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The Method of Moments in Electromagnetics

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A Brief Review <strong>of</strong> <strong>Electromagnetics</strong> 11<strong>of</strong> practical <strong>in</strong>terest, however, it may be difficult or impossible to directly solvethese equations for the fields. To remedy this, we derive a set <strong>of</strong> auxiliary vectorpotentials that can also be used to solve for the radiated fields. <strong>The</strong>se potentials areobta<strong>in</strong>ed via <strong>in</strong>tegrals <strong>of</strong> the currents, and the radiated fields are obta<strong>in</strong>ed directlyfrom the potentials. Vector potential formulations are used extensively <strong>in</strong> the analysis<strong>of</strong> antenna radiation and scatter<strong>in</strong>g problems, and we will use them frequentlythroughout this book. <strong>The</strong>se formulations are very similar to the <strong>in</strong>tegral equationsderived <strong>in</strong> Section 2.3, with slight differences that will be addressed.2.4.1 Magnetic Vector PotentialWe will first derive a magnetic vector potential for a homogeneous, source-freeregion. We beg<strong>in</strong> by observ<strong>in</strong>g that s<strong>in</strong>ce the magnetic field H is always solenoidal,it can be written as the curl <strong>of</strong> another vector A, which is arbitrary. <strong>The</strong>refore, wewriteH ½ Ö¢A (2.53)Substitut<strong>in</strong>g the above <strong>in</strong>to (2.1), we getwhich can be written asWe next use the identityÖ¢E Ö¢A (2.54)Ö¢´E · Aµ ¼ (2.55)Ö¢´ Ö¨µ ¼ (2.56)to writeE A Ö¨ (2.57)where ¨ is an arbitrary electric scalar potential. We next use the identityÖ¢Ö¢A Ö´Ö¡Aµ Ö ¾ A (2.58)and take the curl <strong>of</strong> both sides <strong>of</strong> (2.53), which allows us to writeand comb<strong>in</strong><strong>in</strong>g this with equation (2.2) leads toSubstitut<strong>in</strong>g (2.57) <strong>in</strong>to the above leads toÖ¢H Ö´Ö¡Aµ Ö ¾ A (2.59)J · ¯E Ö´Ö¡Aµ Ö ¾ A (2.60)J · ¯´ A Ö¨µ Ö´Ö¡Aµ Ö ¾ A (2.61)which isÖ ¾ A · ¾ A J · Ö´Ö¡A · ¯¨µ (2.62)

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