Live observations

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Collection status · JSON

At a glance

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Solar wind measured at L1, before it reaches Earth. One-minute source samples; checks for updates every minute. All times are UTC.

NOAA selects the active spacecraft separately for plasma and magnetic field. Measurements are not shifted to Earth arrival time. Gaps and flagged samples are not connected on charts.

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Solar wind measurement details

Solar wind speed

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Measurement unavailable

Proton density

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Measurement unavailable

Bz

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Measurement unavailable

Total field Bt

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Measurement unavailable

Bx

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Measurement unavailable

By

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Measurement unavailable

Proton temperature

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Measurement unavailable

Solar wind history

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Values are operational observations, not independently validated by Argus. A delay above 10 minutes is marked “Delayed”. History resolution depends on the selected period; values are never interpolated.

Geomagnetic activity

Kp retains its three-hour intervals. Kyoto Dst is shown hourly. Both are preliminary operational data and may be revised.

Geomagnetic measurement details

Kp

NOAA SWPC · Preliminary estimate

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Real-time Dst

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Index history

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Blank intervals indicate missing or flagged data. Freshness allows for publication delay after an interval ends: four hours for Kp, two hours for Dst (the next native interval plus one hour).

Additional hourly indices

Hourly indices

Latest available hourly observations. Checks for updates every minute. All times are UTC.

These are normalized data; missing measurements may be interpolated or filled during processing.

S10, M10 and Y10 are calibrated GOES estimates of daily solar indices, updated from the UTC day’s available observations at each hour boundary. Midnight closes the previous day. These estimates are provisional; no forecasts are shown. A dash means no calibrated estimate is available for that hour; these indices are not gap-filled.

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