Add to ORKGObservations at the 1 August 2008 total solar eclipse in western China were obtained through a narrow band interference filter centered on the 530.3 nm FeXIV emission line at a cadence of 30 frames/second. A simplified analysis indicates that in a position near the base of a coronal streamer a short period intensity periodicity is found. The analysis and results are presented
International audienceContext. The origin of the high temperature of the solar corona, in both the i...
The occasion of the partial solar eclipse in Malaysia occurred on 9th March 2016 covered almost 60% ...
International audienceMeasurements of the ionospheric E region during total solar eclipses in the pe...
We performed high resolution spectroscopy of the solar corona during the total solar eclipse of 22 J...
Received; accepted Abstract. Results of the search of the periodic changes of the 530.3 nm line inte...
Encouraged by the detection of high-frequency, low-amplitude continuum intensity oscillations in the...
Results of the search of the periodic changes of the 530.3 nm line intensity emitted by selected str...
An experiment to search for short-period oscillations in the solar corona was conducted during the t...
Coronal spectra during the total solar eclipse of 1980 February 16, were obtained in the 6374Å ...
Photoelectric observations of short term light variations (shadow bands) at the 16 Feb. 1980 total s...
We obtained the images of the eastern part of the solar corona in the Fe xiv 530.3 nm (green) and ...
We report on early results from a suite of instruments for imaging and spectra we deployed to Salem,...
Spectroscopic measurements of the low solar corona are crucial to understanding the mechanisms that ...
Abstract. Coronal spectra during the total solar eclipse of 1980 February 16, were obtained in the 6...
From international astronomical union symposium on coronal disturbances; Surfers Paradise, Australia...
International audienceContext. The origin of the high temperature of the solar corona, in both the i...
The occasion of the partial solar eclipse in Malaysia occurred on 9th March 2016 covered almost 60% ...
International audienceMeasurements of the ionospheric E region during total solar eclipses in the pe...
We performed high resolution spectroscopy of the solar corona during the total solar eclipse of 22 J...
Received; accepted Abstract. Results of the search of the periodic changes of the 530.3 nm line inte...
Encouraged by the detection of high-frequency, low-amplitude continuum intensity oscillations in the...
Results of the search of the periodic changes of the 530.3 nm line intensity emitted by selected str...
An experiment to search for short-period oscillations in the solar corona was conducted during the t...
Coronal spectra during the total solar eclipse of 1980 February 16, were obtained in the 6374Å ...
Photoelectric observations of short term light variations (shadow bands) at the 16 Feb. 1980 total s...
We obtained the images of the eastern part of the solar corona in the Fe xiv 530.3 nm (green) and ...
We report on early results from a suite of instruments for imaging and spectra we deployed to Salem,...
Spectroscopic measurements of the low solar corona are crucial to understanding the mechanisms that ...
Abstract. Coronal spectra during the total solar eclipse of 1980 February 16, were obtained in the 6...
From international astronomical union symposium on coronal disturbances; Surfers Paradise, Australia...
International audienceContext. The origin of the high temperature of the solar corona, in both the i...
The occasion of the partial solar eclipse in Malaysia occurred on 9th March 2016 covered almost 60% ...
International audienceMeasurements of the ionospheric E region during total solar eclipses in the pe...