Solar cycle 25

Solar cycle 25 is the current solar cycle, the 25th since 1755, when extensive recording of solar sunspot activity began. It began in December 2019 with a minimum smoothed sunspot number of 1.8.[2] It is expected to continue until about 2030.[3][4]

Solar cycle 25
ISES Solar Cycle 25 Sunspot Number Progression and Predictions as of September 2023
Sunspot data
Start dateDecember 2019
Max count121 (smoothed)
Max count monthMarch 2023 (progressive)[1]
Min count1.8
Cycle chronology
Previous cycleSolar cycle 24 (12/2008-12/2019)

Predictions

Widely varying predictions regarding the strength of cycle 25 ranged from very weak with suggestions of slow slide in to a Maunder minimum like state[5][6] to a weak cycle similar to previous cycle 24[7] and even a strong cycle.[8][9][10] Upton and Hathaway predicted that the weakness of cycle 25 would make it part of the Modern Gleissberg Minimum.[5]

The Solar Cycle 25 Prediction Panel predicted in December 2019[11] that solar cycle 25 will be similar to solar cycle 24, with the preceding solar cycle minimum in April 2020 (± 6 months), and the number of sunspots reaching a (smoothed) maximum of 115 in July 2025 (± 8 months). This prediction is in line with the current general agreement in the scientific literature, which holds that solar cycle 25 will be weaker than average (i.e. weaker than during the exceptionally strong Modern Maximum).[7] However, observations from 2020 to 2022, the first three years of the cycle, significantly exceed predicted values.[12]

Cycle 25 predictions
Source Date Cycle max Cycle start Cycle end
Thompson, M.J. et al.[4] August 2014 Q4 2019
Zharkova, V. et al 2014, 2015.[13] (Northumbria U.) October 2014 65 (80% of cycle 24)
Upton, L.A. and Hathaway, D.H.[5] (Solar Observatories Group, Stanford University) December 2018 78 (95% of cycle 24) Late 2020 – Early 2021
Xu, J.C. et al.[8] (Chinese Academy of Sciences) August 2018 168.5 ± 16.3 (2024) October 2020
Bhowmik, P. and Nandy, D.[7] (IISER Kolkata) December 2018 124 ± 15 (2023–2025) 2020 after 2031
Ozguc, A. et al.[9] (Harvard U-ty) December 2018 154 ± 12 (2023.2±1.1)
NOAA / SSRC[14] April 2019 117 ± 23 (2023–2026) mid-2019 – late 2020
NASA[15] June 2019 70 ± 29 (30–50% lower than Cycle 24 (2025)) 2020
NOAA / SSRC (update)[16] December 2019 115 ± 10 (July 2025) April 2020 (± 6 months)
Mcintosh et al..[17][18] June 2020 229 ± 25
Mcintosh et al.[17][18] December 2020 190 ± 20
National Center for Atmospheric Research[19] December 2020 233
(Actual) present >121 December 2019 -

Early signs

Time vs. solar latitude diagram of the radial component of the solar magnetic field (supersynoptic map or “butterfly” diagram) for cycle 24 based on the (zero-point corrected) integer rotation synoptic maps from GONG. Blue/red show negative/positive polarity fields scaled between ±5 Gauss. Two black arrows mark approximate location of two latitudinal bands of cycle 25. Data are acquired by GONG instruments operated by NISP/NSO/AURA/NSF.

As of April 2018, the Sun showed signs of a reverse magnetic polarity sunspot appearing and beginning this solar cycle.[20] It is typical during the transition from one cycle to the next to experience a period where sunspots of both polarities exist (during the solar minimum). The polarward reversed polarity sunspots suggested that a transition to cycle 25 was in process.[21] The first cycle 25 sunspot may have appeared in early April 2018[22][23] or even December 2016.[21]

In November 2019, two reversed polarity sunspots appeared, possibly signaling the onset of cycle 25.[24][25]

Nandy et al., analyzed the polarity orientation of bipolar magnetic regions observed in December 2019 and concluded that magnetic regions with the underlying orientation of solar cycle 25 toroidal field component were brewing in the solar convection zone, representing early signs of the new cycle.[26]

Supersynoptic (time vs. solar latitude) map of the radial component of the solar magnetic field for cycles 24-25 based on observations from the Global Oscillations Network Group (GONG) shows magnetic activity of cycle 25 beginning November 2019 at about 30 degree latitudes in both solar hemispheres.[27] A more recent supersynoptic map is available.[28]

The following table gives the number of days so far in cycle 25 against the number up to the same point in cycle 24, and also up to the end of 2012 in cycle 24, which have passed various thresholds for the numbers of sunspots.

