SDO HMI 2014-09-24 02:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.40 | 0.00 | 8.08 | 16.28 | 258.57 | -17.44 | 59.96 | 0.3337 | 810.2 | 688.2 | |
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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 | 0.71 | 0.00 | 0.37 | 16.80 | 259.86 | -16.15 | 56.75 | 0.3198 | 790.0 | 555.9 | |
| 0.00 | 1.33 | 0.00 | 0.69 | 15.12 | 259.76 | -16.24 | 61.64 | 0.3081 | 770.0 | 630.2 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 16.94 | 259.48 | -16.52 | 56.92 | 0.3261 | 713.0 | 653.5 | |
| 0.00 | 2.03 | 0.00 | 1.06 | 15.47 | 259.41 | -16.59 | 61.08 | 0.3158 | 1004.0 | 836.6 | |
| 0.00 | 1.95 | 0.00 | 1.02 | 15.71 | 259.23 | -16.77 | 60.65 | 0.3201 | 958.0 | 778.4 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 15.22 | 259.24 | -16.77 | 62.03 | 0.3166 | 809.0 | 702.7 | |
| 0.00 | 0.80 | 0.00 | 0.42 | 15.28 | 258.97 | -17.03 | 62.22 | 0.3208 | 696.0 | 585.6 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 16.02 | 258.35 | -17.65 | 60.93 | 0.3349 | 956.0 | 820.1 | |
| 0.00 | 1.68 | 0.00 | 0.89 | 17.26 | 258.20 | -17.80 | 57.85 | 0.3464 | 922.0 | 673.5 | |
| 0.00 | 1.77 | 0.00 | 0.93 | 17.16 | 257.95 | -18.06 | 58.43 | 0.3491 | 903.0 | 663.5 | |
| 0.00 | 0.71 | 0.00 | 0.37 | 16.43 | 257.95 | -18.05 | 60.32 | 0.3436 | 397.0 | 379.6 | |
| 0.00 | 1.24 | 0.00 | 0.67 | 17.68 | 254.64 | -21.37 | 60.92 | 0.3989 | 805.0 | 640.9 | |
| 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. | |