SDO HMI 2014-12-11 04:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.30 | 296.17 | 32.79 | 178.81 | -3.95 | 1.08 | 34.73 | 263.65 | 0.5741 | 854.5 | 338.7 | |
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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 | 2.90 | 0.00 | 1.75 | -1.45 | 1.33 | 34.98 | 268.04 | 0.5756 | -957.0 | -729.4 | |
| 34.01 | 269.66 | 20.61 | 163.05 | -4.14 | 1.38 | 35.03 | 263.37 | 0.5786 | 1105.6 | 359.7 | |
| 1.88 | 9.97 | 1.13 | 5.98 | -2.90 | 0.79 | 34.44 | 265.46 | 0.5687 | 782.9 | 510.4 | |
| 16.19 | -2.00 | 9.74 | -2.00 | -3.87 | 0.79 | 34.44 | 263.74 | 0.5698 | 1263.5 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.66 | -1.48 | 0.61 | 34.26 | 267.95 | 0.5653 | -699.0 | -467.8 | |
| 0.60 | -3.00 | 0.36 | -3.00 | -2.72 | 0.49 | 34.14 | 265.74 | 0.5644 | 768.1 | 999999 | |
| 0.43 | 1.36 | 0.25 | 0.81 | -1.83 | 0.26 | 33.91 | 267.30 | 0.5604 | -652.8 | -556.3 | |
| 0.00 | 1.88 | 0.00 | 1.12 | -6.75 | 0.14 | 33.79 | 258.55 | 0.5657 | 672.0 | 388.0 | |
| 0.00 | 1.11 | 0.00 | 0.65 | -2.72 | 359.11 | 32.76 | 265.59 | 0.5443 | 640.0 | 575.9 | |
| 0.00 | 0.51 | 0.00 | 0.30 | -3.61 | 359.07 | 32.72 | 263.95 | 0.5446 | 706.0 | 618.3 | |
| 0.00 | 0.77 | 0.00 | 0.45 | -2.93 | 359.05 | 32.69 | 265.20 | 0.5435 | 167.0 | 141.6 | |
| 0.34 | 2.47 | 0.20 | 1.45 | -2.01 | 358.88 | 32.53 | 266.87 | 0.5404 | 972.2 | 787.9 | |
| 0.00 | 1.11 | 0.00 | 0.65 | -4.08 | 358.84 | 32.49 | 263.04 | 0.5420 | 725.0 | 526.2 | |
| 0.85 | 3.32 | 0.50 | 1.94 | -3.32 | 358.11 | 31.76 | 264.35 | 0.5302 | -806.2 | -731.1 | |
| 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. | |