𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Variability of the integrated solar K line emission

✍ Scribed by V. Bumba; B. Růžičková-Topolová


Publisher
Springer
Year
1967
Tongue
English
Weight
155 KB
Volume
1
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


📜 SIMILAR VOLUMES


Kα line emission during solar X-ray burs
✍ K. J. H. Phillips; W. M. Neupert 📂 Article 📅 1973 🏛 Springer 🌐 English ⚖ 770 KB

Kct X-ray line emission from S, Ar, Ca and Fe is calculated for conditions likely to exist in solar flares. We consider both the non-thermal and thermal phases of flares as indicated by X-ray observations. Impulsive non-thermal events seen at the onset of a flare at photon energies > 20 keV generall

Variations of the asymmetry of disk-inte
✍ David H. Bruning; Barry LaBonte 📂 Article 📅 1985 🏛 Springer 🌐 English ⚖ 335 KB

Mean line bisector positions were found for the neutral iron line at 25250.2 using disk-integrated sunlight. After correction for the apparent time variation of the instrumental profile, it was found that the mean bisector position was constant during the period from May 1982 to February 1983. The c

The relationship between solar activity
✍ Dennis E. Jebsen; Walter E. Mitchell 📂 Article 📅 1978 🏛 Springer 🌐 English ⚖ 446 KB

In this paper we present and analyze new data on the cores of the H and K lines of ionized calcium in the spectrum of integrated sunlight. The intensities of the components n2v, H3, HEr, KEy, K3, and K2r in the line cores were measured in terms of the continuum intensity at 4000 ~ during a solar rot

On the polarization of the solar coronal
✍ E. Mogilevsky; B. Ioshpa; V. Obridko 📂 Article 📅 1973 🏛 Springer 🌐 English ⚖ 694 KB

The results of the spectrophotometrical measurements of the polarization in the coronal lines Fe xIv 5303 fit and Fe x 6374 fit are given. Polarization spectrograms were obtained by two spectrographs (prism and echelle types) during the solar eclipse in Mexico on 7 March, 1970 near the region of the