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Coronal mass ejection

About the Mauna Loa Solar Observatory

The Mauna Loa Solar Observatory (MLSO) occupies part of the NOAA Mauna Loa research site located on the flank of Mauna Loa at an elevation of 3440 meters on the island of Hawaii. It is operated by the High Altitude Observatory, a division of the National Center for Atmospheric Research, which is located in Boulder, Colorado.

Convolutional Neural Networks for Predicting the strength of the Near-Earth Magnetic Field Caused by Interplanetary Coronal Mass Ejections

Image depicting examples of various initial GLOW configurations
Thursday, July 9, 2020

In this paper, regression-based deep convolutional neural networks (CNN), with 12 layers, are developed for predicting the maximal amplitude of the southward component of the near-Earth magnetic field from a passing interplanetary coronal mass ejection (ICME).

Yeimy Rivera

Submitted by whawkins on April 15, 2020 - 8:34am

Yeimy Rivera is a visiting scientist in the High Altitude Observatory (HAO) at the National Center for Atmospheric Research (NCAR). She is completing her PhD program at the University of Michigan under the advisement of Dr. Enrico Landi and Dr. Susan Lepri.

Seeker Science Video Features HAO's Delores Knipp

Photograph of Coronal Mass Ejections

Seeker, an American digital media network and content publisher, interviewed HAO's space scientist, Delores Knipp, in July 2019. The presentation is titled "How Earth's Magnetic Field Twists and Buckles During Solar Storms." Dr.

CME Initiation, Evolution, and Interplanetary Consequences

Submitted by whawkins on September 1, 2016 - 11:56am

HAO scientists have carried out 3D isothermal MHD simulations of the evolution of the large scale coronal magnetic field as a twisted magnetic flux tube is driven (slowly) through the lower boundary into a pre-existing coronal arcade field.

Joan Burkepile

Submitted by whawkins on July 25, 2016 - 3:02pm

Joan Burkepile is a Project Scientist at the High Altitude Observatory of the National Center for Atmospheric Research.

Steve Tomczyk

Submitted by whawkins on April 14, 2016 - 10:54am

Dr. Steven Tomczyk is a Senior Scientist in the High Altitude Observatory at the National Center for Atmospheric Research. He has spent his career developing instrumentation for the remote sensing of magnetic and velocity fields on the Sun. 

Sarah Gibson

Submitted by whawkins on April 13, 2016 - 11:35am

Dr. Sarah Gibson is an Interim Director in the High Altitude Observatory (HAO) at NCAR .

Solar Transients and Space Weather

Overview and Research Goal

On the watch for solar superstorms

Image of coronal mass ejection

NCAR solar physicist Scott McIntosh is raising awareness. While the current peak in the 11-year cycle of sunspot activity is on the weak side, the Sun might still produce a major storm at any point.

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The National Center for Atmospheric Research is sponsored by the National Science Foundation. Any opinions, findings and conclusions or recommendations expressed in this publication are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.