SDO HMI 2014-11-13 00:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.96 | 0.00 | 11.14 | -9.20 | 338.88 | 1.29 | 186.39 | 0.2259 | 68.9 | 50.8 | |
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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 |
| 0.00 | 1.21 | 0.00 | 0.61 | -4.93 | 343.85 | 6.27 | 217.93 | 0.1778 | 834.0 | 710.1 | |
| 0.00 | 0.77 | 0.00 | 0.39 | -6.55 | 343.48 | 5.89 | 211.34 | 0.1971 | 801.0 | 625.1 | |
| 0.00 | 2.75 | 0.00 | 1.40 | -7.99 | 342.47 | 4.89 | 203.68 | 0.2110 | 951.0 | 694.2 | |
| 0.00 | 1.81 | 0.00 | 0.92 | -10.02 | 342.35 | 4.76 | 199.80 | 0.2424 | 797.0 | 642.5 | |
| 0.00 | 1.29 | 0.00 | 0.65 | -8.17 | 342.17 | 4.59 | 202.06 | 0.2119 | 860.0 | 746.6 | |
| 0.00 | 1.38 | 0.00 | 0.70 | -10.50 | 341.87 | 4.28 | 197.34 | 0.2476 | 806.0 | 625.6 | |
| 0.00 | 1.38 | 0.00 | 0.70 | -10.72 | 341.72 | 4.14 | 196.52 | 0.2504 | 702.0 | 619.0 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -10.78 | 341.51 | 3.92 | 195.65 | 0.2504 | 1043.0 | 855.7 | |
| 0.00 | 0.86 | 0.00 | 0.44 | -10.18 | 336.65 | -0.94 | 176.00 | 0.2316 | -879.0 | -702.1 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -9.18 | 336.29 | -1.29 | 174.03 | 0.2151 | -757.0 | -636.8 | |
| 0.00 | 2.15 | 0.00 | 1.09 | -9.36 | 336.02 | -1.56 | 172.89 | 0.2187 | -846.0 | -726.6 | |
| 0.00 | 1.55 | 0.00 | 0.79 | -11.41 | 335.19 | -2.39 | 170.72 | 0.2552 | -785.0 | -532.8 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -10.18 | 335.14 | -2.44 | 169.66 | 0.2349 | -771.0 | -602.1 | |
| 0.00 | 1.89 | 0.00 | 0.97 | -10.31 | 333.87 | -3.71 | 164.65 | 0.2417 | -846.0 | -680.6 | |
| 0.00 | 1.81 | 0.00 | 0.91 | -7.70 | 333.03 | -4.55 | 157.24 | 0.2043 | -877.0 | -643.5 | |
| 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. | |