| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.96 | 80.90 | 7.61 | 47.28 | -18.03 | 158.58 | -19.85 | 142.51 | 0.5318 | 146.0 | 13.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-04 05:00:36 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 |
| 0.00 | 2.24 | 0.00 | 1.27 | -17.06 | 161.35 | -17.07 | 145.37 | 0.4957 | 757.0 | 700.1 | |
| 0.00 | 1.52 | 0.00 | 0.87 | -17.40 | 161.16 | -17.27 | 145.46 | 0.5015 | 669.0 | 652.2 | |
| 4.47 | 9.12 | 2.56 | 5.23 | -17.67 | 161.03 | -17.39 | 145.58 | 0.5059 | 983.1 | 744.0 | |
| 0.00 | 2.06 | 0.00 | 1.18 | -17.23 | 160.54 | -17.88 | 144.31 | 0.5047 | 905.0 | 679.3 | |
| 0.00 | 6.17 | 0.00 | 3.56 | -18.00 | 160.29 | -18.13 | 144.86 | 0.5162 | 1043.0 | 800.3 | |
| 0.00 | 1.61 | 0.00 | 0.93 | -17.63 | 160.33 | -18.09 | 144.49 | 0.5114 | 783.0 | 757.6 | |
| 0.00 | 1.16 | 0.00 | 0.66 | -16.84 | 160.35 | -18.07 | 143.55 | 0.5017 | 556.0 | 426.6 | |
| 0.00 | 3.13 | 0.00 | 1.82 | -18.32 | 159.86 | -18.57 | 144.59 | 0.5237 | 322.0 | 467.9 | |
| 0.00 | 0.98 | 0.00 | 0.57 | -18.33 | 159.59 | -18.84 | 144.22 | 0.5262 | 394.0 | 415.2 | |
| 0.00 | 2.24 | 0.00 | 1.29 | -17.70 | 159.62 | -18.80 | 143.52 | 0.5184 | 611.0 | 441.8 | |
| 0.00 | 0.89 | 0.00 | 0.52 | -18.57 | 159.52 | -18.90 | 144.40 | 0.5295 | 602.0 | 600.0 | |
| 0.00 | 1.34 | 0.00 | 0.78 | -17.97 | 159.56 | -18.86 | 143.75 | 0.5221 | 762.0 | 615.1 | |
| 0.00 | 0.89 | 0.00 | 0.51 | -15.35 | 159.76 | -18.66 | 140.75 | 0.4896 | 735.0 | 659.7 | |
| 0.00 | 0.98 | 0.00 | 0.57 | -18.71 | 159.37 | -19.05 | 144.35 | 0.5325 | 456.0 | 422.2 | |
| 0.00 | 0.89 | 0.00 | 0.52 | -18.37 | 159.41 | -19.01 | 144.02 | 0.5282 | 351.0 | 450.9 | |
| 0.00 | 3.31 | 0.00 | 1.93 | -18.42 | 159.14 | -19.29 | 143.68 | 0.5311 | 707.0 | 360.8 | |
| 0.00 | 0.63 | 0.00 | 0.37 | -18.69 | 159.07 | -19.35 | 143.90 | 0.5349 | 185.0 | 258.0 | |
| 0.00 | 1.16 | 0.00 | 0.67 | -17.72 | 159.12 | -19.30 | 142.82 | 0.5231 | 273.0 | 429.5 | |
| 0.00 | 1.16 | 0.00 | 0.67 | -16.62 | 159.10 | -19.32 | 141.44 | 0.5106 | 533.0 | 483.6 | |
| 0.00 | 0.98 | 0.00 | 0.57 | -16.67 | 158.86 | -19.56 | 141.16 | 0.5133 | 692.0 | 531.2 | |
| 0.00 | 1.07 | 0.00 | 0.63 | -18.81 | 157.97 | -20.45 | 142.53 | 0.5458 | -595.0 | -522.0 | |
| 0.00 | 1.43 | 0.00 | 0.85 | -18.68 | 157.71 | -20.71 | 142.04 | 0.5468 | -794.0 | -639.8 | |
| 0.00 | 2.32 | 0.00 | 1.36 | -17.56 | 157.55 | -20.87 | 140.45 | 0.5357 | -708.0 | -700.2 | |
| 0.00 | 0.98 | 0.00 | 0.58 | -18.37 | 157.24 | -21.18 | 141.04 | 0.5475 | -863.0 | -714.3 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -18.51 | 157.15 | -21.27 | 141.10 | 0.5499 | -476.0 | -437.3 | |
| 2.95 | 25.22 | 1.76 | 15.03 | -18.95 | 157.06 | -21.36 | 141.50 | 0.5556 | -967.5 | -737.7 | |
| 0.89 | -26.00 | 0.53 | -26.00 | -18.80 | 156.77 | -21.65 | 140.94 | 0.5565 | -966.6 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.63 | -17.82 | 156.83 | -21.59 | 139.84 | 0.5453 | -544.0 | -514.6 | |
| 0.98 | 5.01 | 0.57 | 2.91 | -15.87 | 156.86 | -21.56 | 137.37 | 0.5239 | -783.6 | -785.1 | |
| 3.67 | -26.00 | 2.19 | -26.00 | -18.81 | 156.42 | -22.00 | 140.52 | 0.5598 | -911.2 | 999999 | |
| 0.00 | 0.80 | 0.00 | 0.48 | -18.79 | 156.18 | -22.24 | 140.20 | 0.5618 | -307.0 | -406.1 | |
| 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. | |