Image from the Solar Dynamics Observatory mission of the solar disk with multiple sunspots, which appear dark compared with their surroundings.Credit: HMI/SDO/NASA
Licence type: Attribution-ShareAlike (CC BY-SA 4.0)
Researchers at the Center of Excellence in Space Sciences India
at IISER Kolkata have discovered a new relationship between the Sun’s
magnetic field and its sunspot cycle, that can help predict when the
peak in solar activity will occur. Their work indicates that the maximum
intensity of solar cycle 25, the ongoing sunspot cycle, is imminent and
likely to occur within a year. The new research appears in Monthly Notices of the Royal Astronomical Society: Letters.
Our star, the Sun, is made up of hot ionized gas known as plasma. Huge plasma flows and convection conspire together to form magnetic fields inside the Sun which manifest on the surface as dark spots. These sunspots are comparable to the size of the Earth and are seats of intense magnetism, about 10,000 times stronger than the Earth’s magnetic field.
Sometimes the sunspot magnetic fields are disrupted in violent events which result in the birth of solar magnetic storms such as flares or coronal mass ejections. These storms release high energy radiation and hurl vast amounts of magnetized plasma in to outer space. The most intense of these storms can cause serious damage to orbiting satellites, electric power grids and telecommunications when Earth directed.
Centuries of observations starting from the early 1600s show that the number of sunspots observed on the Sun varies periodically. Approximately every 11 years the number of spots and the intensity of solar activity reach a peak when the most violent perturbations in planetary space environments – or space weather – are expected. However, predicting when this peak is going to occur has remained challenging.
The solar cycle is produced by a dynamo mechanism driven by energy from plasma flows inside the Sun. This dynamo mechanism is understood to involve two primary components of the Sun’s magnetic field, one which manifests in the cycle of sunspots and another which manifests in a recycling of the large-scale dipole field of the Sun; the latter is much like the Earth’s magnetic field – stretching from one pole of the Sun to another. With the cycle of sunspots, the Sun’s dipole field is also observed to wax and wane in strength, the north and south magnetic poles swap places, also every 11 years.
In 1935, Swiss astronomer Max Waldmeier discovered that the faster the rate of rise of a sunspot cycle the stronger its strength, so stronger cycles take less time to rise to their peak intensity. This relationship has often been utilised to forecast the strength of a sunspot cycle based on observations of its early rising phase.
In a research manuscript appearing in the Monthly Notices of the Royal Astronomical Society Letters, Priyansh Jaswal, Chitradeep Saha and Dibyendu Nandy of IISER Kolkata report the discovery of a new relationship, namely, the rate of decrease in the Sun’s dipole magnetic field is also related to the rate of rise of the ongoing sunspot cycle.
This discovery, utilising decades-old data archives from multiple ground-based solar observatories around the world, complements the Waldmeier effect, connecting the two primary magnetic field components of the Sun and supporting the theory that the evolution of sunspots are integral to the functioning of the solar dynamo process rather than being a mere symptom of it.
The scientists demonstrate how observations of the rate of decrease of the Sun’s dipole magnetic field can be usefully combined with sunspot observations to predict when the ongoing cycle would peak. Their analysis suggests that the maximum of solar cycle 25 is most likely to occur in early 2024 with an uncertainty in the estimate that ranges to September 2024.
With this discovery, a new window opens up for forecasting the timing of the peak of solar cycles - when the most intense activity and most frequent space weather disturbances are expected.
Our star, the Sun, is made up of hot ionized gas known as plasma. Huge plasma flows and convection conspire together to form magnetic fields inside the Sun which manifest on the surface as dark spots. These sunspots are comparable to the size of the Earth and are seats of intense magnetism, about 10,000 times stronger than the Earth’s magnetic field.
Sometimes the sunspot magnetic fields are disrupted in violent events which result in the birth of solar magnetic storms such as flares or coronal mass ejections. These storms release high energy radiation and hurl vast amounts of magnetized plasma in to outer space. The most intense of these storms can cause serious damage to orbiting satellites, electric power grids and telecommunications when Earth directed.
