Emission gradient curves for extreme ultraviolet (EUV) resonance lines of O vI and Mg x have been constructed from spectroheliograms of quiet limb regions observed with the Harvard experiment on Skylab. An analysis of these data suggests that the coronal temperature rises throughout the height range
Does the ion cyclotron exist in the inner corona?
โ Scribed by N.-E. Raouafi
- Publisher
- John Wiley and Sons
- Year
- 2003
- Tongue
- English
- Weight
- 385 KB
- Volume
- 324
- Category
- Article
- ISSN
- 0004-6337
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
The [ 1,3]-hydrogen shift in cyclopropene has been investigated by ab initio calculations. At Hartree-Fock and Moller-Plesset levels of theory the Woodward-Hoffmann forbidden suprafacial hydrogen migration is calculated to be a concerted reaction, although the energy of the transition structure at l
The energy balance equation for a general solar atmosphere without assuming the planeparallel approximation is solved analytically. This leads to models for both the transition region and inner corona as well as for the outer corona. The form of the latter is very similar to that of the hydrostatic