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In this section, the data is presented. Further discussion and results are presented in section 18.4.
A18.3.1 SST-416/APL
For yoke SST-416/APL measurements of the magnetic field intensity were taken at separations of 0.10 inches in three planes (X, Y = +.1, Z), (X, Y = 0, Z) and (X, Y = -.1, Z). The data for Configuration I are presented in Figures A18-4 through A18-6 and for Configuration II in Figures A18-7 through A18-9. In the formats shown, the yoke outline indicates the outside dimensions to scale and the magnet outline is a projection onto the Y = 0 plane. Also shown in this format is the location of the solid-state detector. It can be seen that the peak field in the Y = 0 plane is 1840 Gauss at X = 0.7 inches from the front surface into the yoke.
Figure A18-4 Yoke SST 416/APL, Configuration I, Magnets 1 and 2, Y=+0.1" | |
Figure A18-5 Yoke SST 416/APL, Configuration I, Magnets 1 and 2, Y=0 | |
Figure A18-6 Yoke SST 416/APL, Configuration I, Magnets 1 and 2, Y=-0.1" | |
Figure A18-7 Yoke SST 416/APL, Configuration II, Magnets 1 and 2, Y=+0.1" | |
Figure A18-8 Yoke SST 416/APL, Configuration II, Magnets 1 and 2, Y=0 | |
Figure A18-9 Yoke SST 416/APL, Configuration II, Magnets 1 and 2, Y=-0.1" |
The data is presented in a different format in Figures A18-10 through A18-12 for Configuration I and Figures A18-13 through A18-15 for Configuration II. This format is similar to the Voyager magnet presentations. Again, it can be seen that for Configuration I, the peak field is 1840 Gauss at X = 0.7 inches in the Y = 0 plane, while for configuration II the peak field is 1480 Gauss at X = 0.9 inches from the front plate. In general, the shape of the field intensity curve is similar to that of the Voyager magnets.
Figure A18-10 Yoke SST 416/APL, Configuration I, Magnets 1 and 2, Y=+0.1" , graphical form | |
Figure A18-11 Yoke SST 416/APL, Configuration I, Magnets 1 and 2, Y=0, graphical form | |
Figure A18-12 Yoke SST 416/APL, Configuration I, Magnets 1 and 2, Y=-0.1", graphical form | |
Figure A18-13 Yoke SST 416/APL, Configuration II, Magnets 1 and 2, Y=+0.1", graphical form | |
Figure A18-14 Yoke SST 416/APL, Configuration II, Magnets 1 and 2, Y=0, graphical form | |
Figure A18-15 Yoke SST 416/APL, Configuration II, Magnets 1 and 2, Y=-0.1", graphical form |
With this yoke in Configuration I, field intensities were measured along the centerline for different pairs of magnets. This data is presented in tabular form, rather than a graph, in Table A18-1.
Table A18-1 Solar Polar Magnetic Field Survey Yoke: SST416/APL (w/o hole). Magnet configuration I. Magnetic field (Gauss)
Magnet Pairs | ||||||
X (in) | Y (in) | Z (in) | 1 & 2 | 3 & 4 | 5 & 6 | 7 & 8 |
-0.4 | 0 | 0 | 28 | 28.4 | 27.8 | 26.1 |
-0.3 | 0 | 0 | 44 | 46.3 | 45.3 | 42.0 |
-0.2 | 0 | 0 | 74 | 76.9 | 75.5 | 69.8 |
-0.1 | 0 | 0 | 123 | 126 | 124 | 115 |
0 | 0 | 0 | 204 | 207 | 205 | 189 |
0.1 | 0 | 0 | 324 | 332 | 324 | 303 |
0.2 | 0 | 0 | 505 | 520 | 508 | 473 |
0.3 | 0 | 0 | 770 | 788 | 765 | 714 |
0.4 | 0 | 0 | 1080 | 1110 | 1070 | 1010 |
0.5 | 0 | 0 | 1420 | 1470 | 1390 | 1340 |
0.6 | 0 | 0 | 1720 | 1780 | 1660 | 1630 |
0.7 | 0 | 0 | 1840 | 1920 | 1760 | 1760 |
0.8 | 0 | 0 | 1720 | 1790 | 1610 | 1670 |
0.9 | 0 | 0 | 1330 | 1390 | 1210 | 1310 |
1.0 | 0 | 0 | 876 | 905 | 772 | 870 |
1.1 | 0 | 0 | 492 | 505 | 423 | 492 |
1.2 | 0 | 0 | 242 | 246 | 206 | 246 |
1.3 | 0 | 0 | 94.5 | 92.4 | 76.7 | 97.5 |
A18.3.2 SST-416/UCB
Yoke SST-416/UCB is similar to SST-416/APL except that it has a hole in the yoke which could accommodate a detector mount. Measurements of the magnetic field intensity were made only along the yoke centerline for Configuration I, but using the same magnet pair as used for the SST-416/APL yoke measurements. The data is presented in tabular form in Figure A18-16 and in graphical form in Figure A18-17. It can be seen that although the peak fields occur in the same location--0.7 inches from the front surface--the magnitude of SST-416/UCB is only 1750 Gauss compared to 1840 Gauss for SST-416/APL. This is probably due to an increase in leakage flux in the vicinity of the detector mounting hole and thereby a reduction in field in the center of the yoke.
Figure A18-16 Yoke SST 416/UCB, Configuration I, Magnets 1 and 2, Y=0 | |
Figure A18-17 Yoke SST 416/UCB, Configuration I, Magnets 1 and 2, Y=0, graphical form |
A18.3.3 C49/APL
Because of the high value of leakage flux from the stainless steel, a yoke of higher permeability material--Carpenter 49--was constructed. The initial C49 yoke had heavy wall thicknesses and no hole for a detector mount. The only magnetic field intensity measurements for the C49/APL yoke were made along the centerline in Configuration I. This data is presented in Figure A18-18 and in graphical form in Figure A18-19. It can be seen that the peak field value is 1890 Gauss, located at 0.7 inches from the front surface.
Figure A18-18 Carpenter 49/APL, Configuration I, Magnets 1 and 2, Y=0 | |
Figure A18-19 Carpenter 49/APL, Configuration I, Magnets 1 and 2, Y=0, graphical form |
Next: A18.3.4 C49/Mod I
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Updated 11/19/02, T. Hunt-Ward
Figure reconstruction by T. Manweiler.