SDO HMI 2014-03-10 21:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.33 | 0.00 | 13.38 | -10.72 | 14.49 | 12.02 | 251.19 | 0.2172 | 350.5 | 325.7 | |
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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 | 1.30 | 0.00 | 0.67 | -7.65 | 17.85 | 15.39 | 267.45 | 0.2644 | 688.0 | 583.9 | |
| 0.00 | 2.25 | 0.00 | 1.16 | -10.07 | 17.61 | 15.14 | 258.19 | 0.2640 | 686.0 | 605.8 | |
| 0.00 | 1.99 | 0.00 | 1.02 | -10.04 | 16.64 | 14.17 | 257.67 | 0.2479 | 904.0 | 694.2 | |
| 0.00 | 1.13 | 0.00 | 0.58 | -10.28 | 16.52 | 14.06 | 256.62 | 0.2468 | 875.0 | 721.7 | |
| 0.00 | 3.55 | 0.00 | 1.81 | -10.74 | 16.17 | 13.71 | 254.48 | 0.2427 | 840.0 | 796.0 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -10.72 | 15.98 | 13.52 | 254.40 | 0.2395 | 880.0 | 695.2 | |
| 0.00 | 2.51 | 0.00 | 1.28 | -10.72 | 15.67 | 13.21 | 254.06 | 0.2345 | 885.0 | 678.3 | |
| 0.00 | 1.30 | 0.00 | 0.66 | -10.64 | 15.42 | 12.95 | 254.15 | 0.2301 | 814.0 | 569.5 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -10.49 | 14.33 | 11.86 | 253.62 | 0.2117 | 652.0 | 507.7 | |
| 0.00 | 2.69 | 0.00 | 1.36 | -10.91 | 14.28 | 11.82 | 251.65 | 0.2128 | 762.0 | 699.5 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -10.65 | 14.02 | 11.56 | 252.52 | 0.2074 | 819.0 | 698.1 | |
| 0.00 | 3.03 | 0.00 | 1.52 | -11.55 | 10.61 | 8.14 | 241.14 | 0.1592 | -1025.0 | -829.0 | |
| 0.00 | 1.47 | 0.00 | 0.74 | -11.82 | 10.49 | 8.03 | 239.30 | 0.1597 | -869.0 | -681.9 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -12.29 | 9.12 | 6.66 | 231.87 | 0.1447 | -838.0 | -714.5 | |
| 0.00 | 0.87 | 0.00 | 0.43 | -12.23 | 8.91 | 6.44 | 231.29 | 0.1412 | -816.0 | -644.7 | |
| 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. | |