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

<table> Influence of Hartmann number Bi on the temperature profiles when Pr = 0.3, Bi = 0.3, <svg height="12.4375" id="M84" style="vertical-align:-0.1638pt" version="1.1" viewbox="0 0 49.125 12.4375" width="49.125" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
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</svg>, and Ec = 0.2.</table>

Mathematical Problems in Engineering

fig7

Figure 7

Figure 7: Hydromagnetic Stagnation-Point Flow towards a Radially Stretching Convectively Heated Disk 