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ICON Press Release: El Nino Affects Conditions in Space

El Nino affects

The warm El Niño conditions affecting weather around the Pacific Ocean are also affecting conditions in space, according to University of California, Berkeley scientists. See ICON Press-release.

HAO Colloquium Series Presents Rachel Osten, STSI

Stellar Flares: from Plasma Physics on Stars to Space Weather on Other Worlds

Roble Honored with Bowie Medal

Roble with peers

HAO is privileged to announce that Dr. Ray Roble was awarded the William Bowie Medal. He received AGU’s highest honor for his pioneering research into Earth’s upper atmosphere at this year’s AGU meeting in San Francisco.

Mk4 Composites

Solar Maximum Mission Coronagraph

This will be the SMM instrument page.

COMING SOON!

MLSO Users' Committee

The Mauna Loa Solar Observatory (MLSO) is a facility of the National Center for Atmospheric Research (NCAR) and is operated by the High Altitude Observatory (HAO). It provides observations of the solar photosphere, chromosphere and corona in order to understand the Sun’s continuous release of plasma and energy into interplanetary space and the impacts at Earth. HAO is committed to providing the community with critically important, high-quality solar observations.

Welcome to Boulder Solar Alliance (BSA)

Boulder is fortunate to have one of the greatest concentrations of solar physics institutes in the world. To encourage communication among researchers from these institutes, we have formed the BSA with representation from:

HAO Colloquium Series presents Joseph Huba, NRL

Joseph Huba

Modeling the Plasmasphere with SAMI3: The study of the plasmasphere is extremely important to understanding space weather phenomena; for example, it plays a critical role in the regulation of radiation belt dynamics.

Synoptic Network Workshop Overview

Synoptic Workshop

The High Altitude Observatory recently partnered with the National Solar Observatory to hold a 3-day workshop to discuss and gather community input on science requirements, capabilities and instrumentation for a next-generation synoptic network of solar observing instruments.

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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.