“It’s exciting to still be observing ‘firsts’ like these simultaneous aurora so many years into the mission. Solar maximum is when the height of solar activity peaks in the Sun’s 11-year solar cycle, meaning CMEs and SEPs are expected to increase in frequency and continue to impact Mars’ atmosphere. The Sun is growing more and more active with events, such as flares and CMEs, as it approaches solar maximum in 2024-2025. This light show is a sign of things to come for Mars and for the MAVEN team. “They’re both increasing with solar activity, so we hope it keeps happening!” A sign of the storms to come “I was so surprised to see proton aurora at the same time as diffuse aurora, because it had never happened before,” she said. Sumedha Gupta, a postdoctoral researcher with the IUVS team at the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder, first noticed the coincidence during her routine check of incoming data a few days after the event. These “proton aurora” just happened to coincide with the arrival of even more dynamic energic particles that penetrated deeper into the atmosphere, creating diffuse aurora visible across the entire nightside. When the incoming solar wind hits all this extra hydrogen, the dayside of the planet lights up with ultraviolet emissions. These dust storms warm the atmosphere enough to allow water vapor to reach high altitudes, where it is broken up by solar ultraviolet radiation, releasing hydrogen atoms in the process. Mars is at the end of dust storm season, which occurs every Mars year during its closest approach of the Sun. Part of the reason that this incredible duo was observed simultaneously came down to timing. MAVEN’s Imaging Ultraviolet Spectrograph (IUVS) instrument observed two types: diffuse aurora and proton aurora. Particles unleashed by the solar storm bombarded Mars’ atmosphere, causing bright auroras at ultraviolet wavelengths. “This allowed the MAVEN team to anticipate some exciting disturbances in Mars’ atmosphere from the impacts of the interplanetary CME and the associated SEPs.” “By utilizing space weather models of CME propagation, we determined when the structure would arrive and impact Mars,” said Christina Lee, a space physicist at the University of California, Berkeley, who is a member of the MAVEN mission team and is collaborating with the Moon to Mars Space Weather Analysis Office scientists. In fact, many of MAVEN’s instruments were collectively able to measure the strength of the solar storm, including the Extreme Ultraviolet Monitor, the Magnetometer, the Solar Wind Ion Analyzer, and the Solar Wind Electron Analyzer. The SEPs that were accelerated ahead of the CME were observed at Mars by MAVEN’s SEP detector on Aug. This CME produced one of the brightest solar energetic particle (SEP) events that the MAVEN spacecraft has ever observed. This interplanetary CME impacted Mars a few days later. The flare activity was accompanied by a coronal mass ejection (CME), a massive explosion of gas and magnetic energy that leaves the Sun and propagates through space. 27, an active region on the Sun produced a series of solar flares, which are intense bursts of radiation. Real-time analysis and simulations of the solar eruptions from NASA’s Moon to Mars Space Weather Analysis Office also allowed the MAVEN team to correctly predict when the developing solar storm would reach the Red Planet.Īccurate space weather forecasting is critical to help protect current missions and future human explorers at the Red Planet because unlike Earth, Mars lacks a global magnetic field to shield against the damaging radiation solar storms can bring. MAVEN – the Mars Atmosphere and Volatile Evolution mission – is the only asset at Mars able to observe the Sun’s activity and the response of the thin Martian atmosphere at the same time.
0 Comments
Leave a Reply. |
AuthorWrite something about yourself. No need to be fancy, just an overview. ArchivesCategories |