SDO HMI 2014-02-26 04:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.17 | 26.96 | 3.75 | 19.47 | 6.21 | 125.08 | -44.80 | 74.40 | 0.7296 | -483.7 | -339.4 | |
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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 | 1.38 | 0.00 | 0.97 | 9.83 | 127.66 | -42.22 | 68.51 | 0.7139 | -615.0 | -531.7 | |
| 0.00 | 2.15 | 0.00 | 1.47 | 5.21 | 128.01 | -41.87 | 74.62 | 0.6918 | -651.0 | -438.4 | |
| 0.00 | 2.15 | 0.00 | 1.51 | 7.81 | 127.30 | -42.59 | 71.38 | 0.7098 | -565.0 | -482.4 | |
| 0.00 | 1.29 | 0.00 | 0.90 | 6.85 | 127.37 | -42.52 | 72.63 | 0.7054 | -545.0 | -470.1 | |
| 0.00 | 1.38 | 0.00 | 0.97 | 8.13 | 127.13 | -42.75 | 71.02 | 0.7130 | -674.0 | -597.4 | |
| 0.00 | 1.21 | 0.00 | 0.84 | 6.91 | 127.03 | -42.85 | 72.69 | 0.7095 | -554.0 | -498.3 | |
| 0.00 | 1.90 | 0.00 | 1.33 | 7.23 | 126.92 | -42.97 | 72.32 | 0.7121 | -756.0 | -503.7 | |
| 0.00 | 1.46 | 0.00 | 1.05 | 8.26 | 126.00 | -43.89 | 71.34 | 0.7265 | -610.0 | -513.5 | |
| 0.00 | 0.86 | 0.00 | 0.61 | 4.55 | 125.27 | -44.61 | 76.55 | 0.7222 | -666.0 | -547.3 | |
| 5.17 | 8.53 | 3.75 | 6.19 | 3.98 | 124.21 | -45.67 | 77.67 | 0.7329 | -787.0 | -507.4 | |
| 0.00 | 0.69 | 0.00 | 0.50 | 4.13 | 123.85 | -46.03 | 77.58 | 0.7374 | -441.0 | -332.2 | |
| 0.00 | 1.38 | 0.00 | 1.03 | 4.98 | 122.61 | -47.28 | 76.88 | 0.7538 | 700.0 | 583.5 | |
| 0.00 | 1.46 | 0.00 | 1.14 | 5.00 | 120.76 | -49.12 | 77.43 | 0.7740 | 604.0 | 537.8 | |
| 0.00 | 1.12 | 0.00 | 0.96 | 14.04 | 118.90 | -50.98 | 67.19 | 0.8199 | -377.0 | -307.5 | |
| 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. | |