The instrument tracks levels of methane and carbon dioxide, two gases crucial for studying the chemistry of Earth’s atmosphere.
A a long-standing solar mystery may have been solved by astronomers from the University of Hawaiʻi Institute for Astronomy (IfA), Brazil and Stanford University. Two decades ago, scientists discovered that the outer five percent of the Sun spins more slowly than the rest of its interior. In a new study, to be published in the journal Physical Review Letters, researchers describe the physical mechanism responsible for slowing the Sun’s outer layers.
Earth is “braking” the Sun
Team leader Kuhn said “The Sun won’t stop spinning anytime soon, but we’ve discovered that the same solar radiation that heats the Earth is ‘braking’ the Sun because of Einstein’s Special Relativity, causing it to gradually slow down starting from its surface.”
The Sun rotates on its axis at an average rate of about once per month but that rotation isn’t like, for example, the solid Earth or a spinning disk because the rate varies with solar latitude and distance from the center of the Sun.
The team used several years of data from NASA’s Solar Dynamics Observatory and the Helioseismic and Magnetic Imager satellite to measure a sharp down-turn in the Sun’s rotation rate in its very outer 150km. Kuhn said, “This is a gentle torque that is slowing it down, but over the Sun’s 5 billion year lifetime it has had a very noticeable influence on its outer 35,000km.” Their paper describes how this “photon-braking effect” should be at work in most stars.
This change in rotation at the Sun’s surface affects the large-scale solar magnetic field and researchers are now trying to understand how the solar magnetism that extends out into the corona and finally into the Earth’s environment will be affected by this braking.
The research will appear in the January issue of Physical Review Letters, and is available online at https://arxiv.org/abs/1612.00873.