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Solar Wind & Bz Right Now

Aurora signal Watch

Bz has been southward for the last 15 minutes. This early sign is our own rule, not a published criterion: a storm needs southward Bz held for hours.

Measured at L1 by SOLAR-1. At 341 km/s the solar wind reaches Earth in about 75 minutes.

Range

Bz

−6.5 nT

south

Southward (below 0) lets solar-wind energy in; northward largely shuts it out.

Speed

341 km/s

slow

Slow wind: 300–500 km/s. Above 500 km/s is fast and favourable.

Density

4.0 p/cm³

typical

Typical: 3–10 particles per cm³.

Bt

7.8 nT

Strength of the whole field; Bz is its north–south part.

Hemispheric power

25 GW

above 20 GW

Northern hemisphere. Below about 20 GW there may be little or no visible aurora.

Source: NOAA SWPC — Real Time Solar Wind · SOLAR-1

How to read solar wind data

These numbers are measured upstream, at L1 between the Sun and Earth, and describe wind that has not reached us yet: the travel time above is how long it still has to go.

Bz

Bz is the north–south part of the interplanetary magnetic field (IMF) the wind carries, and the number that decides most. Read it by direction and by duration. Published storm criteria all ask for southward Bz held for hours — two hours at −5 nT or below for a moderate storm, more than three at below −10 nT for an intense one. That is why the signal above waits before it changes, and why a short swing to the south in the sparkline is not yet news.

Speed

Faster wind carries far more energy: it grows with the square of the speed. Slow wind runs at 300–500 km/s, wind from coronal holes at 500–800, and wind behind a coronal mass ejection (CME) can reach about 2,000 km/s. Speed and Bz work together as one number, the electric field Ey: 600 km/s with Bz at −5 nT gives 3 mV/m, the level of the moderate-storm criterion.

Density

Density adds pressure to the wind that hits Earth's magnetic field. It is not what opens the way in: that is southward Bz, and a northward Bz largely seals the field whatever the density.

Bt

Bt is the total strength of the magnetic field, all three directions together; Bz is its north–south part. A strong Bt matters for aurora when much of it points south — read it next to the Bz row, not on its own.

Hemispheric power

This one is not measured: it is the OVATION model's estimate of the aurora's energy, computed from the wind above. It is the quickest summary of how bright and wide the auroral oval is right now; the aurora map shows where it lies.

How far ahead this tells you

There is no Bz forecast: Bz is measured at L1, not predicted. The signal describes the next few hours, because Earth's magnetic field responds one to four hours after southward Bz. For tonight, see where the aurora is likely tonight and Kp now and the 3-day forecast; for the weeks ahead, the 27-day outlook. What any Kp means where you are is in the Kp index guide.

Frequently asked questions

What Bz is good for aurora?

Negative — pointing south — and staying there. Southward Bz is what couples the solar wind to Earth's magnetic field and drives aurora. What matters is how long it lasts: Bz at −5 nT or below for two hours is the published criterion for a moderate storm, below −10 nT for more than three hours for an intense one. A dip of a few minutes is not a signal. Whether you then see aurora depends on your latitude, clouds and darkness.

How much warning does the solar wind data give?

As much time as the wind needs to travel from the spacecraft to Earth. They sit at L1, about 1.5 million km towards the Sun, so the warning is about an hour at 400 km/s and about half an hour at 800 km/s; the page prints the current figure. Bz cannot be forecast further ahead than that. For tonight and the next nights, use the 3-day Kp forecast instead.

What do calm, watch, active and storm mean?

They are the aurora signal above, read from the last hours of Bz and speed. Active and storm are published criteria for a moderate and an intense geomagnetic storm: southward Bz held for two and for more than three hours. Watch is our own early sign — Bz south for the last 15 minutes — not a published criterion. Calm means Bz is north or near zero. Earth's response peaks one to four hours after the Bz that drives it.

What is hemispheric power?

NOAA's OVATION model estimates how much energy the aurora puts into one hemisphere, in gigawatts, from the solar wind measured at L1. A value under roughly 20 GW means the aurora may be faint or missing altogether; higher values go with a brighter, wider auroral oval. The page shows the northern hemisphere. The same model draws the aurora map, where you can see how far the oval reaches.

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