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<strong>SPINOR</strong> & HINODE inv_070214.024925_hinode_test.tgz I/I c Δ(I/I c) [%] Q/I c [%] Δ(Q/I Δ( c) [%] 1.00 0.83 0.66 0.49 0.32 3.00 0 −3.00 14.90 7.45 0.00 −7.45 −14.90 1.75 0 −1.75 6301.5 6302.5 −0.17 0.17 −0.17 0.17 λ−λ λ−λ0 [Å] λ−λ 0 [Å] 6301.5 −0.17 0.17 λ−λ 0 [Å] FINAL ATM IC= 2 WL= 5000.0000 9 6302.5 −0.17 0.17 λ−λ 0 [Å] FINAL ATM IC= 2 WL= 5000.0000 2.4 flux tube model V/Ic [%] ] Δ(V/I c) [%] U/I c [%] Δ(U/I Δ( c) [%] 11.50 5.75 0.00 −5.75 −11.50 1.70 0 −1.70 5.00 3.33 1.67 −0.00 −1.67 1.90 0 −1.90 6301.5 6302.5 −0.17 0.17 −0.17 0.17 λ−λ λ−λ0 [Å] λ−λ 0 [Å] 6301.5 −0.17 0.17 λ−λ 0 [Å] 6302.5 −0.17 0.17 λ−λ 0 [Å] FINAL ATM IC= 2 WL= 5000.0000 A. Lagg - Abisko Winter School 26 4
Penumbral Flux Tubes �� confirms uncombed model �� flux tube thickness 100 100-300 300 km Borrero et al. 2006 A. Lagg - Abisko Winter School 27
Page 1 and 2: SPINOR Inversions based on RFs A. L
Page 3 and 4: Asymmetric profiles and ME (2) ) MH
Page 5 and 6: Example: SIR inversion + • Spatia
Page 7 and 8: SPINOR core: the synthesis RTE has
Page 9 and 10: Contribution Functions (1) The cont
Page 11 and 12: Response Functions A. Lagg - Abisko
Page 13 and 14: Response functions Linearization: s
Page 15 and 16: RFs - Example: Fe 6302.5 model on t
Page 17 and 18: The even more complex case: A. Lagg
Page 19 and 20: The complex fluxtube case: A. Lagg
Page 21 and 22: Penumbral Flux Tubes � SPINOR app
Page 23: SPINOR & HINODE inv_070214.051204_h
Page 27 and 28: 2-comp comp model Sunspot + molec c
Page 29 and 30: Penumbral Oscillations oscillations
Page 31 and 32: Penumbral Oscillations oscillations
Page 33 and 34: Analysis of Umbral Dots (1) Analysi
Page 35 and 36: Analysis of Umbral Dots (3) atmosph
Page 37 and 38: Analysis of Umbral Dots (5) Conclus
Page 39 and 40: Pore simulation: brightening nea ar
Page 41 and 42: SPINOR: Installation and first us s

SPINOR

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