You are here

Home

Space Weather

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.

Measuring the magnetic origins of solar flares, CMEs and Space Weather

A UV spectrum of α Cen A
Wednesday, April 21, 2021

We take a broad look at the problem of identifying the magnetic solar causes of space weather.

Deciphering Deep-Origin of Active Regions From Analysis Of Magnetograms

Graphic image of active-regions' toroid patterns
Tuesday, February 23, 2021

Dikpati, et. al., derive magnetic toroids from surface magnetograms by employing a novel optimization method based on Trust Region Reflective algorithm. Toroids obtained are combinations of Fourier modes (amplitudes and phases) with low longitudinal wavenumbers.

Data-Driven Ensemble Modeling of Equatorial Ionospheric Electrodynamics

Graphic depicting root-mean-square difference of the plasma drift
Thursday, February 4, 2021

A Case Study During a Minor Storm Period Under Solar Minimum Conditions: The dayside equatorial ionospheric electrodynamics exhibits strong variability driven simultaneously by highly changeable external forcings that originate from the Sun, magnetosphere, and lower atmosphere.

NSF APPROVES FUNDING FOR COSMO

The COSMOS observatory

The National Center for Atmospheric Research (NCAR) has received funding approval to survey prospective locations for the Coronal Solar Magnetism Observatory (COSMO).

SPACE STORMS IN THE UPPER ATMOSPHERE AND IONOSPHERE

Photographic image of Stan Solomon

Stan Solomon presented a NCAR Explorer Series lecture about how the aurora is formed and varies with the solar wind driver. In this public outreach lecture Stan delves into the physics and chemistry of the ionosphere.

Responses of the Thermosphere and Ionosphere System to Concurrent Solar Flares and Geomagnetic Storms

Graphic depicting simulated vertical E x B drift velocity
Wednesday, July 1, 2020

We conducted numerical simulations to examine dayside thermosphere and ionosphere responses to concurrent solar flares and a geomagnetic storm during September 6th – September 11th, 2017, as well as the interplay of flare and storm effects.

Partnership Continues with NASA's PSP and MLSO–WHPI

Graphic image of NASA's Parker Solar Probe

Beginning in January 2021, there are new plans underway for continued coordinated efforts between NASA's PSP seventh perihelion and the WHPI campaign.

Living With A Star Focus Team

Role of solar flows and magnetic field dynamics in active regions emergence and impact on heliospheric space weather

Tao Wang

Submitted by whawkins on April 9, 2020 - 12:28pm

Tao Wang is a scientific visitor in the High Altitude Observatory of the National Center for Atmospheric Research hosted by Dr. HanLi Liu. He is a Ph.D. student at Lanzhou University.

Pages

Subscribe to RSS - Space Weather
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.