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

<table>Influence of Eckert number Ec on the temperature profiles when Pr = 0.3, Ha = 1, <svg height="12.4375" id="M81" 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 Bi = 0.3.</table>

Mathematical Problems in Engineering

fig6

Figure 6

Figure 6: Hydromagnetic Stagnation-Point Flow towards a Radially Stretching Convectively Heated Disk 