SDO HMI 2014-04-06 07:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.58 | 26.60 | 0.79 | 13.27 | -8.29 | 8.16 | -5.97 | 112.22 | 0.1168 | -32.0 | 17.5 | |
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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 | 1.67 | 0.00 | 0.83 | -4.46 | 12.85 | -1.28 | 35.68 | 0.0384 | 900.0 | 650.7 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -8.30 | 12.65 | -1.48 | 144.68 | 0.0443 | 809.0 | 585.9 | |
| 0.00 | 1.06 | 0.00 | 0.52 | -7.82 | 12.62 | -1.50 | 136.71 | 0.0381 | 851.0 | 669.8 | |
| 0.00 | 1.85 | 0.00 | 0.92 | -8.90 | 12.25 | -1.87 | 145.17 | 0.0568 | 920.0 | 600.7 | |
| 0.00 | 1.06 | 0.00 | 0.52 | -9.37 | 11.43 | -2.70 | 139.71 | 0.0722 | 819.0 | 652.9 | |
| 0.00 | 2.73 | 0.00 | 1.36 | -10.21 | 10.29 | -3.84 | 136.52 | 0.0961 | 900.0 | 769.3 | |
| 1.58 | 4.58 | 0.79 | 2.28 | -9.72 | 9.99 | -4.13 | 130.67 | 0.0941 | 1089.2 | 802.1 | |
| 0.00 | 1.41 | 0.00 | 0.70 | -7.51 | 6.00 | -8.12 | 99.43 | 0.1427 | -967.0 | -648.9 | |
| 0.00 | 0.62 | 0.00 | 0.31 | -6.70 | 5.71 | -8.41 | 93.60 | 0.1463 | -1012.0 | -819.9 | |
| 0.00 | 2.38 | 0.00 | 1.19 | -6.96 | 5.22 | -8.91 | 95.14 | 0.1551 | -919.0 | -845.7 | |
| 0.00 | 1.67 | 0.00 | 0.84 | -7.38 | 5.09 | -9.04 | 97.74 | 0.1580 | -1053.0 | -854.6 | |
| 0.00 | 1.41 | 0.00 | 0.71 | -7.55 | 4.87 | -9.26 | 98.66 | 0.1621 | -963.0 | -789.5 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -7.22 | 4.84 | -9.28 | 96.61 | 0.1618 | -947.0 | -795.9 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -7.43 | 4.69 | -9.44 | 97.77 | 0.1649 | -751.0 | -629.2 | |
| 0.00 | 1.76 | 0.00 | 0.88 | -7.36 | 4.38 | -9.74 | 97.18 | 0.1700 | -732.0 | -616.3 | |
| 0.00 | 1.14 | 0.00 | 0.58 | -12.28 | 3.48 | -10.65 | 120.65 | 0.2108 | 780.0 | 586.7 | |
| 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. | |