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 solar measurements and source signatures; the research ledger separately tracks catalog-supported destinations, and remains operational without another monitor being open.

Measured solar lanes remain separate from authoritative MEFI-derived Earth UFR terms. When Earth UFR is present, its ΔQ, coherence, Π, EUMI, propagation stage, and timing are displayed and recorded without being replaced.

How to use this monitor: the solar panels identify the measured source, particles, wind, and magnetic structure. MEFI then carries those timestamped changes into the shared Earth UFR sequence so later monitors can test for ordered responses. The framework adds a common event record and timing context; it does not alter NOAA data or guarantee an Earth impact.

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GOES X-ray

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Flare class

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Solar-wind speed

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Density

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IMF Bz

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Planetary Kp

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Protons ≥10 MeV

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F10.7 radio flux

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Primary solar view

Sun Activity and Live Solar-State Panel

Waiting for the first measured solar packet.

Solar feeds initializingGOES X-ray, particle, and NOAA SWPC solar-wind measurements are loading.

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 and event imagery motion

SDO / SOHO — 20 Distinct Frames or Selected-Event Sequence

Loading retained imagery…

FrameSpeedOverlay trailTrail opacityBlendEvent span

Latest SDO solar image — SDO AIA 171 Å extreme ultraviolet

Latest SOHO coronagraph image — SOHO LASCO C2 white-light coronagraph

Retained-live mode stores only changed observatory images. Select an active or archived event below, then load its historical Helioviewer sequence to inspect the interval around that event.

Operations

Live Controls

History windowAutomatic refreshImport snapshot

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

0.1–0.8 nmFlare bands A, B, C, M, and X are marked on the chart.

Particle environment

GOES Proton and Electron Flux

Logarithmic native flux

Protons ≥10 MeVElectrons ≥2 MeV

L1 plasma

Solar-Wind Speed, Density, and Temperature

Independent display scales; native values retained

SpeedDensityTemperature

Interplanetary field

IMF Bz and Total Field Bt

Measured nT • zero line included

BzBt

Near-Earth response and downward flow

Dst, Measured Kp, and Prospective Kp

Measured history and explicitly labeled future NOAA/model intervals

DstMeasured KpNOAA forecastGeospace model

MEFI comparison

Solar Measurements and Earth UFR State

Shared Earth UFR values when present

X-ray changeEarth UFR ΔQΠ

Concurrent event recorder

GOES source signatures — arrival not established

Armed and monitoring every event; newest 10 entries open by default.

Inspect tracked or archived event

Newest 10 events shown.

Select any propagation stage for its timestamp, entering factor, response, and recorded effect. Every other event continues tracking while you inspect this path.

Standalone downward-flow forecast and Earth UFR comparison

Prospective Kp and Current MEFI Context

The Kp forecast runs here from direct solar inputs; Earth UFR is optional comparison context.

—Prospective Kp

—Forecast time / lead

—Forecast source

—Downward-flow drivers

—Earth UFR ΔQ

—Coherence

—Π

—EUMI

—Propagation stage

—Magnetic alignment

The Solar Monitor independently ingests NOAA’s current published Kp forecast, then carries the forecast downward in MEFI_SOLAR_STATE. A readings-conditioned L1 estimate remains visible as a diagnostic fallback. Earth UFR values are comparison context only and never gate this forecast. The retired stale Geospace Kp-model route is excluded.

Retained packets

Solar Telemetry Record

Newest 10 packets shown initially • UTC • complete history remains exportable

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.

Newest 10 packets shown.

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.

MEFI Space and Solar Monitor

Live focus on the Sun and its Earthbound effects

Sun Activity and Live Solar-State Panel

SDO / SOHO — 20 Distinct Frames or Selected-Event Sequence

Live Controls

Solar Source Status

Measurements and Event Records

GOES X-Ray Flux and Flare Development

GOES Proton and Electron Flux

Solar-Wind Speed, Density, and Temperature

IMF Bz and Total Field Bt

Dst, Measured Kp, and Prospective Kp

Solar Measurements and Earth UFR State

GOES source signatures — arrival not established

Prospective Kp and Current MEFI Context

Solar Telemetry Record

Measurement and Recording Disclosure

Earth-interacting solar events · strength and saved results