<p>These plots are time-elongation maps (J-maps) built from the STEREO Heliospheric Imager data (from HI1 and HI2). Overlaid on these J-maps are the time-elongation profiles of CMEs tracked by three different methods; Solar Stormwatch (blue squares), RAL-HI (pink triangles) and J-tracker (green dots). Above and to the right of each profile is a number identifying each event in their respective catalogues. These plots were used to generate a matched event list to enable the comparison of the time-elongation profiles.</p> <p> </p> <p>The resulting article is available at http://onlinelibrary.wiley.com/doi/10.1002/2015SW001280/full</p
We present an advance toward accurately predicting the arrivals of coronal mass ejections (CMEs) at...
COR2 coronagraph images are the most commonly used data for coronal mass ejection (CME) analysis amo...
Recent observations with the Heliospheric Imagers (HIs) onboard the twin NASA Solar Terrestrial Rela...
CMEs are often tracked the the Heliospheric Imager (HI) field-of-view by identifying the time-elonga...
The Solar TErrestrial RElations Observatory (STEREO) provides high cadence and high resolution image...
The Solar TErrestrial RElations Observatory (STEREO) provides high cadence and high resolution image...
We report on the development of an Automatic Coronal Mass Ejection (CME) Detection tool (AICMED) for...
<p>An example of the CME time-elongation profiles generated by the Solar Stormwatchers (black dots) ...
Observations from the Heliospheric Imager (HI) instruments aboard the twin STEREO spacecraft have en...
Recent observations with the Heliospheric Imagers (HIs) onboard the twin NASA Solar Terrestrial Rela...
With increasing technological dependence, society is becoming ever more affected by changes in the n...
This animation illustrates the method by which the classifications produced by the Solar Stormwatch ...
Matching the Interplanetary Coronal Mass Ejections (ICME) that are being detected at the near-Earth ...
Forecasting the in situ properties of coronal mass ejections (CMEs) from remote images is expected t...
Recent observations with the Heliospheric Imagers (HIs) onboard the twin NASA Solar Terrestrial Rela...
We present an advance toward accurately predicting the arrivals of coronal mass ejections (CMEs) at...
COR2 coronagraph images are the most commonly used data for coronal mass ejection (CME) analysis amo...
Recent observations with the Heliospheric Imagers (HIs) onboard the twin NASA Solar Terrestrial Rela...
CMEs are often tracked the the Heliospheric Imager (HI) field-of-view by identifying the time-elonga...
The Solar TErrestrial RElations Observatory (STEREO) provides high cadence and high resolution image...
The Solar TErrestrial RElations Observatory (STEREO) provides high cadence and high resolution image...
We report on the development of an Automatic Coronal Mass Ejection (CME) Detection tool (AICMED) for...
<p>An example of the CME time-elongation profiles generated by the Solar Stormwatchers (black dots) ...
Observations from the Heliospheric Imager (HI) instruments aboard the twin STEREO spacecraft have en...
Recent observations with the Heliospheric Imagers (HIs) onboard the twin NASA Solar Terrestrial Rela...
With increasing technological dependence, society is becoming ever more affected by changes in the n...
This animation illustrates the method by which the classifications produced by the Solar Stormwatch ...
Matching the Interplanetary Coronal Mass Ejections (ICME) that are being detected at the near-Earth ...
Forecasting the in situ properties of coronal mass ejections (CMEs) from remote images is expected t...
Recent observations with the Heliospheric Imagers (HIs) onboard the twin NASA Solar Terrestrial Rela...
We present an advance toward accurately predicting the arrivals of coronal mass ejections (CMEs) at...
COR2 coronagraph images are the most commonly used data for coronal mass ejection (CME) analysis amo...
Recent observations with the Heliospheric Imagers (HIs) onboard the twin NASA Solar Terrestrial Rela...