SDO HMI 2014-12-07 06:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 93.59 | 589.72 | 129.50 | 816.81 | -19.63 | 85.50 | 67.53 | 248.84 | 0.9346 | 619.5 | 217.8 | |
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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 |
| 28.50 | 574.97 | 42.58 | 798.04 | -18.74 | 87.37 | 69.40 | 250.04 | 0.9446 | 426.2 | 219.5 | |
| 19.96 | -1.00 | 27.67 | -1.00 | -19.18 | 85.68 | 67.71 | 249.36 | 0.9354 | 690.2 | 999999 | |
| 1.62 | -1.00 | 2.17 | -1.00 | -19.52 | 84.82 | 66.85 | 248.88 | 0.9307 | 568.3 | 999999 | |
| 0.00 | 5.63 | 0.00 | 7.95 | -21.35 | 85.81 | 67.84 | 247.08 | 0.9380 | 148.0 | 106.9 | |
| 39.33 | -1.00 | 51.54 | -1.00 | -20.33 | 84.15 | 66.18 | 247.91 | 0.9274 | 825.8 | 999999 | |
| 2.47 | -1.00 | 3.35 | -1.00 | -21.73 | 84.75 | 66.78 | 246.51 | 0.9324 | 465.7 | 999999 | |
| 1.71 | -1.00 | 2.19 | -1.00 | -20.90 | 83.38 | 65.41 | 247.18 | 0.9233 | 808.4 | 999999 | |
| 0.00 | 0.85 | 0.00 | 1.04 | -20.77 | 82.22 | 64.25 | 247.12 | 0.9158 | 242.0 | 275.6 | |
| 0.00 | 1.19 | 0.00 | 1.43 | -20.93 | 81.69 | 63.72 | 246.86 | 0.9125 | 632.0 | 527.3 | |
| 0.00 | 3.41 | 0.00 | 4.22 | -21.85 | 82.36 | 64.39 | 245.98 | 0.9180 | 533.0 | 459.5 | |
| 0.00 | 0.77 | 0.00 | 0.87 | -19.53 | 80.25 | 62.28 | 248.12 | 0.9010 | -278.0 | -262.9 | |
| 0.00 | 0.94 | 0.00 | 1.09 | -21.11 | 80.69 | 62.73 | 246.47 | 0.9061 | -220.0 | -173.0 | |
| 0.00 | 1.62 | 0.00 | 1.81 | -20.60 | 79.64 | 61.67 | 246.83 | 0.8981 | -111.0 | -182.0 | |
| 0.00 | 0.34 | 0.00 | 0.36 | -22.35 | 77.72 | 59.76 | 244.51 | 0.8872 | -140.0 | -209.5 | |
| 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. | |