SDO HMI 2014-11-01 01:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.40 | 99.85 | 22.71 | 80.27 | -4.61 | 84.05 | -51.21 | 99.37 | 0.7895 | 564.7 | 397.2 | |
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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 | 0.87 | 0.00 | 0.65 | -4.71 | 87.65 | -47.61 | 100.29 | 0.7504 | 554.0 | 392.0 | |
| 3.20 | 21.65 | 2.53 | 17.19 | -5.20 | 85.04 | -50.22 | 100.31 | 0.7802 | -342.5 | 356.2 | |
| 2.94 | -2.00 | 2.35 | -2.00 | -5.47 | 84.53 | -50.72 | 100.54 | 0.7861 | 763.6 | 999999 | |
| 4.16 | 67.89 | 3.32 | 54.41 | -4.72 | 84.38 | -50.88 | 99.58 | 0.7864 | 778.4 | 472.0 | |
| 9.35 | -4.00 | 7.47 | -4.00 | -4.40 | 84.27 | -50.99 | 99.15 | 0.7870 | 977.6 | 999999 | |
| 3.29 | -4.00 | 2.64 | -4.00 | -4.08 | 84.01 | -51.24 | 98.70 | 0.7892 | 821.2 | 999999 | |
| 0.00 | 0.78 | 0.00 | 0.63 | -5.27 | 83.84 | -51.42 | 100.14 | 0.7930 | 269.0 | 251.3 | |
| 0.00 | 2.25 | 0.00 | 1.83 | -5.19 | 83.66 | -51.60 | 100.01 | 0.7948 | 460.0 | 264.7 | |
| 0.00 | 2.08 | 0.00 | 1.68 | -4.31 | 83.75 | -51.51 | 98.93 | 0.7923 | 210.0 | 220.9 | |
| 0.00 | 0.87 | 0.00 | 0.69 | -3.04 | 83.86 | -51.40 | 97.36 | 0.7892 | 535.0 | 440.6 | |
| 5.46 | -4.00 | 4.40 | -4.00 | -3.92 | 83.74 | -51.52 | 98.44 | 0.7918 | 601.0 | 999999 | |
| 0.00 | 1.21 | 0.00 | 1.03 | -5.23 | 81.57 | -53.69 | 99.63 | 0.8161 | 528.0 | 456.6 | |
| 0.00 | 0.26 | 0.00 | 0.24 | -6.51 | 78.41 | -56.84 | 100.55 | 0.8482 | -392.0 | -487.7 | |
| 0.00 | 1.99 | 0.00 | 1.92 | -6.70 | 77.03 | -58.23 | 100.50 | 0.8608 | -448.0 | -367.9 | |
| 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. | |