SF Prep Notes

IIA astronomers devise method to estimate radial size of coronal mass ejections

Astronomers at the Indian Institute of Astrophysics devised a method to estimate the instantaneous expansion speed and radial size of coronal mass ejections from single-point spacecraft measurements, DST reported on 30 January 2025.

Summary

Astronomers at the Indian Institute of Astrophysics (IIA), an autonomous institute of the Department of Science and Technology, devised a novel method to estimate the instantaneous expansion speed and radial size of Coronal Mass Ejections (CMEs) using single-point in situ spacecraft measurements, DST reported on 30 January 2025. The IIA method matters because the radial dimension of a CME governs how long it and its geomagnetic storm affect Earth. CMEs are magnetised plasma bubbles from the Sun and the main drivers of geomagnetic storms that can disrupt communication, satellites and power grids.

Key facts

Reported
30 January 2025
Institute
Indian Institute of Astrophysics (DST)
Method
Instantaneous expansion speed and radial size of CMEs from single-point data
Why it matters
Radial size governs duration of geomagnetic storms

Practice MCQs 1 questions

Q1 Advanced

Astronomers of which institute devised a method, reported in January 2025, to estimate the radial size of coronal mass ejections from single-point measurements?

Show answer

Correct answer: A — Indian Institute of Astrophysics

PIB 2097599: astronomers at the Indian Institute of Astrophysics, an autonomous institute of DST, devised the method.

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