SDO HMI 2011-11-06 23:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.63 | 254.76 | 58.60 | 266.04 | 17.67 | 61.16 | -61.42 | 71.95 | 0.8797 | -230.3 | -135.0 | |
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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 |
| 0.43 | 187.96 | 0.41 | 181.36 | 16.37 | 64.32 | -58.26 | 73.12 | 0.8548 | -986.0 | -293.6 | |
| 1.73 | -1.00 | 1.67 | -1.00 | 17.17 | 63.68 | -58.90 | 72.26 | 0.8610 | -438.0 | 999999 | |
| 30.72 | -1.00 | 29.61 | -1.00 | 16.74 | 63.78 | -58.80 | 72.75 | 0.8598 | -778.1 | 999999 | |
| 0.69 | -1.00 | 0.68 | -1.00 | 16.63 | 62.92 | -59.66 | 72.97 | 0.8669 | -341.6 | 999999 | |
| 1.38 | -1.00 | 1.38 | -1.00 | 16.94 | 62.44 | -60.14 | 72.66 | 0.8711 | -146.3 | 999999 | |
| 3.37 | 5.52 | 3.46 | 5.69 | 17.42 | 61.60 | -60.98 | 72.20 | 0.8783 | -482.1 | -260.6 | |
| 0.00 | 2.68 | 0.00 | 2.75 | 17.08 | 61.60 | -60.98 | 72.58 | 0.8780 | 245.0 | 56.9 | |
| 0.00 | 1.64 | 0.00 | 1.74 | 17.49 | 60.64 | -61.94 | 72.21 | 0.8858 | 223.0 | 182.6 | |
| 0.00 | 0.95 | 0.00 | 1.06 | 17.39 | 58.91 | -63.67 | 72.48 | 0.8987 | 384.0 | 403.4 | |
| 1.98 | 27.62 | 2.49 | 35.42 | 19.78 | 55.96 | -66.62 | 70.10 | 0.9203 | 682.3 | 449.7 | |
| 0.00 | 1.21 | 0.00 | 1.54 | 19.66 | 55.57 | -67.01 | 70.25 | 0.9228 | 525.0 | 497.9 | |
| 0.00 | 1.98 | 0.00 | 2.50 | 19.35 | 55.74 | -66.83 | 70.57 | 0.9215 | 441.0 | 393.1 | |
| 7.08 | -10.00 | 9.18 | -10.00 | 19.98 | 55.13 | -67.45 | 69.94 | 0.9257 | 598.2 | 999999 | |
| 7.25 | 25.20 | 9.72 | 33.98 | 20.08 | 54.27 | -68.31 | 69.89 | 0.9310 | 347.1 | 106.8 | |
| 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. | |