Hydromagnetic Stagnation-Point Flow towards a Radially Stretching Convectively Heated Disk

<table>Influence of Ha on the velocity profiles when <svg height="12.4375" id="M59" style="vertical-align:-0.1638pt" version="1.1" viewbox="0 0 37.087502 12.4375" width="37.087502" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
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</svg>, Pr = 0.71, Bi = 0.3, and Ec = 0.2.</table>

Mathematical Problems in Engineering

fig2

Figure 2

Figure 2: Hydromagnetic Stagnation-Point Flow towards a Radially Stretching Convectively Heated Disk 