15.11.2012 Views

Etude de la couronne solaire en 3D et de son évolution avec SOHO ...

Etude de la couronne solaire en 3D et de son évolution avec SOHO ...

Etude de la couronne solaire en 3D et de son évolution avec SOHO ...

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

tel-00089354, version 1 - 17 Aug 2006<br />

304 F. PORTIER-FOZZANI ET AL.<br />

Figure 12. For r1 giv<strong>en</strong> at 10 Mm, minimal variation obtained for φ1 from −90 to −80 <strong>de</strong>g, φ2 from<br />

−200 to −190 <strong>de</strong>g: minimum <strong>de</strong>viation correspond to φ1 ∼−81 <strong>de</strong>g and φ2 ∼−197 <strong>de</strong>g.<br />

Figure 13. For r1 giv<strong>en</strong> at 9 Mm, measurem<strong>en</strong>t of the minimum variation for φ1 from −90 up to<br />

−80 <strong>de</strong>g, φ2 from −200 up to −190 <strong>de</strong>g.<br />

The uncertainty calcu<strong>la</strong>tion is giv<strong>en</strong> by the sum of all uncertainties for each of<br />

the param<strong>et</strong>ers. With 30 points, a previous calcu<strong>la</strong>tion (in the main text) shows that<br />

the most discernible differ<strong>en</strong>ce b<strong>et</strong>we<strong>en</strong> the sampled loop and the mo<strong>de</strong>l is an error<br />

of 0.2 pixels. If s1 is the solution and s2 can be a solution if Error(Norm(s2 −s1)) ≤<br />

0.2 pixels. Th<strong>en</strong> for all fixed param<strong>et</strong>ers except 2, this cooresponds numerically<br />

to ∼ 4.7 <strong>de</strong>g (Portier–Fozzani, 1999). Numerical simu<strong>la</strong>tions for the uncertainties<br />

is used because ev<strong>en</strong> if the torus is a correct analytical function, a line over<br />

a torus is not a simple function and the error cannot be easily <strong>de</strong>rived.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!