SDO HMI 2014-12-09 10:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.48 | 354.85 | 31.17 | 179.98 | -3.85 | 1.28 | 11.84 | 252.61 | 0.2157 | 1184.2 | 389.1 | |
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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 | 1.19 | 0.00 | 0.62 | -4.99 | 4.92 | 15.49 | 252.45 | 0.2803 | 888.0 | 785.1 | |
| 0.00 | 2.30 | 0.00 | 1.19 | -5.20 | 4.86 | 15.43 | 251.68 | 0.2804 | 956.0 | 709.6 | |
| 0.00 | 0.85 | 0.00 | 0.44 | -4.81 | 4.79 | 15.36 | 252.93 | 0.2774 | 896.0 | 801.5 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -5.41 | 4.50 | 15.07 | 250.56 | 0.2757 | 759.0 | 691.3 | |
| 34.11 | 337.65 | 17.31 | 171.21 | -3.98 | 1.49 | 12.05 | 252.29 | 0.2197 | 1391.7 | 389.9 | |
| 9.21 | -5.00 | 4.67 | -5.00 | -4.07 | 1.16 | 11.72 | 251.43 | 0.2148 | 1395.1 | 999999 | |
| 0.00 | 4.43 | 0.00 | 2.24 | -2.36 | 1.11 | 11.67 | 259.30 | 0.2067 | 938.0 | 691.3 | |
| 0.00 | 1.53 | 0.00 | 0.78 | -2.00 | 1.01 | 11.58 | 260.94 | 0.2041 | 538.0 | 473.6 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -1.65 | 0.98 | 11.55 | 262.65 | 0.2027 | -539.0 | -412.8 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -2.33 | 0.84 | 11.40 | 259.20 | 0.2020 | 1009.0 | 708.9 | |
| 0.77 | 3.41 | 0.39 | 1.72 | -1.62 | 0.77 | 11.34 | 262.66 | 0.1991 | -948.8 | -834.9 | |
| 16.20 | -5.00 | 8.20 | -5.00 | -3.60 | 0.76 | 11.32 | 253.02 | 0.2058 | 1501.2 | 999999 | |
| 1.19 | -5.00 | 0.60 | -5.00 | -3.89 | 0.76 | 11.33 | 251.66 | 0.2074 | 878.4 | 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. | |