SDO HMI 2014-06-06 14:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.96 | 0.00 | 9.20 | 5.06 | 261.72 | -22.23 | 74.39 | 0.3856 | 77.6 | 60.7 | |
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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 | 2.08 | 0.00 | 1.05 | 5.44 | 273.54 | -10.40 | 62.11 | 0.2043 | -817.0 | -597.4 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 4.92 | 273.52 | -10.43 | 64.47 | 0.2007 | -1052.0 | -874.1 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 5.26 | 273.42 | -10.53 | 63.18 | 0.2048 | -917.0 | -766.9 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 3.19 | 273.04 | -10.90 | 73.51 | 0.1978 | -856.0 | -593.4 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 2.49 | 268.17 | -15.78 | 80.84 | 0.2764 | -750.0 | -503.5 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 8.16 | 260.34 | -23.61 | 70.27 | 0.4229 | 773.0 | 610.6 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 5.74 | 259.33 | -24.62 | 76.40 | 0.4282 | 746.0 | 613.9 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 5.19 | 257.96 | -25.98 | 78.25 | 0.4475 | 774.0 | 528.0 | |
| 0.00 | 1.36 | 0.00 | 0.76 | 5.53 | 256.30 | -27.64 | 78.18 | 0.4737 | 549.0 | 451.0 | |
| 0.00 | 1.54 | 0.00 | 0.88 | 4.68 | 253.86 | -30.08 | 80.70 | 0.5082 | 756.0 | 580.1 | |
| 0.00 | 1.09 | 0.00 | 0.62 | 3.73 | 253.87 | -30.08 | 82.56 | 0.5064 | 750.0 | 591.4 | |
| 0.00 | 1.00 | 0.00 | 0.60 | 5.93 | 249.48 | -34.46 | 79.56 | 0.5745 | 564.0 | 528.6 | |
| 0.00 | 1.09 | 0.00 | 0.69 | 5.39 | 245.44 | -38.50 | 81.36 | 0.6292 | 489.0 | 387.0 | |
| 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. | |