ArticleslgStudy

astronomy

Transequatorial loop

Transequatorial loop is a astronomy topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Transequatorial loop rather than just read about it. In short: In solar physics, a transequatorial loop is a structure present in the solar corona that connects two different regions of opposite magnetic polarity in opposite hemispheres of the Sun. These connected regions are not limited to active regions, but are most commonly found during the times of maximum solar activity, the solar maximum.

Transequatorial loop — main illustration
Transequatorial loop — illustration

Key takeaways

  • Transequatorial loop belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Transequatorial loop to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Transequatorial loop from memory before moving on to harder problems.

Reference excerpt

In solar physics, a transequatorial loop is a structure present in the solar corona that connects two different regions of opposite magnetic polarity in opposite hemispheres of the Sun. These connected regions are not limited to active regions, but are most commonly found during the times of maximum solar activity, the solar maximum. Transequatorial loops play an integral role in the Babcock Model of solar dynamics and are therefore important to the future study of the solar dynamo.

Babcock Model

The idea of transequatorial loops was first developed by Horace W. Babcock in his 1961 model for the 11 year sunspot cycle. It explains that during each cycle, starting around the time of solar minimum, the Sun's internal, poloidal (parallel with the solar meridian) magnetic field is wrapped around the Sun via solar differential rotation. Over time, this process turns the field from primarily poloidal, to primarily toroidal (parallel with the solar equator) until the toroidal field reaches its maximum strength at the solar maximum. In order for it to return to its initial, poloidal state, Babcock theorized that the magnetic field from different hemispheres, which continuously emerges from the inside of the Sun into the solar atmosphere, would reconnect with each other forming transequatorial loops. After evidence for the existence of transequatorial loops was first observed in Skylab X-ray data, they were found to be more common during solar maximum then during solar minimum in accordance with the Babcock Model.

Characteristics

Transequatorial loops connect regions of opposite magnetic polarity on opposite solar hemispheres. Typically, they connect active regions with inactive regions, but can also connect active regions together and inactive regions together. Some regions may possess multiple transequatorial loops. In addition to this, about one third of all active regions possess at least one transequatorial loop and about one third of those possessing one have it associated with the preceding, or westernmost, polarity of the active region. Transequatorial loops have also been associated with flare activity and coronal mass ejections.

See also Solar corona Coronal seismology Coronal loop Solar prominence

References

Further reading Chen, Jie; Pevtsov, Alexei A.; Su, Jiangtao; Erdélyi, Robertus; Deng, Yuanyong; Yang, Shangbin; Song, Yongliang (April 2020). "Formation of Two Homologous Transequatorial Loops" (PDF). Solar Physics. 295 (4): 59. Bibcode:2020SoPh..295...59C. doi:10.1007/s11207-020-01625-z. S2CID 255071863. Pevtsov, Alexei A. (June 2004). "Transequatorial Connections: Loops or Magnetic Separators?". Proceedings of the International Astronomical Union. 2004 (IAUS223): 521–524. Bibcode:2004IAUS..223..521P. doi:10.1017/S1743921304006726.

Illustrations

Transequatorial loop: Pictured is the Sun as seen in soft x-ray with a transequatorial loop slightly right of center arcing across the solar equator.
Pictured is the Sun as seen in soft x-ray with a transequatorial loop slightly right of center arcing across the solar equator.
Transequatorial loop: Various examples of coronal loops.
Various examples of coronal loops.

Worked examples

Example 1 — a first encounter with Transequatorial loop

Start with the simplest possible case. Write down what Transequatorial loop claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In astronomy, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Transequatorial loop before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Transequatorial loop ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Transequatorial loop

In research
Transequatorial loop appears in astronomy research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Transequatorial loop in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Transequatorial loop is common in secondary-school and first-year university syllabi. It links to neighbouring topics Solar phenomena, Stellar phenomena, so understanding it makes those chapters shorter.
In everyday life
Look for Transequatorial loop outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.

Affiliate

Preply — study more efficiently by working with a personal tutor. 50% off.

How to study Transequatorial loop in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Transequatorial loop means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Transequatorial loop out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Transequatorial loop in simple terms?

In solar physics, a transequatorial loop is a structure present in the solar corona that connects two different regions of opposite magnetic polarity in opposite hemispheres of the Sun. These connected regions are not limited to active regions, but are most commonly found during the times of maximu…

Why does Transequatorial loop matter?

Because it connects several astronomy ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Transequatorial loop?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Transequatorial loop.

Tags

  • Solar phenomena
  • Stellar phenomena

Keep exploring