SDO HMI 2014-03-09 10:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.94 | 47.16 | 2.47 | 23.64 | -11.02 | 13.98 | -7.71 | 117.39 | 0.1485 | 635.2 | 200.8 | |
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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 | 0.95 | 0.00 | 0.47 | -9.50 | 18.56 | -3.13 | 126.40 | 0.0672 | 938.0 | 714.7 | |
| 0.00 | 3.99 | 0.00 | 1.98 | -8.98 | 17.48 | -4.21 | 113.04 | 0.0792 | 652.0 | 915.8 | |
| 0.00 | 2.86 | 0.00 | 1.42 | -9.10 | 17.21 | -4.48 | 113.09 | 0.0843 | 804.0 | 606.1 | |
| 0.00 | 2.34 | 0.00 | 1.16 | -10.05 | 17.07 | -4.62 | 121.99 | 0.0939 | 1396.0 | 1100.6 | |
| 0.00 | 1.39 | 0.00 | 0.69 | -10.28 | 16.62 | -5.08 | 121.64 | 0.1028 | 948.0 | 721.6 | |
| 0.00 | 1.82 | 0.00 | 0.91 | -11.01 | 15.66 | -6.04 | 122.85 | 0.1234 | 934.0 | 832.9 | |
| 0.00 | 1.91 | 0.00 | 0.95 | -11.55 | 15.28 | -6.41 | 124.77 | 0.1339 | 970.0 | 830.4 | |
| 2.60 | 8.32 | 1.30 | 4.16 | -10.98 | 15.17 | -6.52 | 120.66 | 0.1303 | 1164.5 | 827.2 | |
| 1.39 | 2.69 | 0.69 | 1.34 | -10.14 | 14.79 | -6.90 | 113.56 | 0.1296 | 1113.1 | 971.5 | |
| 0.95 | 2.77 | 0.48 | 1.39 | -10.19 | 14.49 | -7.21 | 113.07 | 0.1348 | 1087.8 | 933.2 | |
| 0.00 | 2.17 | 0.00 | 1.09 | -11.53 | 14.27 | -7.42 | 120.96 | 0.1483 | 1002.0 | 755.6 | |
| 0.00 | 13.26 | 0.00 | 6.72 | -12.26 | 10.45 | -11.24 | 115.26 | 0.2116 | -586.0 | -849.2 | |
| 0.00 | 1.56 | 0.00 | 0.79 | -12.73 | 10.31 | -11.39 | 117.02 | 0.2172 | -964.0 | -825.8 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -12.39 | 9.92 | -11.78 | 114.89 | 0.2208 | -794.0 | -687.1 | |
| 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. | |