April 29, 2022: Planets aren’t supposed to have tails, but Mercury does. Dr. Sebastian Voltmer just photographed it from La Palma in the Canary Islands:
“This is NOT a comet, not even a meteor, but the planet Mercury, which is currently very close to the Pleiades,” says Voltmer. “How is the tail formed? The solar wind and micro-meteorites eject sodium atoms from Mercury’s surface. This creates a yellow-orange tail of sodium gas that is around 24 million kilometers long.”
People around the world have been watching Mercury climb up the evening sky this month. Some of them are probably wondering “why didn’t I see the tail?”
Answer: A special filter is required. “I used a 589 nanometer filter tuned to the yellow glow of sodium,” says Voltmer. Without this kind of sodium filter, Mercury’s tail would be invisible.
Voltmer says the tail is so bright, he could see it in individual 30 second exposures. “I can see some very small changes in shape of the tail,” he says, “and the brightness is slightly increasing.”
The nights ahead are excellent times to catch this phenomenon. On April 29th and 30th, Mercury will glide past the Pleiades star cluster for a fantastic photo-op. Then, on May 1st and 2nd, the crescent Moon joins the show.
“Currently I’m imaging Mercury day by day just after sunset from the Canary Islands,” says Voltmer. Stay tuned for more sodium.
April 11, 2022: The corpse of old sunspot AR2987 exploded today, April 11, 2022, hurling debris directly toward Earth. NASA’s Solar Dynamics Observatory recorded the eruption:
The S-shaped magnetic filament at the base of the explosion is a classic “sigmoid structure.” Solar magnetic fields often assume this shape just before they explode. One study shows that sigmoid precursors are present in over 50% of CMEs.
Indeed, shortly after the explosion, a full-halo CME emerged from the blast site. Here it is. The CME is expected to reach Earth on April 14th; a new NOAA model pinpoints its arrival time at 1100 UTC. The impact could spark a G2-class geomagnetic storm. Aurora alerts:SMS Text
April 10, 2022: Earth’s magnetic field was supposed to be quiet on April 10th. Instead a strong (G3-class) geomagnetic storm broke out. At the apex of the disturbance, auroras crossed the Canadian border into multiple northern-tier US states. Ron Risman sends this time-lapse movie from Milton, New Hampshire:
“We don’t get to see the aurora all that often in New Hampshire, but this solar cycle so far has been fantastic,” says Risman. Before the show was over, the lights spread west all the way to Washington state.
What caused the storm? The prime suspect is a “canyon of fire” CME, which hit Earth’s magnetic field on April 8th. The impact was weak and, at first, it seemed to have little effect. Geomagnetic unrest increased on April 9th as Earth passed into the CME’s strongly magnetized wake. The arrival of an unrelated solar wind stream on April 10th tipped conditions into G3-category storming.
April 3, 2022: A filament of magnetism whipsawed out of the sun’s atmosphere today. On the way out it carved a gigantic canyon of fire. NASA’s Solar Dynamics Observatory recorded the eruption:
The glowing walls of the canyon are at least 20,000 km high and 10 times as long. They trace the channel where the filament (R.I.P.) was previously suspended by magnetic forces inside the sun’s atmosphere.
Debris from the explosion formed a slow-moving coronal mass ejection (CME), shown here in a movie from the Solar and Heliospheric Observatory (SOHO):
The CME is not squarely Earth-directed. The bulk of the cloud is expected to miss. However, there is clearly a small Earth-directed component, which could sideswipe our planet’s magnetic field on April 7th. (Update: It arrived on April 8th instead.)
April 5, 2022: New sunspot counts from NOAA confirm that Solar Cycle 25 is racing ahead of the official forecast–and the gap is growing:
Sunspot counts have now exceeded predictions for 18 straight months. The monthly value at the end of March was more than twice the forecast, and the highest in nearly 7 years.
The “official forecast” comes from the Solar Cycle Prediction Panel, a group of scientists representing NOAA, NASA and International Space Environmental Services (ISES). The Panel predicted that Solar Cycle 25 would peak in July 2025 as a relatively weak cycle, similar in magnitude to its predecessor Solar Cycle 24. Instead, Solar Cycle 25 is shaping up to be stronger.
In March 2022, the sun produced 146 solar flares, including one X-flare and 13 M-flares. Auroras were sighted as far south as Colorado (+38N) and Nebraska (+42N). Multiple shortwave radio blackouts disrupted communications on ships at sea and airplanes flying over the poles. If current trends continue, April will be even busier. Stay tuned. Solar flare alerts:SMS Text
April 2, 2022: On March 30th, the sun did two seemingly contradictory things at once. It produced a loud radio burst and, at the same time, caused a deep radio blackout. Both were side-effects of an X1.3-class solar flare. First, let’s listen to the radio burst:
The gentle roar of static you just heard emerged from the loudspeaker of a shortwave radio receiver in New Mexico. Amateur astronomer Thomas Ashcraft recorded it. “The sun was well positioned in my radio antennas for the X1.3 solar flare,” says Ashcraft. “The left channel of the audio file is 22.2 MHz, the right channel is 21.1 MHz.”
This is a Type II solar radio burst. Shock waves from the flare rippled through the sun’s atmosphere, creating plasma oscillations that emit shortwave static. Briefly, the sun turned itself into a natural radio transmitter.
While the sun was busy creating radio waves, it was equally busy wiping them out. Radiation from the flare ionized the top of Earth’s atmosphere, preventing terrestrial radio stations from bouncing their signals over the horizon as usual. This map shows where manmade signals suddenly faded:
Ashcraft’s observatory in New Mexico is located near the middle of the blackout zone. Take another look at his dynamic spectrum. Horizontal lines are terrestrial radio stations. They vanished for about 10 minutes around the time of the flare. The effect is strongest at frequencies below ~20 MHz.
In Gainesville, Florida, radio astronomer Francisco Reyes recorded the blackout as well. “I used an array of 4 dipoles with an FSX-7 radio spectrograph (Radio JOVE),” he says.
Would you like to record an event like this? NASA’s Radio JOVE program makes it easy. Off-the-shelf radio telescope kits allow even novices to monitor radio outbursts from the sun, which are becoming more frequent as Solar Cycle 25 intensifies. Solar flare alerts:SMS Text