SDO HMI 2014-12-10 13:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.30 | 335.25 | 36.69 | 185.76 | -3.81 | 1.04 | 26.42 | 262.11 | 0.4501 | 924.7 | 359.1 | |
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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 |
| 37.07 | 297.50 | 20.62 | 165.13 | -4.05 | 1.44 | 26.82 | 261.68 | 0.4568 | 1245.7 | 371.9 | |
| 0.00 | 1.02 | 0.00 | 0.57 | -2.89 | 1.11 | 26.49 | 264.14 | 0.4497 | 648.0 | 508.1 | |
| 1.70 | 6.99 | 0.94 | 3.86 | -1.39 | 0.98 | 26.37 | 267.50 | 0.4463 | -1022.8 | -654.6 | |
| 0.00 | 0.94 | 0.00 | 0.52 | -2.16 | 0.99 | 26.38 | 265.77 | 0.4471 | 419.0 | 512.5 | |
| 1.11 | 3.24 | 0.61 | 1.79 | -2.72 | 0.97 | 26.36 | 264.51 | 0.4474 | 820.2 | 608.2 | |
| 0.00 | 1.79 | 0.00 | 0.99 | -2.45 | 0.87 | 26.25 | 265.09 | 0.4454 | 574.0 | 596.3 | |
| 18.75 | -1.00 | 10.37 | -1.00 | -3.81 | 0.80 | 26.19 | 262.03 | 0.4465 | 1331.5 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.33 | -1.83 | 359.28 | 24.67 | 266.28 | 0.4198 | 627.0 | 501.4 | |
| 0.00 | 1.28 | 0.00 | 0.70 | -2.69 | 359.23 | 24.62 | 264.23 | 0.4200 | 768.0 | 603.8 | |
| 0.51 | 5.62 | 0.28 | 3.06 | -1.92 | 359.09 | 24.47 | 266.04 | 0.4168 | 1064.5 | 719.0 | |
| 0.00 | 1.19 | 0.00 | 0.65 | -5.26 | 359.18 | 24.57 | 258.15 | 0.4248 | 911.0 | 723.4 | |
| 0.00 | 1.53 | 0.00 | 0.83 | -1.74 | 359.06 | 24.44 | 266.46 | 0.4161 | 729.0 | 533.9 | |
| 0.00 | 1.79 | 0.00 | 0.97 | -2.69 | 358.78 | 24.16 | 264.13 | 0.4128 | 931.0 | 867.3 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -3.55 | 358.73 | 24.12 | 262.05 | 0.4136 | 802.0 | 759.6 | |
| 7.16 | 10.40 | 3.87 | 5.62 | -3.22 | 358.11 | 23.50 | 262.66 | 0.4031 | -938.7 | -688.7 | |
| 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. | |