Coronal hole high-speed stream is arriving. If you feel it before the data confirms it — sleep disruption, brain fog, ear ringing, mood shifts — you are not imagining it. Here is what is happening and how to support yourself. reynasynergy.com

Coronal hole high-speed stream is arriving. If you feel it before the data confirms it — sleep disruption, brain fog, ear ringing, mood shifts — you are not imagining it. Here is what is happening and how to support yourself. reynasynergy.com
🔴 Sustained southward Bz detected
Bz has been consistently southward (currently -8.1 nT). Sustained southward fields maximise geomagnetic coupling and support aurora activity.
https://lumina.observer/events
🌍 Weltraumwetter — 13:28 UTC
☀️ Kp: 3.0 🟡 Erhöht
💨 Wind: 287 km/s
🧲 Bz: 2.9 nT · Bt: 5.0 nT
🔥 X-Ray: A4.2
⚛️ Proton: 0.2 pfu
📡 ~7.83 Hz · Solaraktivität beeinflusst den Erde-Ionosphären-Hohlraum.
🟡 Hey Tasmania, aurora odds are looking pretty decent tonight — sitting at 51%. Might be worth a peek!
Check conditions and your local forecast 👉 https://lumina.observer
#Aurora #AuroraNow #AustralianAurora #AuroraAustralis #SpaceWeather
🔴 Sustained southward Bz detected
Bz has been consistently southward (currently -7.9 nT). Sustained southward fields maximise geomagnetic coupling and support aurora activity.
https://lumina.observer/events
🔴 Sustained southward Bz detected
Bz has been consistently southward (currently -6.4 nT). Sustained southward fields maximise geomagnetic coupling and support aurora activity.
https://lumina.observer/events
🌍 Weltraumwetter — 22:41 UTC
☀️ Kp: 2.0 🟢 Ruhig
💨 Wind: 290 km/s
🧲 Bz: -1.4 nT · Bt: 2.8 nT
🔥 X-Ray: A6.7
⚛️ Proton: 0.2 pfu
📡 ~7.83 Hz · Solaraktivität beeinflusst den Erde-Ionosphären-Hohlraum.
🌍 Weltraumwetter — 18:18 UTC
☀️ Kp: 0.0 🟢 Ruhig
💨 Wind: 295 km/s
🧲 Bz: 2.3 nT · Bt: 3.7 nT
🔥 X-Ray: A7.5
⚛️ Proton: 0.3 pfu
📡 ~7.83 Hz · Solaraktivität beeinflusst den Erde-Ionosphären-Hohlraum.
🌍 Weltraumwetter — 13:32 UTC
☀️ Kp: 0.0 🟢 Ruhig
💨 Wind: 326 km/s
🧲 Bz: 2.6 nT · Bt: 3.7 nT
🔥 X-Ray: A5.2
⚛️ Proton: 0.3 pfu
📡 ~7.83 Hz · Solaraktivität beeinflusst den Erde-Ionosphären-Hohlraum.
This coronal hole in the southwestern part of the Sun's visible face will cause propagation disturbances on the shortwave bands from Wednesday into Thursday due to fast solar winds. Credit: NASA/SDO/AIA #spaceweather #hamradio #hamr
Geomagnetic activity will be quiet to unsettled (Kp 0–3) until the expected arrival of the fast winds from a coronal hole. Later, active phases are likely, with the possibility of magnetic storms (Kp 5–6). The risk of solar flares remains low to moderate (M20% X01%). #spaceweather #hamradio #hamr
🌍 Weltraumwetter — 22:44 UTC
☀️ Kp: 0.0 🟢 Ruhig
💨 Wind: 334 km/s
🧲 Bz: -3.9 nT · Bt: 4.1 nT
🔥 X-Ray: A5.5
⚛️ Proton: 0.3 pfu
📡 ~7.83 Hz · Solaraktivität beeinflusst den Erde-Ionosphären-Hohlraum.
🌍 Weltraumwetter — 17:59 UTC
☀️ Kp: 0.0 🟢 Ruhig
💨 Wind: 334 km/s
🧲 Bz: 0.1 nT · Bt: 3.4 nT
🔥 X-Ray: B1.1
⚛️ Proton: 0.2 pfu
📡 ~7.83 Hz · Solaraktivität beeinflusst den Erde-Ionosphären-Hohlraum.
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🌍 Weltraumwetter — 13:18 UTC
☀️ Kp: 0.0 🟢 Ruhig
💨 Wind: 392 km/s
🧲 Bz: 0.7 nT · Bt: 3.4 nT
🔥 X-Ray: —
⚛️ Proton: 0.2 pfu
📡 ~7.83 Hz · Solaraktivität beeinflusst den Erde-Ionosphären-Hohlraum.