Centuries of observations starting from the early 1600s show that the number of sunspots observed on the Sun varies periodically. Approximately every 11 years the number of spots and the intensity of solar activity reach a peak when the most violent perturbations in planetary space environments – or space weather – are expected. However, predicting when this peak is going to occur has remained challenging.
The solar cycle is produced by a dynamo mechanism driven by energy from plasma flows inside the Sun. This dynamo mechanism is understood to involve two primary components of the Sun’s magnetic field, one which manifests in the cycle of sunspots and another which manifests in a recycling of the large-scale dipole field of the Sun; the latter is much like the Earth’s magnetic field – stretching from one pole of the Sun to another. With the cycle of sunspots, the Sun’s dipole field is also observed to wax and wane in strength, the north and south magnetic poles swap places, also every 11 years.
In 1935, Swiss astronomer Max Waldmeier discovered that the faster the rate of rise of a sunspot cycle the stronger its strength, so stronger cycles take less time to rise to their peak intensity. This relationship has often been utilised to forecast the strength of a sunspot cycle based on observations of its early rising phase.
In a research manuscript appearing in the Monthly Notices of the Royal Astronomical Society Letters, Priyansh Jaswal, Chitradeep Saha and Dibyendu Nandy of IISER Kolkata report the discovery of a new relationship, namely, the rate of decrease in the Sun’s dipole magnetic field is also related to the rate of rise of the ongoing sunspot cycle.
This discovery, utilising decades-old data archives from multiple ground-based solar observatories around the world, complements the Waldmeier effect, connecting the two primary magnetic field components of the Sun and supporting the theory that the evolution of sunspots are integral to the functioning of the solar dynamo process rather than being a mere symptom of it.
The scientists demonstrate how observations of the rate of decrease of the Sun’s dipole magnetic field can be usefully combined with sunspot observations to predict when the ongoing cycle would peak. Their analysis suggests that the maximum of solar cycle 25 is most likely to occur in early 2024 with an uncertainty in the estimate that ranges to September 2024.
With this discovery, a new window opens up for forecasting the timing of the peak of solar cycles - when the most intense activity and most frequent space weather disturbances are expected.
Science contacts:
Dibyendu Nandi
Professor of Physics and Head, Center of Excellence in Space Sciences India
Indian Institute of Science Education and Research Kolkata
dnandi@iiserkol.ac.in
Priyansh Jaswal
PhD Student, Center of Excellence in Space Sciences India
Indian Institute of Science Education and Research Kolkata
pj22rs046@iiserkol.ac.in
Phone: +91 8219647798
Media contact:
Robert Massey
Royal Astronomical Society
Mob: +44 (0)7802 877699
press@ras.ac.uk
Further information
Discovery
of a relation between the decay rate of the Sun’s magnetic dipole and
the growth rate of the following sunspot cycle: a new precursor for
solar cycle prediction”, 2023, Jaswal, P., Saha, C., and Nandy, D., Monthly Notices of the Royal Astronomical Society: Letters
Notes for editors:
The Royal Astronomical Society (RAS), founded in 1820, encourages and
promotes the study of astronomy, solar-system science, geophysics and
closely related branches of science. The RAS organises scientific
meetings, publishes international research and review journals,
recognises outstanding achievements by the award of medals and prizes,
maintains an extensive library, supports education through grants and
outreach activities and represents UK astronomy nationally and
internationally. Its more than 4,000 members (Fellows), a third based
overseas, include scientific researchers in universities, observatories
and laboratories as well as historians of astronomy and others.
The RAS accepts papers for its journals based on the principle of peer review, in which fellow experts on the editorial boards accept the paper as worth considering. The Society issues press releases based on a similar principle, but the organisations and scientists concerned have overall responsibility for their content.
The RAS accepts papers for its journals based on the principle of peer review, in which fellow experts on the editorial boards accept the paper as worth considering. The Society issues press releases based on a similar principle, but the organisations and scientists concerned have overall responsibility for their content.
