SDO HMI 2014-11-08 12:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.35 | 48.22 | 13.74 | 41.40 | -5.28 | 91.01 | 54.07 | 260.88 | 0.8177 | 164.8 | 119.7 | |
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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 |
| 6.38 | 23.98 | 5.85 | 21.84 | -4.87 | 93.67 | 56.73 | 261.87 | 0.8437 | 439.3 | 397.3 | |
| 5.78 | -1.00 | 5.23 | -1.00 | -4.81 | 93.23 | 56.29 | 261.87 | 0.8395 | 763.4 | 999999 | |
| 0.00 | 1.38 | 0.00 | 1.19 | -3.35 | 91.60 | 54.66 | 263.38 | 0.8220 | 460.0 | 341.2 | |
| 1.47 | 2.59 | 1.23 | 2.18 | -5.91 | 90.10 | 53.16 | 260.01 | 0.8105 | 604.1 | 478.6 | |
| 1.12 | 4.14 | 0.94 | 3.47 | -5.64 | 90.06 | 53.12 | 260.34 | 0.8097 | 674.3 | 499.3 | |
| 0.00 | 2.50 | 0.00 | 2.09 | -4.88 | 89.97 | 53.03 | 261.25 | 0.8076 | 476.0 | 513.6 | |
| 0.00 | 0.60 | 0.00 | 0.49 | -6.14 | 88.75 | 51.81 | 259.46 | 0.7971 | -262.0 | -266.7 | |
| 0.00 | 1.04 | 0.00 | 0.83 | -5.93 | 88.23 | 51.29 | 259.61 | 0.7914 | -508.0 | -343.1 | |
| 0.60 | 5.09 | 0.49 | 4.09 | -6.26 | 88.04 | 51.10 | 259.17 | 0.7899 | -693.7 | -453.4 | |
| 0.00 | 1.90 | 0.00 | 1.52 | -5.94 | 87.81 | 50.87 | 259.52 | 0.7869 | -97.0 | -120.0 | |
| 0.00 | 1.29 | 0.00 | 1.00 | -5.21 | 86.45 | 49.51 | 260.16 | 0.7710 | -613.0 | -528.5 | |
| 0.00 | 1.21 | 0.00 | 0.92 | -4.51 | 85.61 | 48.67 | 260.90 | 0.7604 | -682.0 | -603.1 | |
| 0.00 | 0.60 | 0.00 | 0.45 | -8.81 | 84.10 | 47.16 | 254.93 | 0.7527 | -504.0 | -469.6 | |
| 0.00 | 0.78 | 0.00 | 0.54 | -7.08 | 80.68 | 43.74 | 256.24 | 0.7087 | -537.0 | -451.2 | |
| 0.00 | 1.12 | 0.00 | 0.79 | -8.38 | 80.68 | 43.74 | 254.45 | 0.7123 | -561.0 | -484.8 | |
| 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. | |