MEFI Space and Solar Monitor
The Sun, solar particles, solar wind, magnetic structure, and the complete Sun-to-Earth event path
Starting solar feedsUpdated —Recorder armed
Live focus on the Sun and its Earthbound effects
This dedicated monitor directly ingests measured NOAA SWPC solar, particle, solar-wind, interplanetary magnetic-field, and near-Earth response lanes. It continuously publishes MEFI_SOLAR_STATE, records each solar event from source through surface response, and remains operational without another monitor being open.
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GOES X-ray
waiting
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Flare class
waiting
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Solar-wind speed
waiting
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Density
waiting
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IMF Bz
waiting
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Planetary Kp
waiting
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Protons ≥10 MeV
waiting
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F10.7 radio flux
waiting
Primary solar view
Sun Activity and Live Solar-State Panel
Waiting for the first measured solar packet.
ARMED — awaiting next solar eventBaseline measurements continue continuously.
GOES long-channel X-ray flux—
Most recent GOES flare—
Proton flux ≥10 MeV—
Electron flux ≥2 MeV—
Solar wind / density / temperature—
IMF Bx / By / Bz / Bt—
Kp / Dst / auroral probability—
F10.7 radio flux—
The interpretation panel will describe the current measured solar state after the first complete packet.
Live imagery motion
SDO / SOHO — Last 20 Snapshot Overlay
Loading retained imagery…
Waiting for retained frames. The newest snapshot opens by default; playback advances chronologically while prior frames remain blended underneath.
Operations
Live Controls
Changing the visible history window changes only chart resolution. Native measurements and timestamps remain unchanged in exports and shared state.
Feed health
Solar Source Status
Export
Measurements and Event Records
No locally retained packets yet.
Solar source
GOES X-Ray Flux and Flare Development
Logarithmic measured W/m²
Particle environment
GOES Proton and Electron Flux
Logarithmic native flux
L1 plasma
Solar-Wind Speed, Density, and Temperature
Independent display scales; native values retained
Interplanetary field
IMF Bz and Total Field Bt
Measured nT • zero line included
Near-Earth response
Dst and Planetary Kp
Independent display scales; measured values shown in readouts
MEFI comparison
Solar Measurements and Earth UFR State
Shared Earth UFR values when present
Concurrent event recorder
Complete Solar Event Propagation Paths
Armed and monitoring every event; latest opens by default.
Select any propagation stage for its timestamp, entering factor, response, and recorded effect. Every other event continues tracking while you inspect this path.
Authoritative Earth UFR bridge
Current MEFI Comparison
Waiting for retained or live Earth UFR state.
—ΔQ
—Coherence
—Π
—EUMI
—Propagation stage
This panel reads Earth UFR shared state when available. The Solar Monitor does not fabricate or independently replace these MEFI terms.
Retained packets
Solar Telemetry Record
Newest 150 packets shown • UTC
| UTC | X-ray | Flare | Protons | Electrons | Speed | Density | Temperature | Bx | By | Bz | Bt | Kp | Dst | F10.7 | Event / stage | Earth UFR ΔQ | Π |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Waiting for the first measured packet. | |||||||||||||||||
Methodology
Measurement and Recording Disclosure
GOES X-ray, proton, and electron measurements describe the solar and particle source lanes. NOAA SWPC real-time solar wind and IMF measurements describe the L1 plasma and magnetic lanes. Kp, Dst, F10.7, and OVATION are displayed as measured or published context/response products. Sun-to-Earth stage timing is recorded from incoming timestamps and the live propagation state; any transit estimate is labeled in the stage details and never substitutes for a measured arrival packet.