SDO HMI 2014-05-26 04:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.58 | 0.00 | 8.90 | -18.59 | 50.53 | -24.47 | 127.29 | 0.4946 | 565.0 | 466.0 | |
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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 |
| 0.00 | 1.44 | 0.00 | 0.80 | -15.86 | 53.12 | -21.88 | 125.07 | 0.4397 | 728.0 | 561.1 | |
| 0.00 | 2.89 | 0.00 | 1.61 | -18.26 | 52.71 | -22.28 | 129.03 | 0.4654 | 195.0 | 334.7 | |
| 0.00 | 1.35 | 0.00 | 0.76 | -19.15 | 52.52 | -22.48 | 130.34 | 0.4758 | 718.0 | 502.2 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -19.43 | 51.92 | -23.08 | 130.12 | 0.4854 | 724.0 | 626.1 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -19.01 | 51.59 | -23.40 | 129.05 | 0.4855 | 793.0 | 589.0 | |
| 0.00 | 1.53 | 0.00 | 0.88 | -20.03 | 50.91 | -24.09 | 129.98 | 0.5025 | 825.0 | 615.4 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -20.25 | 50.66 | -24.34 | 130.07 | 0.5073 | 709.0 | 522.8 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -15.12 | 51.08 | -23.91 | 121.46 | 0.4606 | 755.0 | 594.5 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -15.27 | 50.93 | -24.07 | 121.60 | 0.4638 | 719.0 | 580.5 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -21.43 | 49.33 | -25.67 | 130.55 | 0.5327 | 646.0 | 519.5 | |
| 0.00 | 1.17 | 0.00 | 0.72 | -20.32 | 43.29 | -31.71 | 123.64 | 0.5942 | 707.0 | 559.8 | |
| 0.00 | 0.72 | 0.00 | 0.45 | -20.18 | 41.90 | -33.09 | 122.44 | 0.6095 | -739.0 | -635.6 | |
| 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. | |