SDO HMI 2014-09-20 05:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.78 | 259.41 | 71.88 | 307.85 | -9.51 | 263.83 | -63.33 | 103.94 | 0.9079 | 158.3 | 64.2 | |
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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 | 1.06 | 0.00 | 1.08 | -8.12 | 268.15 | -59.00 | 103.47 | 0.8746 | 454.0 | 496.2 | |
| 24.83 | 152.99 | 26.13 | 162.10 | -8.27 | 267.02 | -60.13 | 103.36 | 0.8839 | 932.6 | 229.1 | |
| 8.60 | -2.00 | 9.25 | -2.00 | -8.47 | 266.35 | -60.81 | 103.41 | 0.8895 | 464.3 | 999999 | |
| 0.00 | 1.33 | 0.00 | 1.48 | -9.21 | 265.49 | -61.66 | 104.02 | 0.8973 | -93.0 | -98.7 | |
| 0.00 | 1.24 | 0.00 | 1.39 | -9.02 | 265.29 | -61.86 | 103.76 | 0.8985 | -213.0 | -178.4 | |
| 2.93 | 8.07 | 3.23 | 8.97 | -7.89 | 265.42 | -61.74 | 102.55 | 0.8957 | 353.5 | 247.2 | |
| 0.00 | 2.48 | 0.00 | 2.76 | -8.40 | 265.28 | -61.88 | 103.08 | 0.8975 | 281.0 | 147.4 | |
| 0.00 | 1.06 | 0.00 | 1.19 | -8.63 | 265.15 | -62.01 | 103.30 | 0.8989 | 126.0 | 101.2 | |
| 0.00 | 0.89 | 0.00 | 1.00 | -7.84 | 264.78 | -62.38 | 102.35 | 0.9004 | 210.0 | 201.5 | |
| 0.00 | 1.24 | 0.00 | 1.49 | -7.99 | 263.17 | -63.99 | 102.15 | 0.9121 | -369.0 | -403.2 | |
| 0.00 | 1.60 | 0.00 | 2.01 | -8.62 | 261.97 | -65.19 | 102.57 | 0.9211 | -379.0 | -356.0 | |
| 0.00 | 0.89 | 0.00 | 1.12 | -8.34 | 261.99 | -65.17 | 102.27 | 0.9206 | -196.0 | -244.8 | |
| 0.00 | 0.62 | 0.00 | 0.85 | -10.70 | 260.40 | -66.76 | 104.43 | 0.9338 | -489.0 | -458.7 | |
| 16.32 | 85.94 | 23.25 | 122.41 | -11.57 | 259.66 | -67.49 | 105.17 | 0.9393 | -582.6 | -159.2 | |
| 7.10 | -14.00 | 10.02 | -14.00 | -10.72 | 259.67 | -67.49 | 104.29 | 0.9382 | -263.1 | 999999 | |
| 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. | |