.25 | 0.00 | 0.63 | 11.59 | 185.78 | -7.50 | 58.88 | 0.1500 | -922.0 | -714.5 | |
| 0.00 | 1.07 | 0.00 | 0.54 | 12.38 | 185.48 | -7.80 | 55.56 | 0.1614 | -874.0 | -686.8 | |
| 0.00 | 1.70 | 0.00 | 0.85 | 11.07 | 185.36 | -7.92 | 63.24 | 0.1521 | -982.0 | -786.1 | |
| 0.00 | 1.52 | 0.00 | 0.76 | 11.67 | 185.06 | -8.22 | 60.63 | 0.1613 | -755.0 | -587.5 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 11.98 | 184.96 | -8.32 | 59.30 | 0.1653 | -847.0 | -673.8 | |
| 0.00 | 1.43 | 0.00 | 0.72 | 5.86 | 185.00 | -8.28 | 98.95 | 0.1457 | -699.0 | -578.8 | |
| 0.00 | 1.61 | 0.00 | 0.84 | 10.76 | 175.76 | -17.51 | 77.17 | 0.3046 | 944.0 | 683.7 | |
| 0.00 | 1.25 | 0.00 | 0.67 | 8.06 | 171.16 | -22.12 | 86.37 | 0.3752 | 563.0 | 597.1 | |
| 0.00 | 1.16 | 0.00 | 0.65 | 11.94 | 165.80 | -27.48 | 77.99 | 0.4635 | 820.0 | 636.2 | |
| 0.00 | 0.63 | 0.00 | 0.36 | 15.53 | 162.34 | -30.93 | 71.93 | 0.5230 | 233.0 | 283.6 | |
| 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. | |