Add to ORKGAbstract. In this paper we present new results of spectra-photometrical investigations of the flaring kernels ’ sizes and their intensities measured simultaneously in various parts of the Hα line profile. Our investigations were based on the very high temporal resolution spectral-imaging observa-tions of the solar flares collected with Large Coronagrap
From international astronomical union symposium on coronal disturbances; Surfers Paradise, Australia...
Results of the search of the periodic changes of the 530.3 nm line intensity emitted by selected str...
During the past year we have been working with the HESSI (High Energy Solar Spectroscopic Imager) te...
In this paper we present new results of spectra-photometrical investigations of the flaring kernels...
International audienceThe Multichannel Subtractive Double Pass (MSDP) is an imaging spectroscopy tec...
Spectral imaging is a fundamental diagnostic technique for the study of the solar coronal plasma, an...
We present a unique design of a post-focal instrument suitable to detect fast changes of flux in wav...
During the recent solar maximum the combination of imaging and spectroscopy in the visible part of t...
International audienceContext. The origin of the high temperature of the solar corona, in both the i...
Received; accepted Abstract. Results of the search of the periodic changes of the 530.3 nm line inte...
International audienceSWAP images from PROBA2 taken at 174 Å in the Fe ix/ x lines are compared with...
International audienceObservations of the dynamics of solar coronal structures are necessary to inve...
We report the results of a high temporal resolution spectroscopic monitoring of the flare star AD Le...
Spectrometers provide our most detailed diagnostics of the solar coronal plasma, and spectral data i...
Soft X-ray spectroscopy of the Sun is an important tool to understand the coronal dynamics and compo...
From international astronomical union symposium on coronal disturbances; Surfers Paradise, Australia...
Results of the search of the periodic changes of the 530.3 nm line intensity emitted by selected str...
During the past year we have been working with the HESSI (High Energy Solar Spectroscopic Imager) te...
In this paper we present new results of spectra-photometrical investigations of the flaring kernels...
International audienceThe Multichannel Subtractive Double Pass (MSDP) is an imaging spectroscopy tec...
Spectral imaging is a fundamental diagnostic technique for the study of the solar coronal plasma, an...
We present a unique design of a post-focal instrument suitable to detect fast changes of flux in wav...
During the recent solar maximum the combination of imaging and spectroscopy in the visible part of t...
International audienceContext. The origin of the high temperature of the solar corona, in both the i...
Received; accepted Abstract. Results of the search of the periodic changes of the 530.3 nm line inte...
International audienceSWAP images from PROBA2 taken at 174 Å in the Fe ix/ x lines are compared with...
International audienceObservations of the dynamics of solar coronal structures are necessary to inve...
We report the results of a high temporal resolution spectroscopic monitoring of the flare star AD Le...
Spectrometers provide our most detailed diagnostics of the solar coronal plasma, and spectral data i...
Soft X-ray spectroscopy of the Sun is an important tool to understand the coronal dynamics and compo...
From international astronomical union symposium on coronal disturbances; Surfers Paradise, Australia...
Results of the search of the periodic changes of the 530.3 nm line intensity emitted by selected str...
During the past year we have been working with the HESSI (High Energy Solar Spectroscopic Imager) te...