On estimation of the i l hi k i l optical thickness in solar i prominences
On estimation of the i l hi k i l optical thickness in solar i prominences
On estimation of the i l hi k i l optical thickness in solar i prominences
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Method<br />
• Pr<strong>of</strong>ile <strong>of</strong> Hα emission l<strong>in</strong>e <strong>of</strong> a prom<strong>in</strong>ence, with<br />
some approximations i can be represented with<br />
function:<br />
I S e<br />
=<br />
λ<br />
2<br />
( λλ − max2<br />
)<br />
−<br />
2<br />
τ e<br />
∆λ<br />
(1 −<br />
d<br />
0 ⋅<br />
)
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