Geomagnetic storms

geomagnetic storms begin as potent coronal hole becomes geoeffective

Geomagnetic storms begin as potent coronal hole becomes geoeffective

A recurrent, negative-polarity coronal hole is affecting our planet, causing geomagnetic storming. A G2 - Moderate geomagnetic storm watch is in effect for March 28 and 29. A high speed solar wind stream produced by a recurrent, negative-polarity (potent) coronal...

March 27, 2017

sdo aia geoeffective coronal hole

CH HSS sparks geomagnetic storming, G2 warning issued

Earth is under the influence of a positive polarity coronal hole high speed stream (CH HSS) which is causing geomagnetic storming. G1 - Minor geomagnetic storm threshold was first reached at 16:12 UTC on March 21, 2017. A G2 - Moderate geomagnetic storm warning was...

March 21, 2017

Earth under influence polar connected CH HSS

Earth under the influence of polar-connected CH HSS

A negative polarity, polar-connected coronal hole high speed stream (CH HSS) is affecting Earth for the second day in a row, sparking geomagnetic storms reaching G2 Moderate levels. Over the past 24 hours, the solar wind environment was elevated due to the passage...

March 02, 2017

recurrent ch hss sparks g1 geomagnetic storm

Negative polarity CH HSS sparks G1 geomagnetic storm

Earth is under the influence of a recurrent, polar-connected coronal hole which has sparked G1 (Minor) geomagnetic storming today. Unsettled to active conditions, with G1 storming likely, are expected to continue through March 2. Geomagnetic K-index of 5 (G1 - Minor...

March 01, 2017

geomagnetic storm february 24 2017

CH HSS sparks geomagnetic storm reaching G1 levels

Our planet is under the influence of a recurrent, positive polarity coronal hole high speed stream since around 20:48 UTC on February 23. This is causing G1 geomagnetic storming. Geomagnetic K-index of 5 (G1 - Minor geomagnetic storm) threshold was first reached at...

February 24, 2017

geomagnetic storm february 1 2017

G1 geomagnetic storm in progress

A recurrent, negative polarity coronal hole high-speed stream (CH HSS) is affecting our planet causing isolated periods of G1 Minor geomagnetic storming and vivid auroras. High-speed solar wind speed hit Earth late January 31, 2017. Geomagnetic K-index of 5 (G1 -...

February 01, 2017

g2 geomagnetic storm aurora forecast december 21 2016

G2 geomagnetic storm in progress

Earth is under the influence of a positive polarity coronal hole high speed stream today, December 21, 2016, which is causing geomagnetic storms reaching G2 Moderate levels. Shortly after 04:00 UTC on December 21, solar wind speeds increased to just over 500 km/s,...

December 21, 2016

9aurora forecast december 9 2016 21 50 z

G1 geomagnetic storm in progress

A geomagnetic storm is currently in progress due to ongoing negative polarity coronal hole high speed stream (CH HSS) influence. The G1 Watch is in effect for the next three days. Geomagnetic K-index of 5 (G1 - Minor geomagnetic storm) threshold was first reached at...

December 09, 2016

Aurora outburst Mia Stalnacke_ November 24 2016 Kiruna Sweden

Positive polarity CH HSS sparks geomagnetic storms

Earth is under the influence of a positive polarity coronal hole high speed stream (CH HSS). A sudden escalation in overall planetary geomagnetic response from a favorable solar wind environment and elevated solar wind streams triggered periods of G1 and G2...

November 25, 2016

coronal hole october 25 2016 aia 211 193 171 f

Geomagnetic storm in progress, CH HSS influence expected until October 27

​Earth is passing through a stream of high speed solar wind produced by a recurrent, polar connected, positive polarity coronal hole. This is causing isolated periods of G1 class geomagnetic storming. G2 - Moderate geomagnetic storm watch is in effect for October...

October 25, 2016

aurora forecast ovation prime model run at 22 41z october 13 2016 f

G2 geomagnetic storm in progress, G3 - Strong watch in effect for October 14

A filament in Sun's northeast quadrant erupted between 15:00 and 17:00 UTC on Saturday, October 8, 2016, producing an asymmetric, partial-halo CME. The CME, although faint, was first observed in LASCO C2 imagery beginning 00:48 UTC on October 9. It reached ACE...

October 13, 2016

aurora australis by varun dongre at maitri research base antarctica september 29 2016

Prolonged geomagnetic storming, isolated periods of G2 - Moderate levels

Earth is under the influence of a positive polarity coronal hole high speed stream (CH HSS) for several days now. Enhanced solar wind parameters are expected to continue through October 1, with G3 - Strong geomagnetic storm levels possible today. G2 - Moderate...

September 29, 2016

coronal hole 27 september 2016 sdo aia

Recurrent coronal hole sparks another round of geomagnetic storming

High-speed solar wind from a recurrent coronal hole has sparked another round of geomagnetic storming on Earth. The solar wind environment is expected to remain elevated but steady through the rest of the UTC day before becoming further enhanced on September 28 and...

September 27, 2016

geoeffective_ch_17sep2016_f

G1 - Minor geomagnetic storm conditions observed

During the past 24 hours, solar wind parameters transitioned from near background conditions to an enhanced state, causing G1 - Minor geomagnetic storming on Earth. This was most likely caused by the onset of co-rotating interaction region (CIR) ahead of a negative...

September 20, 2016

sdo_aia211_193_171_pfss_31aug2016_f

Positive polarity CH HSS sparks geomagnetic storm

Earth is under continued influence of a positive polarity coronal hole high speed stream (CH HSS), which is now causing geomagnetic storms at high latitudes. K-index of 5 (G1 - Minor geomagnetic storm) threshold was reached at 08:59 UTC on September 1, 2016. ...

September 01, 2016

g1_aurora_fcst_07 35utc_20jul2016_f

Geomagnetic storm in progress

A geomagnetic storm reaching G1 - Minor levels is currently in progress following the early arrival of July 17th Coronal Mass Ejection (CME). The interplanetary shockwave produced by the long duration C1 flare on July 17, initially expected to arrive early on July...

July 20, 2016

sdo_aia_211_193_171_21jun2016_aia_lmsal_f

Negative polarity CH HSS drives isolated periods of geomagnetic storming

Solar wind parameters reflected a brief enhancement associated with the arrival of a co-rotating interaction region (CIR) and subsequent negative polarity coronal hole high speed stream (CH HSS) late June 22, 2016. A gradual increase in solar wind speeds began after...

June 23, 2016