SDO HMI 2014-09-13 05:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.48 | 141.01 | 13.25 | 76.41 | -15.79 | 65.95 | 6.38 | 195.35 | 0.4069 | 736.3 | 479.1 | |
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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 |
| 0.00 | 1.07 | 0.00 | 0.59 | -16.94 | 67.15 | 7.59 | 197.18 | 0.4294 | 643.0 | 461.2 | |
| 1.16 | 130.23 | 0.63 | 70.53 | -15.95 | 67.02 | 7.45 | 197.62 | 0.4138 | 952.4 | 533.3 | |
| 4.63 | -2.00 | 2.51 | -2.00 | -15.88 | 66.64 | 7.07 | 196.82 | 0.4109 | 975.7 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -16.31 | 66.59 | 7.02 | 196.41 | 0.4172 | 456.0 | 368.5 | |
| 3.20 | -2.00 | 1.74 | -2.00 | -15.74 | 66.38 | 6.81 | 196.34 | 0.4076 | 1201.0 | 999999 | |
| 5.87 | -2.00 | 3.18 | -2.00 | -15.74 | 66.13 | 6.56 | 195.77 | 0.4065 | 1174.8 | 999999 | |
| 9.35 | -2.00 | 5.05 | -2.00 | -15.57 | 65.87 | 6.30 | 195.29 | 0.4028 | 1271.6 | 999999 | |
| 0.27 | -2.00 | 0.14 | -2.00 | -15.31 | 65.86 | 6.30 | 195.45 | 0.3987 | 1293.7 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.68 | -16.25 | 65.07 | 5.50 | 193.03 | 0.4102 | 807.0 | 636.4 | |
| 0.00 | 1.34 | 0.00 | 0.72 | -14.93 | 64.03 | 4.47 | 191.29 | 0.3859 | 732.0 | 539.5 | |
| 0.00 | 0.80 | 0.00 | 0.43 | -16.20 | 63.74 | 4.18 | 189.98 | 0.4052 | 700.0 | 584.1 | |
| 0.00 | 1.69 | 0.00 | 0.92 | -16.68 | 62.49 | 2.92 | 186.88 | 0.4099 | -893.0 | -694.8 | |
| 0.00 | 1.07 | 0.00 | 0.58 | -17.21 | 61.90 | 2.33 | 185.37 | 0.4172 | -693.0 | -573.3 | |
| 0.00 | 1.16 | 0.00 | 0.64 | -19.21 | 60.71 | 1.14 | 182.42 | 0.4475 | -683.0 | -557.3 | |
| 0.00 | 1.51 | 0.00 | 0.84 | -19.07 | 59.81 | 0.25 | 180.53 | 0.4450 | -721.0 | -575.5 | |
| 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. | |