FeXIV Line Emission Polarization of the July 11, 1991 Solar Corona
1994 ◽
Vol 144
◽
pp. 541-547
Keyword(s):
AbstractHigh resolution images, obtained during July 11, 1991 total solar eclipse, allowed us to estimate the degree of solar corona polarization in the light of FeXIV 530.3 nm emission line and in the white light, as well. Very preliminary analysis reveals remarkable differences in the degree of polarization for both sets of data, particularly as for level of polarization and its distribution around the Sun’s limb.
1994 ◽
Vol 144
◽
pp. 565-566
◽
1974 ◽
Vol 57
◽
pp. 485-487
1994 ◽
Vol 144
◽
pp. 593-596
Keyword(s):
1998 ◽
Vol 15
(1)
◽
pp. 165-166
Keyword(s):