Solar cycle 24

"[8] Another group of researchers, including one at NASA, predicted that it "looks like its going to be one of the most intense cycles since record-keeping began almost 400 years ago.

[14] According to NASA, the intensity of geomagnetic storms during Solar Cycle 24 may be elevated in some areas where the Earth's magnetic field is weaker than expected.

While acknowledging that the next solar maximum will not necessarily produce unusual geomagnetic activity, astrophysicist Michio Kaku took advantage of the media focus on the 2012 phenomenon to draw attention to the need to develop strategies for coping with the terrestrial damage that such an event could inflict.

He asserted that governments should ensure the integrity of electrical infrastructure, so as to prevent a recurrence of disruption akin to that caused by the solar storm of 1859.

Sunspots did not begin to appear immediately after the last minimum (in 2008) and although they started to reappear in late 2009, they were at significantly lower rates than anticipated.

[19] On April 19, 2012, the National Astronomical Observatory of Japan predicted that the Sun's magnetic field would assume a quadrupole configuration.

[20] Throughout 2012, NASA posted news releases discrediting the 2012 phenomenon and the so-called Mayan prophecy, delinking them from solar activity and space weather.

[21][22] On 4 January 2008, an active region appeared with magnetic polarity reversed compared to that expected by Hale's law for solar cycle 23.

The region was located at the relatively high latitude 30° N which, according to Spörer's law, provided further evidence for the arrival of cycle 24.

On 5 April 2010, the first coronal mass ejection (CME) of cycle 24 erupted at an active region causing a G3 (strong) geomagnetic storm on Earth.

[30] On 4 August 2010, a G2 (moderate) geomagnetic storm caused aurorae to be visible in the northern hemisphere at latitudes as far south as 45° N near Michigan and Wisconsin in the United States, and Ontario, Canada.

NOAA issued an R3 (strong) radio blackout alert pertaining this prominent x-ray flux event.

[39] On August 5, 2011, the combined cloud of three consecutive CMEs produced brilliant aurorae, reported as far south as Oklahoma and Alabama.

Although the flare was not Earth-directed, radiation created waves of ionization in Earth's upper atmosphere, briefly disrupting communications at some VLF and HF radio frequencies.

The Sun unleashed eight M-class flares this month, being the strongest the M3.9 event, followed by an Earth-directed CME, produced by sunspot 1305 on October 2.

[49] On November 3, 2011, active region 1339, one of the largest sunspots in years - 40,000 km wide and at least twice that in length - unleashed an X1.9-class solar flare.

The CME hit the Earth's magnetic field in the early hours of January 22, with minor geomagnetic disturbances reported.

The wave of high energy electromagnetic rays, reaching Earth in minutes, caused an R3 (strong) radio blackout over China, India and Australia, according to NOAA.

[63] Months later, in June, NASA reported that its Fermi Gamma-ray Space Telescope detected in this powerful flare the highest flux of gamma rays — greater than 100 MeV — ever associated with an eruption on the Sun.

[65] NASA also reported that these powerful flares heated the Earth's upper atmosphere with the biggest dose of infrared radiation since 2005.

Infrared radiation from carbon dioxide and nitric oxide, the two most efficient coolants in the thermosphere, re-radiated 95% of that total back into space.

This so-called "monster" sunspot complex, the largest active region of the cycle to date, was about the size of Jupiter, or eleven times the diameter of Earth.

Six days after, sunspot 1520, the largest active region of Solar Cycle 24 to date, unleashed an X1.4-class flare, peaking at 12:52 PM EDT.

This huge group of sunspots, which rotated into view on July 6, was located in the center of the Sun at the time of this event.

On August 31, 2012, a long filament of solar material that had been hovering in the Sun's atmosphere (the corona) erupted out into space at 4:36 p.m.

These powerful bursts all surged from the just-numbered sunspot AR1748, located on the eastern limb of the Sun and barely rotating around the front of the solar disk.

Larger than the planet Jupiter, the AR 12192 sunspot was visible during a partial solar eclipse seen in North America.

[85] In early November 2015, solar flares disrupted the air traffic control system in central and southern Sweden, causing heavy delays for passengers.

[91][92] Then, when this region was just crossing the west limb, another X-class flare (SOL2017-09-10, X8.2) produced only the second ground-level particle event of the cycle.

A small active region, NOAA 12694, appeared at the surprisingly high latitude of S32, near the disk center (January 8).

NASA Solar Cycle 24 Sunspot Number Prediction
The 2008 breach of Earth's magnetic shield
Magnetogram showing the magnetic polarity of AR10981 (labeled as sunspot region 10981) compared to an active region from solar cycle 23.
Video captured by NASA'sof the initial ejection taken August 1, 2010.
The coronal mass ejection starts at 2:36 UTC and ends at 3:56 UTC on August 1, 2010 in this animation on STEREO Ahead images.
The Aug 9, 2011 X6.9-class flare, taken by NASA's Solar Dynamics Observatory (SDO) in extreme UV light at 131 Angstroms.
The active region 1302, responsible for two X-class flares in Sep 22 and 24, 2011. Image taken that month by NASA's SDO.
Enlil model for the March 2012 coronal mass ejection, plotted out to ten astronomical units (beyond the orbit of Saturn ). The top view slices the data in the plane of the Earth's orbit and projects the planetary orbits onto that. The side view is a cross-section through the Sun-Earth line. The wedge-shape of the side view is because the ENLIL model only extends above and below the solar equator by 60 degrees.
Short video of the eruption beginning on April 16th 2012. The video begins in 304 Angstrom extreme ultraviolet and ends with 171 Angstrom.
August 31, 2012 CME: pictured here is a lighten blended version of the 304 and 171 angstrom wavelengths.
Video of the X1.8 class solar flare on Oct. 23, 2012,kel as captured by NASA's Solar Dynamics Observatory (SDO) in the 131 and 304 Angstrom wavelengths. The 131 wavelength of light is used for observing solar material heated to 10 million kelvin , as in a solar flare. The wavelength is typically colorized in teal, as it is here.
The 13–15 May 2013 series of four X-class flares erupted by AR1748: X1.7, X2.8, X3.2 and X1.2. Shots taken by NASA's Solar Dynamics Observatory (SDO) in the 131 Angstrom wavelength of extreme UV light.
The 13–15 May 2013 series of four X-class flares as they were registered by the real-time monitor of GOES satellites X-ray Flux (NOAA/SWPC).
The SDO captured an image of the June 25, 2015 event.