The behavior of filaments and prominences during the Solar Cycle is a signature of Sun's activity. It is therefore important to follow their evolution during the cycle, in order to be able to associate it with the various phases of the Solar Cycle as well as with other Solar features or events. The virtual observatory HELIO provides information that can be used for such studies, especially its Heliophysics Feature Catalogue gives a unique access to the description of various features during around one cycle. Features available are: filaments, prominences, photospheric and coronal active regions, coronal radio emission, type III radio bursts, coronal holes and sunspots. Web interfaces allow the user to query data for these features. Useful i...
The objective of the research in this dissertation is to develop a software system to automatically ...
This volume presents the latest research results on solar prominences, including new developments on...
We present the results of a comparative study between automatic and manually compiled coronal mass e...
A new algorithm for automatic detection of prominences on the solar limb in 304 Å EUV images is pres...
International audienceIn Fall 2008 NASA selected a large international consortium to produce a compr...
We present a statistical analysis of coronal mass ejections (CMEs) imaged by the Heliospheric Imager...
YesIn this study a method for 3D representation of active regions and sunspots that are detected fro...
International audienceThe Solar Feature Catalogues (SFCs) are created from digitized solar images us...
noThe Solar Feature Catalogues (SFCs) are created from digitized solar images using automated patter...
International audienceThe searchable Solar Feature Catalogues (SFCs) are developed from digitized so...
The massive repository of images of the Sun captured by the Solar Dynamics Observatory (SDO) mission...
Recent observations with the Heliospheric Imagers (HIs) onboard the twin NASA Solar Terrestrial Rela...
Recent observations with the Heliospheric Imagers (HIs) onboard the twin NASA Solar Terrestrial Rela...
The immense volume of data generated by the suite of instruments on SDO requires new tools for effic...
A new algorithm for automatic detection of prominences on the solar limb in 304 A EUV images is pres...
The objective of the research in this dissertation is to develop a software system to automatically ...
This volume presents the latest research results on solar prominences, including new developments on...
We present the results of a comparative study between automatic and manually compiled coronal mass e...
A new algorithm for automatic detection of prominences on the solar limb in 304 Å EUV images is pres...
International audienceIn Fall 2008 NASA selected a large international consortium to produce a compr...
We present a statistical analysis of coronal mass ejections (CMEs) imaged by the Heliospheric Imager...
YesIn this study a method for 3D representation of active regions and sunspots that are detected fro...
International audienceThe Solar Feature Catalogues (SFCs) are created from digitized solar images us...
noThe Solar Feature Catalogues (SFCs) are created from digitized solar images using automated patter...
International audienceThe searchable Solar Feature Catalogues (SFCs) are developed from digitized so...
The massive repository of images of the Sun captured by the Solar Dynamics Observatory (SDO) mission...
Recent observations with the Heliospheric Imagers (HIs) onboard the twin NASA Solar Terrestrial Rela...
Recent observations with the Heliospheric Imagers (HIs) onboard the twin NASA Solar Terrestrial Rela...
The immense volume of data generated by the suite of instruments on SDO requires new tools for effic...
A new algorithm for automatic detection of prominences on the solar limb in 304 A EUV images is pres...
The objective of the research in this dissertation is to develop a software system to automatically ...
This volume presents the latest research results on solar prominences, including new developments on...
We present the results of a comparative study between automatic and manually compiled coronal mass e...