A Microfilm Atlas of Magnetic Fields in the Solar Corona
This is a Microfilm atlas of magnetic fields in the solar corona. The original item included a text of 26 pages and 11,000 maps on 11 reels of microfilm. This Atlas contains 11,000 maps of the calculated potential (or current-free) magnetic fields of the solar corona between August 1959 and June 1970. For each solar rotation in this interval, there are two sets of maps. The first set of maps shows the geometry of the coronal magnetic field but includes field lines originating from both strong or weak fields at the photosphere. (However, no field lines are drawn from a photospheric region if the calculated field strength there is less than 0.08 Gauss.) The second set of maps shows field lines which emanate from the regions of strongest photospheric magnetic field. Each set provides one map for every 100 interval of solar longitude or 36 maps for each rotation.
document
http://n2t.net/ark:/85065/d7v987hn
eng
geoscientificInformation
Text
publication
2016-01-01T00:00:00Z
EARTH SCIENCE > SUN-EARTH INTERACTIONS > IONOSPHERE/MAGNETOSPHERE DYNAMICS > MAGNETIC FIELDS/MAGNETIC CURRENTS
EARTH SCIENCE > SUN-EARTH INTERACTIONS > SOLAR ACTIVITY > CORONA
revision
2021-09-17
publication
1973-01-01T00:00:00Z
Copyright Author(s). This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.
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OpenSky Support
UCAR/NCAR - Library
PO Box 3000
Boulder
80307-3000
name: homepage
pointOfContact
2023-08-18T18:05:11.721737