WASHINGTON, USA: NASA has chosen the Naval Research Laboratory’s (NRL’s) Wide-field Imager to be part of the Solar Probe Plus mission slated for launch no later than 2018.
The Solar Probe Plus, a small car-sized spacecraft will plunge directly into the sun's atmosphere approximately four million miles from our star's surface. It will explore a region no other spacecraft ever has encountered in an effort to unlock the sun's biggest mysteries.
For decades, scientists have known that the corona, or the outer atmosphere, is several hundreds of times hotter than the visible solar surface and that the solar wind accelerates up to supersonic speeds as it travels through the corona.
In the Solar Probe Plus mission, scientists hope to find answers to the questions: why is the solar corona so much hotter than the photosphere? And how is the solar wind accelerated? The answers to these questions can be obtained only through in-situ measurements of the solar wind down in the corona.
NRL’s Wide-field Imager for Solar Probe (WISPR) is one of five science investigations selected by NASA for this mission. It is the only optical investigation because the solar environment is so hot the instruments need to be tucked behind a heat shield.
NRL’s Dr. Russell Howard, the principal investigator, says, “This is an extremely exciting mission - no other spacecraft has ever gone this close - it is like the early voyagers of the earth, we don't really know what to expect, but we know, whatever it is, it is going to be spectacular.”
The imager is a telescope, which looks off to the side of the heat shield, and will make 2-D images of the sun's corona as the spacecraft flies through. But like a medical CAT scan, the orbit of the spacecraft through the corona will enable 3-D images and a determination of the 3-D structure of the corona.
The experiment actually will see the solar wind and provide 3-D images of clouds and shocks as they approach and pass the spacecraft. “We'll be flying through the structures that we've only seen from 100 million miles away. We'll be able to see all the phenomena (mass ejections, streamers, shocks, comets, and dust) up close. Other instruments will be able to measure the magnetic and electric fields and the plasma itself,” explains Howard.
This investigation complements instruments on the spacecraft by providing direct measurements of the plasma far away as well as near the spacecraft – the same plasma the other instruments sample.