SDO HMI 2014-11-14 04:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.24 | 55.33 | 10.02 | 36.88 | 8.58 | 4.16 | 41.96 | 279.56 | 0.6725 | 141.5 | -306.4 | |
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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 | 1.29 | 0.00 | 0.89 | 8.38 | 6.48 | 44.28 | 278.95 | 0.7016 | -515.0 | -477.2 | |
| 0.00 | 2.58 | 0.00 | 1.77 | 8.43 | 5.78 | 43.58 | 279.11 | 0.6929 | -508.0 | -336.5 | |
| 0.26 | 25.99 | 0.18 | 17.62 | 8.29 | 5.51 | 43.31 | 278.93 | 0.6895 | -729.0 | -637.6 | |
| 0.00 | 1.12 | 0.00 | 0.76 | 8.56 | 5.55 | 43.35 | 279.32 | 0.6902 | -453.0 | -393.8 | |
| 3.79 | -3.00 | 2.58 | -3.00 | 8.09 | 5.40 | 43.20 | 278.65 | 0.6879 | -874.6 | 999999 | |
| 1.03 | -3.00 | 0.70 | -3.00 | 8.18 | 5.17 | 42.96 | 278.82 | 0.6850 | -933.4 | 999999 | |
| 0.00 | 3.70 | 0.00 | 2.47 | 8.13 | 4.26 | 42.06 | 278.84 | 0.6735 | -712.0 | -705.7 | |
| 0.00 | 0.77 | 0.00 | 0.51 | 9.62 | 3.59 | 41.38 | 281.15 | 0.6667 | 512.0 | 467.9 | |
| 0.00 | 1.03 | 0.00 | 0.68 | 10.10 | 2.70 | 40.50 | 282.03 | 0.6560 | 396.0 | 392.5 | |
| 0.00 | 1.64 | 0.00 | 1.06 | 9.48 | 2.41 | 40.20 | 281.14 | 0.6513 | 643.0 | 463.7 | |
| 0.69 | 1.89 | 0.45 | 1.23 | 10.05 | 2.22 | 40.01 | 282.06 | 0.6497 | 859.1 | 737.1 | |
| 0.00 | 0.86 | 0.00 | 0.56 | 10.26 | 2.21 | 40.01 | 282.38 | 0.6500 | 646.0 | 577.0 | |
| 2.07 | 4.39 | 1.34 | 2.84 | 9.52 | 1.98 | 39.78 | 281.29 | 0.6458 | 819.4 | 608.6 | |
| 7.40 | 10.07 | 4.77 | 6.49 | 8.78 | 1.84 | 39.64 | 280.16 | 0.6428 | 891.0 | 609.4 | |
| 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. | |