SDO HMI 2013-09-26 00:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.55 | 384.97 | 41.75 | 244.80 | -17.95 | 57.99 | 30.26 | 229.79 | 0.6300 | 890.1 | 370.0 | |
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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 | 0.62 | 0.00 | 0.41 | -19.65 | 61.13 | 33.40 | 230.40 | 0.6752 | 440.0 | 362.6 | |
| 62.81 | 376.39 | 40.01 | 239.50 | -17.92 | 58.10 | 30.38 | 229.94 | 0.6309 | 1169.7 | 391.6 | |
| 1.24 | -2.00 | 0.79 | -2.00 | -18.38 | 57.64 | 29.91 | 228.93 | 0.6300 | 734.0 | 999999 | |
| 1.50 | -2.00 | 0.95 | -2.00 | -18.06 | 57.29 | 29.56 | 229.00 | 0.6237 | 1014.9 | 999999 | |
| 0.00 | 1.24 | 0.00 | 0.77 | -16.30 | 56.84 | 29.11 | 230.87 | 0.6042 | -568.0 | -399.7 | |
| 0.00 | 1.33 | 0.00 | 0.82 | -18.06 | 55.05 | 27.33 | 226.81 | 0.6009 | -610.0 | -454.1 | |
| 0.00 | 0.97 | 0.00 | 0.60 | -19.67 | 53.09 | 25.36 | 222.71 | 0.5969 | -747.0 | -542.4 | |
| 0.00 | 1.06 | 0.00 | 0.65 | -18.91 | 52.58 | 24.85 | 223.06 | 0.5845 | -632.0 | -559.2 | |
| 0.00 | 1.50 | 0.00 | 0.91 | -18.86 | 52.25 | 24.53 | 222.76 | 0.5809 | -543.0 | -484.6 | |
| 0.00 | 1.06 | 0.00 | 0.64 | -18.14 | 51.90 | 24.18 | 223.24 | 0.5703 | -782.0 | -703.0 | |
| 0.00 | 0.80 | 0.00 | 0.50 | -22.42 | 51.27 | 23.54 | 217.51 | 0.6086 | -616.0 | -410.1 | |
| 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. | |