Tuesday, January 26, 2016

ESA’s Integral Mission X-rays Earth's Aurora

Artist's impression of ESA's Integral gamma-ray observatory. Credit: ESA

Normally busy with observing high-energy black holes, supernovas and neutron stars, ESA’s Integral space observatory recently had the chance to look back at our own planet’s aurora. Auroras are well known as the beautiful light shows at polar latitudes as the solar wind interacts with Earth’s magnetic field. As energetic particles from the Sun are drawn along Earth’s magnetic field, they collide with different molecules and atoms in the atmosphere to create dynamic, colorful light shows in the sky, typically in green and red.

But what may be less well known is that auroras also emit X-rays, generated as the incoming particles decelerate.

Integral detected high-energy auroral X-rays on 10 November 2015 as it turned to Earth – although it was looking for something else at the time.


Its task was to measure the diffuse cosmic X-ray background that arises naturally from supermassive black holes that are gobbling up material at the centers of some galaxies.

To achieve this, Integral records the X-ray brightness with and without the Earth in the way, blocking the background. These types of measurements help astronomers estimate how many distant supermassive black holes there are in the Universe.

Sequence of X-ray images taken by Integral’s IBIS/ISGRI instrument on 10 November 2015 at time intervals of about 8 minutes. The images cover the energy range 17–60 keV (although higher emission energies were also recorded) and show intense auroral emission first visible on the near-side of Earth (roughly around east Siberia, north of Japan, at around 11:00 GMT), and then on the opposite side of the pole for a more prolonged period and over a wider area in the following hours, first above Canada and later above Greenland.  Earth’s position is shown by its coordinate grid and is kept fixed, while it is drifting towards the border of the instrument’s field-of-view (the nearing edge at the left at the start of the sequence). Its apparent size increases as the spacecraft approaches Earth on its elliptical orbit (Integral orbits Earth in a highly eccentric 64 hour orbit that takes it between about 10 000 km and 140 000 km from Earth). Credit: ESA/Integral/ E. Churazov (IKI/MPA)/ M. Türler (ISDC/Univ. of Geneva)
Sequence of X-ray images taken by Integral’s IBIS/ISGRI instrument on 10 November 2015 at time intervals of about 8 minutes. The images cover the energy range 17–60 keV (although higher emission energies were also recorded) and show intense auroral emission first visible on the near-side of Earth (roughly around east Siberia, north of Japan, at around 11:00 GMT), and then on the opposite side of the pole for a more prolonged period and over a wider area in the following hours, first above Canada and later above Greenland.  Earth’s position is shown by its coordinate grid and is kept fixed, while it is drifting towards the border of the instrument’s field-of-view (the nearing edge at the left at the start of the sequence). Its apparent size increases as the spacecraft approaches Earth on its elliptical orbit (Integral orbits Earth in a highly eccentric 64 hour orbit that takes it between about 10 000 km and 140 000 km from Earth). Credit: ESA/Integral/ E. Churazov (IKI/MPA)/ M. Türler (ISDC/Univ. of Geneva)

Unfortunately, on this occasion, the X-rays from Earth’s aurora drowned out the cosmic background – but the observations were not a waste.

They also help us to understand the distribution of electrons raining into Earth’s upper atmosphere, and they reveal interactions between the solar wind and Earth’s protective magnetic bubble, or magnetosphere.

“Auroras are transient, and cannot be predicted on the timeframe that satellite observations are planned, so it was certainly an unexpected observation,” comments Erik Kuulkers, Integral project scientist.

“It’s also quite unusual for us to point the spacecraft at Earth: it requires innovative planning by the operations teams to coordinate such a dedicated set of maneuvers to ensure it can operate safely with Earth inside the instruments’ field of view and then return to its standard observing program.

“Although the original background X-ray measurements didn’t go quite to plan this time, it was exciting to capture such intense auroral activity by chance.”

Credit: ESA

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