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<strong>SPINOR</strong>: Versatility<br />
� Plane-parallel, 1-component models to<br />
obtain averaged properties of the<br />
atmosphere<br />
� Multiple components (e.g. to take caree<br />
of scattered light, or unresolved<br />
features on the Sun). Allows for arbitraary<br />
number of magnetic or field-free<br />
components (turns out to be important,<br />
e.g. in flare observations, where we<br />
have seen 4-5 components).<br />
� Flux-tubes in total pressure equilibriumm<br />
with surroundings, at arbitrary<br />
inclination<br />
� in field-free (or weak-field surrounddings)<br />
� embedded in strong fields (e.g. sunnspot<br />
penumbra, or umbral dots)<br />
� includes the presence of multiple flux<br />
tubes along a ray when computing<br />
away from disk centre<br />
�� efficient computation of lines acros s jumps in atmospheric quantities<br />
� Integration over solar or stellar disk, inncluding<br />
solar/stellar rotation<br />
� molecular lines (S. ( Berdyugina) y g )<br />
� non-LTE (MULTI 2.2, not tested yet, reequires<br />
brave MULTI expert)<br />
A. Lagg - Abisko Winter School 22
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