SPINOR

More documents

Recommendations

Info

<strong>SPINOR</strong>: GG-band band spectrum syn thesis G-Band (Fraunhofer): spectral rang ge from 4295 to 4315 Å contains many temperature-sensitive molecular lines (CH) For comparison with observatioons, we define as G-band intensity the integral of the speectrum obtained from the simulation data: I G = 4315 ∫ 4295 A I ( λ λ ) d dλλ A 241 CH lines + 87 atomic lines [Shelyag, 2004] A. Lagg - Abisko Winter School 42
<strong>SPINOR</strong>: Installation and first us sage Download from http://www.mps .mpg.de/homes/lagg GBSO download-section � spinor use invert and IR$soft A. Lagg - Abisko Winter School 43
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 and 24: SPINOR & HINODE inv_070214.051204_h
Page 25 and 26: Penumbral Flux Tubes �� confirm
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: Pore simulation: brightening nea ar

SPINOR

You also want an ePaper? Increase the reach of your titles

Delete template?

Save as template?