Distribution of X-ray Emission from the Sun deduced from Measurements of Ionospheric Absorption

Details Distribution of X-ray Emission from the Sun deduced from Measurements of Ionospheric Absorption Distribution of X-ray Emission from the Sun deduced from Measurements of Ionospheric Absorption

Sep 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968natur.219.1139a&link_type=abstract

Nature, Volume 219, Issue 5159, pp. 1139-1141 (1968).

Physics

Scientific paper

DURING the annular solar eclipse of May 20, 1966, over parts of northern Africa and southern Europe, solar flux and ionospheric absorption measurements were made from several points along the central line of the path of the eclipse. Solar flux was measured at various frequencies in the cm and mm bands. All the data obtained during the eclipse showed characteristic variations in flux related to local active sources on the solar disk. Fig. 1 shows the distribution of local sources on the solar disk measured in Athens by Castelli on 2,695 MHz (private communication). Three sources giving an increase in flux were identified during this eclipse: one on the west limb, the second in the middle of the disk and the third on the east limb. Two sources of less importance were also identified on the north-east part of the disk.

Affiliated with

Also associated with

No associations

Rating

Distribution of X-ray Emission from the Sun deduced from Measurements of Ionospheric Absorption does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Distribution of X-ray Emission from the Sun deduced from Measurements of Ionospheric Absorption, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Distribution of X-ray Emission from the Sun deduced from Measurements of Ionospheric Absorption will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1788268