PUNCH MISSION

NASA is launching PUNCH from Vandenberg to capture first-ever 3D images of the Sun's corona using four LEO satellites. By employing polarimetric techniques, the mission will track solar wind and CMEs, generating time-lapse videos and improving space weather forecasts critical to safeguarding Earth’s satellite and power infrastructures, enhancing our understanding.

Last Updated on 1st March, 2025
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Context:

NASA set to launch PUNCH mission.

PUNCH Mission

NASA is launching the PUNCH mission from Vandenberg Space Force Base, California.

The mission aims to enhance the understanding of the Sun’s atmosphere and solar winds by capturing the first 3D images of the corona (the Sun’s outer atmosphere) and tracking how disturbances evolve into space weather events like coronal mass ejections (CMEs).

Key Objectives of the Mission

3D Imaging of the Corona and Solar Wind

PUNCH will use polarization of light—a technique leveraging sunlight scattered by electrons in the corona—to construct detailed 3D maps of the Sun’s atmosphere. This allows scientists to observe how the corona transitions into the solar wind and identify forces driving solar phenomena.

Tracking Solar Storms

The mission will monitor coronal disturbances from their origin to their propagation through the inner solar system, creating "movies" of events like CMEs as they evolve.

Improving Space Weather Predictions

Data from PUNCH will improve forecasts of space weather events, which can disrupt satellites, power grids, and GPS systems on Earth.

Technology & Innovation

PUNCH comprises four identical satellites (each 64 kg) in Low Earth Orbit (LEO). Their combined imagery acts as a single "virtual telescope," providing a wider field of view than previous missions.

The satellites use polarizing filters to measure polarized light, enabling 3D reconstruction of the corona and solar wind structure.

Instrumentation

  • Three Wide Field Imagers (WFIs): Capture broad views of the corona.
  • One Narrow Field Imager (NFI): Focuses on the inner corona, similar to NASA’s SOHO satellite.
  • Cameras take images every 4–32 minutes, with unpolarized images captured every 8 minutes.

Expected Outcomes

PUNCH will create time-lapse videos of coronal disturbances evolving into solar winds and CMEs.

Polarization data will reveal the corona’s magnetic field interactions and solar wind acceleration mechanisms.

Improved predictions of solar storms’ impact on Earth.

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Source:

INDIAN  EXPRESS

PRACTICE QUESTION

Q. Which of the following are the significant impacts of solar wind?

  1. Erosion of the Earth's atmosphere.
  2. Induction of geomagnetically induced currents (GICs).
  3. Disruption of satellite operations and communication.
  4. Enhancement of the Earth's ozone layer. 

How many of the above statements are correct?

A) Only one

B) Only two

C) Only three

D) All four

Answer: C

Explanation:

Statement 1 is correct: Solar wind erosion has contributed to the loss of atmospheres on planets like Mars. While Earth's magnetosphere provides significant protection, some atmospheric escape still occurs due to solar wind interaction. This is a very slow process, not a short-term impact.

Statement 2 is correct: During geomagnetic storms driven by solar wind disturbances, rapid changes in Earth's magnetic field induce currents in long conductors like power grids and pipelines. 

Statement 3 is correct: Solar wind and associated space weather events can severely disrupt satellite operations. Increased radiation levels can damage satellite electronics. Communication and navigation (GPS) signals can be degraded or interrupted.

Statement 4 is incorrect: Solar wind does not enhance the ozone layer. In fact, energetic particles from space weather events can potentially deplete the ozone layer by triggering chemical reactions in the stratosphere.  

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