SDO HMI 2014-08-29 13:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.13 | 42.65 | 13.78 | 34.92 | -17.57 | 206.12 | -47.17 | 118.55 | 0.7974 | 240.5 | 136.9 | |
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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 |
| 3.32 | 19.00 | 2.61 | 15.02 | -17.69 | 208.10 | -45.19 | 119.65 | 0.7801 | 701.3 | 439.6 | |
| 8.96 | -1.00 | 7.10 | -1.00 | -17.55 | 207.78 | -45.51 | 119.33 | 0.7825 | 599.9 | 999999 | |
| 0.99 | 2.06 | 0.76 | 1.58 | -14.99 | 208.23 | -45.06 | 116.53 | 0.7665 | 601.2 | 560.1 | |
| 0.00 | 2.15 | 0.00 | 1.73 | -17.27 | 206.95 | -46.34 | 118.58 | 0.7889 | 468.0 | 348.9 | |
| 0.00 | 2.51 | 0.00 | 2.02 | -16.71 | 206.53 | -46.76 | 117.73 | 0.7905 | 633.0 | 494.7 | |
| 0.72 | 1.70 | 0.60 | 1.42 | -18.77 | 205.77 | -47.52 | 119.72 | 0.8063 | 370.1 | 325.5 | |
| 0.72 | 4.84 | 0.58 | 3.90 | -16.61 | 206.29 | -47.00 | 117.49 | 0.7923 | 431.1 | 461.5 | |
| 1.70 | 4.48 | 1.46 | 3.84 | -18.50 | 204.38 | -48.91 | 118.76 | 0.8175 | -655.5 | -497.2 | |
| 0.00 | 0.81 | 0.00 | 0.73 | -19.70 | 202.43 | -50.86 | 119.20 | 0.8387 | -530.0 | -489.9 | |
| 0.00 | 0.90 | 0.00 | 0.80 | -17.77 | 202.43 | -50.86 | 117.07 | 0.8316 | -586.0 | -558.9 | |
| 0.00 | 1.43 | 0.00 | 1.28 | -17.65 | 202.27 | -51.02 | 116.87 | 0.8325 | -565.0 | -480.2 | |
| 0.00 | 1.43 | 0.00 | 1.35 | -19.35 | 200.55 | -52.74 | 118.03 | 0.8528 | -413.0 | -362.8 | |
| 0.72 | 1.34 | 0.67 | 1.25 | -17.71 | 200.38 | -52.91 | 116.16 | 0.8487 | -464.5 | -374.4 | |
| 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. | |