SDO HMI 2014-01-15 14:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.05 | 40.51 | 7.02 | 24.97 | 16.24 | 27.76 | 30.31 | 305.72 | 0.5975 | -14.3 | 53.1 | |
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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 |
| 8.33 | 11.73 | 5.32 | 7.49 | 15.95 | 31.07 | 33.62 | 302.41 | 0.6328 | -828.2 | -518.5 | |
| 2.04 | 3.49 | 1.29 | 2.21 | 16.05 | 30.43 | 32.97 | 303.03 | 0.6261 | -799.9 | -627.9 | |
| 0.00 | 1.28 | 0.00 | 0.80 | 16.00 | 30.02 | 32.56 | 303.27 | 0.6211 | -698.0 | -616.7 | |
| 0.00 | 6.12 | 0.00 | 3.84 | 15.95 | 29.68 | 32.23 | 303.47 | 0.6169 | -804.0 | -692.2 | |
| 0.34 | 1.79 | 0.21 | 1.08 | 15.70 | 26.64 | 29.18 | 305.67 | 0.5800 | 821.2 | 645.9 | |
| 0.34 | 1.79 | 0.20 | 1.07 | 15.93 | 25.35 | 27.89 | 307.21 | 0.5670 | -858.8 | -637.6 | |
| 0.00 | 1.87 | 0.00 | 1.13 | 16.84 | 25.11 | 27.65 | 308.75 | 0.5718 | 642.0 | 585.6 | |
| 0.00 | 4.93 | 0.00 | 2.97 | 17.23 | 24.61 | 27.16 | 309.80 | 0.5697 | 581.0 | 728.6 | |
| 0.00 | 0.94 | 0.00 | 0.56 | 16.14 | 24.27 | 26.82 | 308.58 | 0.5565 | 689.0 | 568.6 | |
| 0.00 | 0.77 | 0.00 | 0.45 | 16.04 | 24.05 | 26.60 | 308.65 | 0.5531 | 742.0 | 640.9 | |
| 0.00 | 1.28 | 0.00 | 0.75 | 15.89 | 23.24 | 25.79 | 309.27 | 0.5426 | 1000.0 | 879.5 | |
| 0.00 | 1.87 | 0.00 | 1.10 | 16.31 | 22.75 | 25.30 | 310.42 | 0.5409 | 921.0 | 810.0 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 18.18 | 21.94 | 24.48 | 314.00 | 0.5495 | 692.0 | 541.4 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 16.19 | 21.12 | 23.66 | 312.10 | 0.5216 | 767.0 | 596.0 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 17.11 | 18.17 | 20.72 | 317.18 | 0.4994 | 656.0 | 478.0 | |
| 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. | |