SECCHI Consortium Meeting, Stanford (Agenda)

Agenda for Session on Space Weather SECCHI Consortium meeting, Stanford

Introduction to the STEREO Space Weather Group

Use and Structure of the Website
How should the Group be structured?
Specific Group tasks and timelines
Make poster(s) or general drawings/images for STEREO Space Weather

SECCHI images for the Beacon mode [PDF]

Heliospheric Imagers and Space Weather [PPT]

Use of the SECCHI coronal instruments for SW

Uses of the PLASTIC, IMPACT, and SWAVES instruments for SW

IMPACT - Tool set-up using magnetogram-based potential field model

Real-time forecasting using solar observations with shock modeling

HAF: An Operational, Event-driven Solar Wind Forecast Model [PPT]

Summary and Future Plans (not done!)

SECCHI-publication-number-goes-here

2024 Geomagnetic Storms

In May 2024, Earth experienced some of the most intense geomagnetic storms seen in recent years. Solar eruptions that led to these storms were imaged by the SECCHI HI-2 camera on NASA STEREO-A. This image sequence shows the large CME front passing over Earth (far left, not to scale) along with concurrent Kp observations, which shows the Earth's geomagnetic response to the event.

Observations from the SECCHI HI-2 camera on May 12, 2024 (top), along with the concurrent "kp" geomagnetic activity index (lower). The location of Earth is as indicated on the left of the animation. [Credits: NASA/NRL/STEREO]

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Agenda for Session on Space Weather SECCHI Consortium meeting, Stanford

2024 Geomagnetic Storms

SECCHI is a suite of 5 scientific telescopes that observe the solar corona and inner heliosphere from the surface of the Sun to the orbit of Earth.