| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 90.61 | 351.83 | 52.02 | 201.34 | 10.43 | 142.97 | -24.52 | 54.64 | 0.5007 | -152.3 | -98.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-25 16:00:31 UT
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 |
| 22.54 | 176.83 | 12.55 | 98.51 | 10.09 | 146.21 | -21.28 | 51.59 | 0.4579 | -1282.8 | -429.8 | |
| 7.78 | -1.00 | 4.34 | -1.00 | 10.07 | 145.92 | -21.57 | 52.00 | 0.4613 | -1079.8 | 999999 | |
| 5.42 | -1.00 | 3.03 | -1.00 | 10.48 | 145.82 | -21.67 | 51.42 | 0.4663 | -831.3 | 999999 | |
| 0.87 | -1.00 | 0.49 | -1.00 | 10.56 | 145.42 | -22.07 | 51.80 | 0.4719 | -716.5 | 999999 | |
| 0.00 | 1.75 | 0.00 | 0.98 | 10.77 | 145.08 | -22.41 | 51.89 | 0.4780 | -433.0 | -429.0 | |
| 1.14 | 2.53 | 0.64 | 1.43 | 10.49 | 144.44 | -23.05 | 53.14 | 0.4831 | -931.8 | -712.9 | |
| 0.00 | 0.70 | 0.00 | 0.40 | 10.67 | 144.43 | -23.06 | 52.85 | 0.4850 | -750.0 | -666.5 | |
| 3.06 | 6.20 | 1.72 | 3.50 | 9.87 | 144.35 | -23.13 | 54.30 | 0.4786 | -984.4 | -761.8 | |
| 0.00 | 2.45 | 0.00 | 1.39 | 10.81 | 144.22 | -23.27 | 52.87 | 0.4888 | -449.0 | -504.6 | |
| 0.00 | 0.96 | 0.00 | 0.55 | 10.94 | 144.04 | -23.45 | 52.86 | 0.4921 | -596.0 | -454.3 | |
| 0.00 | 0.87 | 0.00 | 0.50 | 10.70 | 143.36 | -24.13 | 54.06 | 0.4982 | -651.0 | -478.3 | |
| 3.76 | 5.68 | 2.14 | 3.23 | 9.99 | 143.12 | -24.37 | 55.51 | 0.4951 | -984.5 | -742.0 | |
| 0.00 | 0.96 | 0.00 | 0.55 | 10.54 | 142.87 | -24.62 | 54.87 | 0.5027 | -745.0 | -608.7 | |
| 8.82 | 16.77 | 5.04 | 9.58 | 9.83 | 142.60 | -24.89 | 56.35 | 0.5003 | -966.9 | -728.5 | |
| 0.00 | 2.36 | 0.00 | 1.35 | 10.62 | 142.50 | -24.99 | 55.15 | 0.5081 | -774.0 | -638.9 | |
| 0.00 | 0.87 | 0.00 | 0.50 | 10.48 | 142.14 | -25.35 | 55.76 | 0.5113 | -588.0 | -458.2 | |
| 0.00 | 1.14 | 0.00 | 0.66 | 9.91 | 141.24 | -26.25 | 57.63 | 0.5178 | 669.0 | 432.5 | |
| 0.00 | 1.05 | 0.00 | 0.61 | 9.66 | 141.20 | -26.29 | 58.08 | 0.5165 | 799.0 | 701.6 | |
| 0.00 | 1.22 | 0.00 | 0.72 | 11.55 | 140.37 | -27.12 | 55.86 | 0.5417 | 712.0 | 586.8 | |
| 0.00 | 1.40 | 0.00 | 0.82 | 10.91 | 140.13 | -27.36 | 57.11 | 0.5396 | 773.0 | 637.6 | |
| 0.00 | 1.05 | 0.00 | 0.61 | 10.53 | 140.16 | -27.32 | 57.68 | 0.5362 | -647.0 | -452.3 | |
| 4.46 | 71.03 | 2.63 | 42.12 | 11.37 | 139.74 | -27.75 | 56.76 | 0.5479 | 948.6 | 552.9 | |
| 0.00 | 1.05 | 0.00 | 0.62 | 9.67 | 139.32 | -28.17 | 59.84 | 0.5404 | 544.0 | 483.2 | |
| 25.16 | -22.00 | 14.94 | -22.00 | 11.12 | 139.10 | -28.38 | 57.73 | 0.5538 | 970.0 | 999999 | |
| 0.00 | 2.10 | 0.00 | 1.25 | 11.63 | 138.98 | -28.51 | 57.06 | 0.5592 | 585.0 | 461.0 | |
| 0.00 | 1.66 | 0.00 | 0.98 | 10.28 | 139.12 | -28.37 | 59.05 | 0.5473 | 823.0 | 743.2 | |
| 0.00 | 1.14 | 0.00 | 0.67 | 9.84 | 139.09 | -28.39 | 59.77 | 0.5444 | 833.0 | 681.7 | |
| 0.00 | 2.10 | 0.00 | 1.24 | 10.14 | 138.86 | -28.63 | 59.51 | 0.5495 | 1021.0 | 890.7 | |
| 1.31 | 7.25 | 0.77 | 4.29 | 9.86 | 138.85 | -28.64 | 59.96 | 0.5476 | 1011.1 | 777.4 | |
| 1.83 | 32.06 | 1.09 | 19.16 | 10.91 | 138.54 | -28.95 | 58.58 | 0.5591 | 900.7 | 324.3 | |
| 2.80 | 7.25 | 1.65 | 4.29 | 9.56 | 138.57 | -28.92 | 60.68 | 0.5491 | 791.6 | 516.0 | |
| 1.66 | -30.00 | 0.99 | -30.00 | 10.79 | 138.44 | -29.04 | 58.85 | 0.5594 | 818.9 | 999999 | |
| 0.00 | 1.40 | 0.00 | 0.83 | 9.85 | 138.40 | -29.09 | 60.36 | 0.5533 | 684.0 | 533.1 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |