SDO HMI 2014-09-19 10:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.70 | 0.00 | 9.91 | 9.35 | 334.01 | -3.60 | 209.91 | 0.1403 | 125.7 | 5.9 | |
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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 | 1.95 | 0.00 | 0.97 | 9.15 | 344.46 | 6.85 | 287.18 | 0.1238 | 617.0 | 331.9 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 8.32 | 343.74 | 6.13 | 281.61 | 0.1083 | -888.0 | -707.6 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 8.63 | 343.56 | 5.95 | 284.74 | 0.1064 | -949.0 | -817.3 | |
| 0.00 | 2.31 | 0.00 | 1.15 | 9.23 | 343.48 | 5.87 | 290.37 | 0.1081 | -871.0 | -665.2 | |
| 0.00 | 1.15 | 0.00 | 0.57 | 9.99 | 339.33 | 1.71 | 329.60 | 0.0584 | -973.0 | -766.2 | |
| 0.00 | 2.22 | 0.00 | 1.10 | 8.16 | 337.58 | -0.03 | 1.77 | 0.0182 | -840.0 | -754.8 | |
| 0.00 | 1.51 | 0.00 | 0.75 | 8.49 | 337.40 | -0.21 | 8.81 | 0.0243 | -983.0 | -811.1 | |
| 0.00 | 0.71 | 0.00 | 0.36 | 8.43 | 329.55 | -8.06 | 80.15 | 0.1415 | 814.0 | 609.2 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 8.91 | 329.14 | -8.47 | 77.41 | 0.1499 | 750.0 | 592.2 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 7.56 | 328.12 | -9.49 | 86.71 | 0.1645 | 854.0 | 718.2 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 7.68 | 327.88 | -9.74 | 86.07 | 0.1688 | 998.0 | 804.4 | |
| 0.00 | 1.33 | 0.00 | 0.67 | 8.06 | 327.43 | -10.18 | 84.01 | 0.1768 | 925.0 | 730.1 | |
| 0.00 | 1.51 | 0.00 | 0.76 | 7.91 | 327.28 | -10.33 | 84.94 | 0.1792 | 844.0 | 738.4 | |
| 0.00 | 0.89 | 0.00 | 0.47 | 16.29 | 317.41 | -20.21 | 63.29 | 0.3727 | 786.0 | 647.2 | |
| 0.00 | 1.33 | 0.00 | 0.71 | 14.37 | 317.40 | -20.22 | 68.23 | 0.3620 | 802.0 | 610.7 | |
| 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. | |