SDO HMI 2014-12-10 20:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.66 | 322.77 | 34.81 | 185.59 | -3.81 | 1.05 | 30.30 | 263.05 | 0.5092 | 916.6 | 368.6 | |
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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 | 1.28 | 0.00 | 0.76 | -6.13 | 3.53 | 32.77 | 259.27 | 0.5500 | 605.0 | 455.9 | |
| 33.82 | 299.08 | 19.51 | 172.20 | -4.06 | 1.39 | 30.64 | 262.62 | 0.5147 | 1201.4 | 380.4 | |
| 1.28 | 3.75 | 0.73 | 2.15 | -1.37 | 1.15 | 30.39 | 267.85 | 0.5082 | -993.8 | -773.0 | |
| 3.41 | -2.00 | 1.96 | -2.00 | -2.91 | 1.01 | 30.25 | 264.80 | 0.5073 | 745.3 | 999999 | |
| 4.26 | -2.00 | 2.44 | -2.00 | -4.03 | 0.87 | 30.12 | 262.56 | 0.5069 | 1278.3 | 999999 | |
| 0.51 | -2.00 | 0.29 | -2.00 | -2.64 | 0.79 | 30.04 | 265.30 | 0.5039 | 809.2 | 999999 | |
| 12.27 | -2.00 | 7.03 | -2.00 | -3.80 | 0.76 | 30.01 | 263.00 | 0.5049 | 1341.8 | 999999 | |
| 0.00 | 2.39 | 0.00 | 1.36 | -2.14 | 0.54 | 29.79 | 266.27 | 0.4996 | -4.0 | 24.6 | |
| 0.00 | 1.02 | 0.00 | 0.58 | -2.97 | 359.48 | 28.73 | 264.43 | 0.4843 | 790.0 | 720.0 | |
| 0.00 | 2.73 | 0.00 | 1.53 | -2.15 | 359.09 | 28.34 | 266.10 | 0.4774 | 1020.0 | 825.5 | |
| 0.00 | 1.28 | 0.00 | 0.72 | -1.91 | 359.05 | 28.30 | 266.59 | 0.4766 | 1017.0 | 878.3 | |
| 0.00 | 0.85 | 0.00 | 0.48 | -3.03 | 358.94 | 28.19 | 264.21 | 0.4761 | 547.0 | 466.2 | |
| 0.00 | 1.28 | 0.00 | 0.72 | -2.44 | 358.86 | 28.11 | 265.45 | 0.4742 | 768.0 | 507.2 | |
| 0.00 | 2.21 | 0.00 | 1.24 | -3.68 | 358.76 | 28.01 | 262.81 | 0.4743 | 290.0 | 343.8 | |
| 5.11 | 6.90 | 2.85 | 3.85 | -3.27 | 358.11 | 27.36 | 263.55 | 0.4637 | -928.8 | -667.5 | |
| 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. | |