| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.61 | 58.82 | 0.32 | 31.57 | -10.55 | 300.93 | -21.99 | 100.38 | 0.3791 | 416.7 | 325.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-13 21:00:29 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 | 1.65 | 0.00 | 0.84 | -10.52 | 310.21 | -12.72 | 105.73 | 0.2260 | 774.0 | 589.2 | |
| 0.00 | 1.04 | 0.00 | 0.54 | -17.99 | 309.63 | -13.30 | 131.03 | 0.2914 | 817.0 | 614.1 | |
| 0.00 | 1.30 | 0.00 | 0.67 | -13.15 | 307.30 | -15.63 | 112.42 | 0.2851 | 941.0 | 833.3 | |
| 0.00 | 1.65 | 0.00 | 0.85 | -13.28 | 306.65 | -16.28 | 112.11 | 0.2957 | 884.0 | 749.7 | |
| 0.00 | 1.39 | 0.00 | 0.72 | -10.61 | 304.92 | -18.01 | 102.17 | 0.3123 | 820.0 | 633.6 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -6.70 | 304.93 | -18.00 | 89.53 | 0.3083 | 642.0 | 527.8 | |
| 0.00 | 1.56 | 0.00 | 0.82 | -10.63 | 304.69 | -18.24 | 102.13 | 0.3160 | 857.0 | 723.9 | |
| 0.00 | 2.08 | 0.00 | 1.09 | -13.12 | 304.10 | -18.83 | 109.24 | 0.3345 | 800.0 | 570.6 | |
| 0.00 | 1.48 | 0.00 | 0.77 | -11.07 | 303.77 | -19.16 | 103.00 | 0.3321 | 955.0 | 827.7 | |
| 0.00 | 1.39 | 0.00 | 0.73 | -13.08 | 303.16 | -19.77 | 108.42 | 0.3488 | 755.0 | 657.6 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -12.96 | 303.04 | -19.89 | 107.99 | 0.3501 | 764.0 | 641.6 | |
| 0.00 | 2.34 | 0.00 | 1.23 | -8.87 | 303.17 | -19.76 | 96.22 | 0.3375 | 790.0 | 594.6 | |
| 0.00 | 0.78 | 0.00 | 0.41 | -12.08 | 302.92 | -20.01 | 105.46 | 0.3487 | 741.0 | 624.4 | |
| 0.00 | 5.64 | 0.00 | 2.97 | -9.13 | 303.09 | -19.84 | 96.99 | 0.3391 | 911.0 | 687.1 | |
| 0.00 | 2.08 | 0.00 | 1.10 | -10.77 | 302.92 | -20.01 | 101.71 | 0.3448 | 727.0 | 648.9 | |
| 0.61 | 1.91 | 0.32 | 1.01 | -11.21 | 302.73 | -20.20 | 102.88 | 0.3491 | 940.0 | 824.0 | |
| 0.00 | 1.30 | 0.00 | 0.69 | -11.17 | 302.53 | -20.40 | 102.69 | 0.3520 | 611.0 | 539.1 | |
| 0.00 | 3.12 | 0.00 | 1.65 | -10.57 | 302.45 | -20.48 | 100.95 | 0.3519 | 569.0 | 581.2 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -10.38 | 302.30 | -20.63 | 100.37 | 0.3539 | 669.0 | 603.0 | |
| 0.00 | 1.48 | 0.00 | 0.78 | -2.80 | 302.16 | -20.77 | 79.04 | 0.3624 | 993.0 | 877.1 | |
| 0.00 | 1.48 | 0.00 | 0.78 | -3.90 | 302.10 | -20.83 | 82.08 | 0.3597 | 825.0 | 714.5 | |
| 0.00 | 0.87 | 0.00 | 0.46 | -4.85 | 301.46 | -21.47 | 84.95 | 0.3677 | 770.0 | 646.9 | |
| 0.00 | 2.26 | 0.00 | 1.20 | -5.06 | 301.33 | -21.60 | 85.54 | 0.3694 | 836.0 | 705.8 | |
| 0.00 | 1.91 | 0.00 | 1.02 | -4.66 | 301.05 | -21.88 | 84.56 | 0.3747 | 819.0 | 679.6 | |
| 0.00 | 1.30 | 0.00 | 0.71 | -6.21 | 298.11 | -24.81 | 89.21 | 0.4190 | 805.0 | 589.4 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -6.36 | 298.07 | -24.86 | 89.56 | 0.4195 | 719.0 | 482.6 | |
| 0.00 | 3.73 | 0.00 | 2.09 | -13.97 | 295.67 | -27.26 | 106.48 | 0.4654 | -638.0 | -732.7 | |
| 0.00 | 1.48 | 0.00 | 0.82 | -4.57 | 296.09 | -26.83 | 85.89 | 0.4530 | 522.0 | 514.7 | |
| 0.00 | 1.48 | 0.00 | 0.83 | -13.73 | 294.59 | -28.34 | 105.55 | 0.4806 | -857.0 | -725.7 | |
| 0.00 | 2.60 | 0.00 | 1.49 | -15.57 | 293.55 | -29.38 | 108.82 | 0.5014 | -928.0 | -825.8 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -15.12 | 293.58 | -29.35 | 107.95 | 0.4994 | -811.0 | -723.7 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -7.95 | 294.20 | -28.73 | 93.42 | 0.4789 | -718.0 | -609.2 | |
| 0.00 | 2.00 | 0.00 | 1.14 | -15.40 | 293.29 | -29.64 | 108.38 | 0.5045 | -873.0 | -742.6 | |
| 0.00 | 0.43 | 0.00 | 0.25 | -15.67 | 293.25 | -29.68 | 108.89 | 0.5060 | -644.0 | -546.0 | |
| 0.00 | 0.26 | 0.00 | 0.15 | -9.22 | 293.36 | -29.57 | 96.02 | 0.4918 | -303.0 | -379.7 | |
| 0.00 | 1.04 | 0.00 | 0.60 | -15.56 | 292.51 | -30.42 | 108.38 | 0.5160 | -651.0 | -468.8 | |
| 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. | |