ASTR 370 · Lecture 03

The Solar Magnetic Field and the 11-Year Cycle

Differential rotation, the dynamo, and the real sunspot-number record

Learning Goals

  1. Describe the Babcock-Leighton dynamo mechanism qualitatively: differential rotation winding up a poloidal field into a toroidal field.
  2. Interpret the sunspot butterfly diagram and the 11-year sunspot cycle using real SILSO sunspot-number data.
  3. Compare Solar Cycle 24 and Solar Cycle 25’s real published maximum sunspot numbers.

Reading anchor: OpenStax Astronomy 2e (local extracted reference copy: references/openstax-astronomy-2e-extracted.txt) covers the Sun in Chapter 15 ("The Sun: A Garden-Variety Star"): 15.1 The Structure and Composition of the Sun, 15.2 The Solar Cycle, and 15.3 Solar Activity above the Photosphere. Chapter 15’s section numbering was cross-checked directly against its own embedded figure numbering this session (Figures 15.1 through 15.24 all appear under their matching section headers with no offset), so this citation is verified against the local extracted text rather than extrapolated by analogy from a prior course. OpenStax’s treatment throughout Chapter 15 is descriptive and qualitative; nearly every quantitative derivation in this course (the hydrostatic solar-atmosphere/scale-height argument, the sunspot magnetic-pressure balance, the Parker solar-wind critical-point argument and its numerical transonic solution, flare free-energy budgets, the Chapman-Ferraro magnetopause standoff distance, and the Dessler-Parker-Sckopke ring-current/Dst relation) goes well beyond OpenStax Astronomy 2e’s introductory level; each lecture states explicitly where this course extends beyond the assigned reading.

Why This Matters

Lecture 02 identified the magnetic field as the missing agent behind coronal heating; this lecture derives where that field comes from and how its large-scale behavior (the 11-year cycle) is tracked using the longest continuously maintained series of astronomical measurements, sunspot counts, setting up Lecture 04’s detailed sunspot physics.

Opening Phenomenon

Solar Cycle 25, which began around December 2019, reached a smoothed maximum monthly sunspot number of 160.8 in October 2024 (not-smoothed monthly peak 216 in August 2024) -- moderately stronger than the preceding Solar Cycle 24’s smoothed maximum of 116.4, both real, tracked values from the SILSO World Data Center sunspot-number catalogue (WDC-SILSO, Royal Observatory of Belgium).

First question: what here is directly observed or a published/live-verified measurement, and what follows only once a physical law is derived and applied?

Terms for This Lecture

differential rotation

Definition: Rotation whose angular speed varies with latitude and depth; the solar equator rotates faster than the poles.

Why it matters here: The Babcock-Leighton dynamo model explains the cyclic magnetic behavior qualitatively as follows: differential rotation stretches and winds up a large-scale poloidal (roughly north-south, dipole-like) field into a much stronger, wound-up toroidal (east-west) field over time; buoyant magnetic flux tubes from this toroidal field rise to the surface, forming sunspot pairs (Lecture 04), and the decay/diffusion of these sunspot pairs’ magnetic flux gradually regenerates a new poloidal field of opposite polarity, restarting the cycle roughly every 11 years (22 years for a full magnetic-polarity cycle).

Relationship: Use this term alongside dynamo; the lecture's quantitative model is summarized below.

\[ \text{Poloidal field} \xrightarrow{\text{differential rotation (shear)}} \text{Toroidal field} \xrightarrow{\text{buoyant rise, Babcock-Leighton decay}} \text{New poloidal field (reversed)} \]

Boundary or common confusion: Treating the 11-year sunspot cycle as strictly periodic or fully predictable. Real cycles vary substantially in amplitude and length (compare Cycle 24’s comparatively weak maximum to Cycle 25’s stronger, and largely under-predicted, maximum), and the dynamo mechanism, while capturing the essential physics, does not yet allow precise, first-principles prediction of a cycle’s exact strength in advance -- a genuine, disclosed limitation of current solar-cycle science.

Evidence We Need to Explain

Derivation and Model

Quantitative Tool

\[ \text{Poloidal field} \xrightarrow{\text{differential rotation (shear)}} \text{Toroidal field} \xrightarrow{\text{buoyant rise, Babcock-Leighton decay}} \text{New poloidal field (reversed)} \]

Worked Example

  1. Comparing the two most recent cycles’ real published smoothed maxima: Solar Cycle 25’s 160.8 is 1.38 times Solar Cycle 24’s 116.4 -- a moderately stronger cycle, consistent with Solar Cycle 25 substantially exceeding most pre-cycle predictions (many of which anticipated a cycle comparable to or weaker than Cycle 24).
  2. Solar Cycle 25 began from a smoothed minimum sunspot number of only 1.8 (essentially spot-free) around December 2019, illustrating the enormous dynamic range (a factor of 89) between solar minimum and maximum conditions that this course’s later space-weather units must account for.

Visual Reasoning

Trace the reasoning chain from raw observation or live-verified/published data to derived physical law to inferred quantity in this lecture’s figure.

  • Which stage is directly observed or a real published measurement?
  • Which stage is the physical law or derivation step?
  • What would change if an assumption in the derivation failed?
Lecture 03: The Solar Magnetic Field and the 11-Year CycleYears since cycle startSunspot latitude (degrees)Schematic butterfly diagram (idealized double-cycle, level 3): new-cycle spots emerge near +/-30 deg latitude and migrate toward the equator as each ~11-year cycle progresses.
The Solar Magnetic Field and the 11-Year Cycle: from observation to inferred quantity.

Common Misconception

Treating the 11-year sunspot cycle as strictly periodic or fully predictable. Real cycles vary substantially in amplitude and length (compare Cycle 24’s comparatively weak maximum to Cycle 25’s stronger, and largely under-predicted, maximum), and the dynamo mechanism, while capturing the essential physics, does not yet allow precise, first-principles prediction of a cycle’s exact strength in advance -- a genuine, disclosed limitation of current solar-cycle science.

Active Learning Segment

Using the real Cycle 24/Cycle 25 smoothed-maximum sunspot numbers, compute the percent difference between the two cycles, and discuss why this course’s space-weather risk assessment (Unit 7) should not assume every future cycle will resemble the two most recently observed ones.

Lab Connection

Lab 02 tabulates and compares real SILSO-sourced sunspot-number data across Cycles 24 and 25 and connects the sunspot-number proxy to the magnetic-flux-based sunspot area/field data used in Lecture 04.

Synthesis

The Babcock-Leighton dynamo, powered by the Sun’s differential rotation, produces the 11-year sunspot cycle tracked in the world’s longest continuous quantitative astronomical record -- and the individual, buoyantly emerged flux tubes responsible for that record are exactly the sunspots Lecture 04 now examines in detail.

References