Counts SC 24
to Dec 31 2012
SC 24
to Sep 22 2012
SC 25
to Sep 22 2023
≥75 sunspots 399 353 494
≥100 241 223 334
≥125 116 109 207
≥150 39 39 99
≥175 6 6 41
≥200 0 0 13
≥225 0 0 2


As at Sep 22 2023, solar cycle 25 is averaging 25% more spots per day than solar cycle 24 at the same point in the cycle (Sep 22 2012).
Year 4 of solar cycle 25 (Dec 1 2022 to Sep 22 2023) is averaging 45% more spots per day than the corresponding period in solar cycle 24.

Events

Solar flares by year
10
20
30
40
2019
2020
2021
2022
2023
2024
2025
2026
2027
2028
2029
2030
  •   M5-M9
  •   X1-X5
  •   X5-X9
The strongest flares of Solar Cycle 25 (above M5.0 class) and related events
ClassYearDateSunspot regionRadio B.SR StormCMEGM Storm
X2.282023Feb 173229R3-Yes-
X2.252022Apr 202992R3-Yes-
X2.072023Mar 33234R3-Yes-
X1.982023Jan 93184R3-No-
X1.632023Aug 53386R3S1Yes-
X1.592021Jul 32838R3-Yes-
X1.512022May 103006R3-No-
X1.512023Aug 73386R3S1Yes-
X1.382022Mar 302975R3S1YesG1
X1.272023Mar 293256R3-Yes-
X1.222023Jan 63182R3-No-
X1.172022Apr 172994R3-Yes-
X1.162023Feb 113217R3-No-
X1.132022Apr 302994R3-Yes-
X1.132022May 33006R3-No-
X1.112023Jun 203341R3-Yes-
X1.082023Jul 23354R3-No-
X1.062022Oct 23110R3-Yes-
X1.062023Jan 103186R3-Yes-
X1.02021Oct 282887R3S1Yes-
M9.672022Mar 312975R2-Yes-
M9.662022Apr 212993R2-Yes-
M9.622023May 163310R2-No-
M8.962023May 203311R2-No-
M8.772022Oct 23110R2-YesG1
M8.722023Sep 213435R2-Yes ?
M8.672022Aug 293088R2-No-
M8.622023Feb 283234R2-Yes-
M8.232023Sep 203435R2-No-
M7.922022Sep 163098R2-No-
M7.292022Apr 202992R2-Yes-
M7.272023May 33293R2-No-
M7.242022Aug 263089R2-Yes-
M7.122023May 13288R2-No-
M6.972023Jul 123372R2-No-
M6.832023Jul 113368R2-No-
M6.732022Aug 283088R2-Yes-
M6.572023May 93296R2-Yes-
M6.52023May 203311R2-No-
M6.392023Feb 73213R2-No-
M6.362022Dec 143165R2-No-
M6.352023Feb 253229R2S1YesG3
M6.22022Sep 163098R2-No-
M6.032023Jan 153191R2-Yes-
M6.012023Sep 33413R2-Yes ?
M5.862022Oct 13110R2-YesG1
M5.862023Jul 113372R2-No-
M5.82023Mar 63243R2-Yes-
M5.762022May 43004R2-No-
M5.742022Dec 153165R2-No-
M5.722023Jul 173363R2S2Yes-
M5.682023May 203311R2-No-
M5.672023Jan 113184R2-Yes-
M5.542022May 193014R2-No-
M5.512023Aug 63386R2-Yes-
M5.52022Jan 202929R2S1Yes-
M5.412023Mar 303256R2S0Yes-
M5.392022Aug 263089R2-No-
M5.392023May 193311R2-No-
M5.322022May 43006R2-No-
M5.272022Mar 43234R2-Yes-
M5.252022Nov 73141R2-No-
M5.22023May 203311R2-No-
M5.152023Jan 103186R2S0Yes-
M5.092023Feb 213234R2-Yes-
M5.082022Aug 163078R2-No-
M5.042023Mar 53243R2-No-
M5.022023May 93296R2-No-
Number of days at geomagnetic storm intensity[29]
100
200
300
400
2019
2020
2021
2022
2023
2024
2025
2026
2027
2028
2029
2030
  •   Kp1
  •   Kp2
  •   Kp3
  •   Kp4
  •   Kp5 (G1)
  •   Kp6 (G2)
  •   Kp7 (G3)
  •   Kp8 (G4)
  •   Kp9 (G5)

