Fast changes between the solar seasons resolved by new sun clock

Date:
August 17, 2021
Source:
University of Warwick
Summary:
Violent activity on our Sun leads to some of the most extreme space
weather events on Earth, impacting systems such as satellites,
communications systems, power distribution and aviation. The
roughly 11 year cycle of solar activity has three 'seasons', each
of which affects the space weather felt at Earth differently: (i)
solar maximum, the sun is active and disordered, when space weather
is stormy and events are irregular (ii) the declining phase, when
the sun and solar wind becomes ordered, and space weather is more
moderate and (iii) solar minimum, when activity is quiet. Scientists
found that the change from solar maximum to the declining phase
is fast, happening within a few (27 day) solar rotations.



FULL STORY ========================================================================== Violent activity on our Sun leads to some of the most extreme
space weather events on Earth, impacting systems such as satellites, communications systems, power distribution and aviation. The roughly 11
year cycle of solar activity has three 'seasons', each of which affects
the space weather felt at Earth differently: (i) solar maximum, the sun
is active and disordered, when space weather is stormy and events are
irregular (ii) the declining phase, when the sun and solar wind becomes ordered, and space weather is more moderate and (iii) solar minimum,
when activity is quiet.


==========================================================================
In a new study led by the University of Warwick and published in The Astrophysical Journal, scientists found that the change from solar
maximum to the declining phase is fast, happening within a few (27 day)
solar rotations.

They also showed that the declining phase is twice as long in
even-numbered solar cycles as it is in odd-numbered cycles.

No two solar cycles are the same in amplitude or duration. To study the
solar seasons, the scientists built a sun clock from the daily sunspot
number record available since 1818. This maps the irregular solar cycles
onto a regular clock. The magnetic polarity of the sun reverses after
each roughly 11 year solar cycle giving a roughly 22 year magnetic cycle
(named after George Ellery Hale) and to explore this, a 22 year clock was constructed. The effect on space weather at earth can be tracked back
using the longest continuous records of geomagnetic activity over the
past 150 years, and once the clock is constructed, it can be used to study multiple observations of seasonal solar activity which affect the earth.

With the greater detail afforded by the sun clock, the scientists could
see that the switch from solar maximum to the declining phase is fast, occurring within a few (27 day) solar rotations. There was also a clear difference in the duration of the declining phase when the sun's magnetic polarity is 'up' compared to 'down': in even-numbered cycles it is around
twice as long as odd- numbered cycles. As we are about to enter cycle 25,
the scientists anticipate that the next declining phase will be short.

Lead author Professor Sandra Chapman of the University of Warwick
Department of Physics said: "By combining well known methods in a new
way, our clock resolves changes in the Sun's climate to within a few
solar rotations. Then you find the changes between some phases can be
really sharp.

"If you know you've had a long cycle, you know the next one's going to be short, we can estimate how long it's going to last. Knowing the timing of
the climate seasons helps to plan for space weather. Operationally it is
useful to know when conditions will be active or quiet, for satellites,
power grids, communications." The results also provide a clue to
understanding how the Sun reverses polarity after every cycle.

Professor Chapman adds: "I also think it is remarkable that
something the size of the sun can flip its magnetic field every 11
years, and going down-up is different to going up-down. Somehow
the sun 'knows which way up it is', and this is an intriguing
problem, at the heart of how the sun generates its magnetic field." ========================================================================== Story Source: Materials provided by University_of_Warwick. Note: Content
may be edited for style and length.


========================================================================== Journal Reference:
1. S. C. Chapman, S. W. McIntosh, R. J. Leamon, N. W. Watkins. The
Sun's
Magnetic (Hale) Cycle and 27 Day Recurrences in the aa Geomagnetic
Index.

The Astrophysical Journal, 2021; 917 (2): 54 DOI: 10.3847/1538-4357/
ac069e ==========================================================================

Link to news story: https://www.sciencedaily.com/releases/2021/08/210817131420.htm

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