Release notes for the publication number can go here
Readout Times
Readout Times
Camera Readout Times
| Image Size | Actual time (usec) | Est Readout time |
| 2176x2048 | 4851979 | 5.0 |
| 2176x2048 bin | 2561514 | 2.7 |
| 2048x2048 | 4691743 | 4.8 |
| 2176x2112 | 5002963 | 5.1 |
Boot Times
Here are reboot times from execution of SFMODE proc on the EDM for your reference..
/SWMAINTMODE -> TM#0112 Xition to Maint Mode 1:03
/SWOPSMODE -> TM#0113 Xition to Ops Mode 1:19
/SWRESETCOLD -> TM#0111 Board Level Reset 2:03
/RECOVERREBOOT COLD -> TM#0105 Spurious Processor Reset 2:04
/SHSLOTDIS -> TM#0101 Reset Due to Watchdog 2:01 (includes 10-second timer count-down)
Synoptic Program Plans
SECCHI schedules, Dec 2021
SECCHI 2 hour block schedules beginning on 02/19/2021
210214_0.bsf 47kbps
| SSR1 Images | SSR1 MB | SSR2 images | SSR2 MB | 00 block images |
|---|
SECCHI Data Overview
SECCHI is a suite of five telescopes, with two identical SECCHI suites operating on both NASA STEREO satellites (and only operational on STEREO-A since 2014). The five telescopes are as follows:
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 Consortium Meeting, Stanford
Tasks or Action Items for Session on Space Weather SECCHI Consortium meeting, Stanford
On the structure of the SW Group, the consensus was that our group should be open to all the STEREO instrument teams as well as outside scientists interested in space weather. It is OK to keep the present NRL SECCHI internet site, but to link it as needed elsewhere such as the GSFC STEREO Science Center. We should use the website interactively, especially for sending email to the entire group. Comments, ideas, changes to the site are solicited.
Space Weather
THE STEREO SPACE WEATHER GROUP
CME Queries
The CME query database is currently down for maintenance and will be available as soon as possible.
EA Mode Test On 12 May 09
Plots for STEREO-Behind
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]