Near infrared spectral and polarization imaging observation of coronal emission lines during the 2008 total solar eclipse

Edlén B. Die Deutung der Emissionlinien im Spektrum der Sonnenkorona. Z Astrophys, 1942, 22: 30–46

Lin H, Penn M J, Tomczyk S. A new precise measurement of the coronal magnetic field strength. Astrophys J, 2000, 541: L83–L86

Lin H, Kuhn J R, Coulter R. Coronal magnetic field measurements. Astrophys J, 2004, 613: L177–180

Liu Y, Lin H. Observational test of coronal magnetic field models. I. Comparison with potential field model. Astrophys J, 2008, 680: 1496–1507

Eddy J A, Lee R H, Emerson J D. The λ10747 coronal line at the 1966 eclipse. Sol Phys, 1973, 30: 351–369

Kuhn J R, Penn M J, Mann I. The near-infrared cornal spectrum. Astrophys J, 1996, 456: L67–L70

Habbal S R, Arndt M B, Nayfeh M H, et al. On the detection of the signature of silicon nanoparticle dust grains in the coronal holes. Astrophys J, 2003, 592: L87–L90

Chevalier R A, Lambert D L. The excitation of the forbidden coronal lines. Sol Phys, 1969, 10: 115–134

Flower D R. Pineau des Forêts Excitation of the Fe XIII spectrum in the solar corona. Astron Astrophys, 1973, 24: 181–192

Penn M J, Kuhn J R, Arnaud J, et al. Coronal electron density measurement using the near-IR [FE XIII] emission lines. Space Sci Rev, 2004, 70: 185–188

Lagg A. Recent advances in measuring chromospheric magnetic fields in the He I 10830 Å line. Adv Space Res, 2007, 39: 1734–1740

Mann I, Kuhn J R, Penn M J. Infrared spectroscopic observations of neutral Helium during the 1994 eclipse. In: Gustafson B A S, Hanner M S, eds. Proceedings of the 150th colloquium of the International Astronomical Union held in Gainesville, Florida, U.S.A. 1996, 104: 345–348

Liu Y. The coronal magnetic field reversal observed by the SOLARC instrument. Sci China Ser G-Phys Mech Astron, 2009, 52: 1696–1701