ISSN:
1573-093X
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract Using high resolution (3–5″) rocket spectroheliograms obtained by NRL, we have analyzed hundreds of small, bright, quiet Sun features to determine the heights of formation of five transition zone lines: He i 584, He ii 304, O v 630, Ne vii 465, and Mg ix 368. The results are in excellent agreement with theoretical model calculations.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00154974
Permalink