2020

Solar flares in 2020[30]
10
20
30
40
50
60
Jan
Feb
Mar
Apr
May
Jun
Jul
Aug
Sep
Oct
Nov
Dec
  •   C
  •   M
  •   X
Number of days at geomagnetic storm intensity in 2020[30]
10
20
30
40
Jan
Feb
Mar
Apr
May
Jun
Jul
Aug
Sep
Oct
Nov
Dec
  •   Kp1
  •   Kp2
  •   Kp3
  •   Kp4
  •   Kp5 (G1)
  •   Kp6 (G2)
  •   Kp7 (G3)
  •   Kp8 (G4)
  •   Kp9 (G5)

On 29 May, the first C-class solar flares of Solar Cycle 25 took place, as well as the first M-class flare. Solar activity continued to increase in the following months, especially abruptly in October, with flares taking place on a near-daily basis by November. On 29 November, an M4.4 flare, the strongest of the cycle to date, took place, possibly indicating the solar cycle would be more active than initially thought.[31]

On 8 December, a small coronal mass ejection was found heading directly towards Earth shortly after a strong C-class solar flare, hitting the planet on 9-10 December and causing bright aurorae at high latitudes.[32][33]

2021

Solar flares in 2021[34]
50
100
150
200
Jan
Feb
Mar
Apr
May
Jun
Jul
Aug
Sep
Oct
Nov
Dec
  •   C
  •   M
  •   X
Number of days at geomagnetic storm intensity in 2021[34]
10
20
30
40
Jan
Feb
Mar
Apr
May
Jun
Jul
Aug
Sep
Oct
Nov
Dec
  •   Kp1
  •   Kp2
  •   Kp3
  •   Kp4
  •   Kp5 (G1)
  •   Kp6 (G2)
  •   Kp7 (G3)
  •   Kp8 (G4)
  •   Kp9 (G5)

The first X-class solar flare of the cycle took place on 3 July, peaking at X1.59.[35]

On 22 July, a total of six different active regions were seen on the solar disk for the first time since 6 September 2017.[36]

On 9 October, a M1.6 class solar flare erupted sending a coronal mass ejection that hit earth on 12 October triggering a (moderate) G2 geomagnetic storm.[37]

The second X-class flare of the solar cycle erupted on 28 October, producing a CME and a S1 solar radiation storm.[38] Reports initially predicted that the CME could graze Earth,[38] however geomagnetic storms on 30-31 October only reached a moderate Kp index of 4.[39]

On 3 and 4 November, the Kp index reached 8-, equivalent to a G4 geomagnetic storm.[40] This was the most intense geomagnetic storm to hit Earth since September 2017.

2022

Solar flares in 2022[29]
100
200
300
400
Jan
Feb
Mar
Apr
May
Jun
Jul
Aug
Sep
Oct
Nov
Dec
  •   C
  •   M
  •   X
Number of days at geomagnetic storm intensity in 2022[29]
10
20
30
40
Jan
Feb
Mar
Apr
May
Jun
Jul
Aug
Sep
Oct
Nov
Dec
  •   Kp1
  •   Kp2
  •   Kp3
  •   Kp4
  •   Kp5 (G1)
  •   Kp6 (G2)
  •   Kp7 (G3)
  •   Kp8 (G4)
  •   Kp9 (G5)

In late March, sunspot region 2975 released X1.3 and M9.6 flares, the former causing a G1 geomagnetic storm on 31 March despite being near the solar limb.[41] The region rotated out of view of Earth on 5 April, but helioseismic measurements on April 8 showed it still active on the far side of the Sun.[42] On 12 April, a Coronal Mass Ejection on the far side likely erupted from the region,[43] with helioseismic measurements showing the region to have intensified since crossing over the limb. As the region began rotating into view from Earth, a possibly X-class flare occurred on 15 April.[44]

After rotating to the visible hemisphere of the Sun, the regions of the sunspot complex were designated 2993 through 2996. On 17 April, sunspot group 2994 released an X1.2 flare.[45][46] However, the complex's activity subsided slightly in the next few days.[47] While crossing the solar limb, sunspot region 2992 emitted M7.3 and X2.2 flares, the latter being the strongest of the cycle yet.[47]

2023

Solar flares in 2023[48]
100
200
300
400
Jan
Feb
Mar
Apr
May
Jun
Jul
Aug
Sep
Oct
Nov
Dec
  •   C
  •   M
  •   X
Number of days at geomagnetic storm intensity in 2023[48]
10
20
30
40
Jan
Feb
Mar
Apr
May
Jun
Jul
Aug
Sep
Oct
Nov
Dec
  •   Kp1
  •   Kp2
  •   Kp3
  •   Kp4
  •   Kp5 (G1)
  •   Kp6 (G2)
  •   Kp7 (G3)
  •   Kp8 (G4)
  •   Kp9 (G5)

See also

References

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