Space lasers to track Earth’s ice

With new space missions come new and improved capabilities. And for those interested in what’s happening to the ice on Planet Earth, we have two ventures this year that are going to make a major contribution to our understanding.

Ice is the “climate canary”. The loss, and the rate of that loss, tell us something about how global warming is progressing.

In the Arctic, the most visible sign is the decline of sea-ice, which, measured at its minimum extent over the ocean in September, is reducing by about 14% per decade.

At the other pole, the marine floes look much the same as they did in the earliest satellite imagery from the 1960s, but land ice is in a negative phase.

Something on the order of 160 billion tonnes are being lost annually, with most of that mass going from the west of the White Continent.

The two 2018 missions of interest that will pick up these trends and extend them into the future are Grace Follow-On and IceSat-2.

The former is the successor to the highly successful US-German gravity spacecraft that operated from 2002 to 2017.

Grace is actually a pair of satellites that pursue each other around the globe in formation with a separation of 220km.

They accelerate and decelerate in turn as they pass over variations in the local gravity field. It is a very small effect – a change in distance equivalent to the thickness of a human hair – but discernible to the microwave ranging instrumentation carried on the satellites.

Because the gravity variations are a function of changes in mass, the pair are able, literally, to weigh the ice sheets sitting below them on land as they pass overhead.

Its from the first Grace mission’s observations, for example, that we know Greenland is currently losing about 280 billion tonnes of ice to the ocean every year.

It’s a significant contribution to the 3.4mm per annum rise in global sea levels.

Grace Follow-On will work in the same way as its predecessor did, but it will also demonstrate a laser range-finder.

“It’s a first in space, and it allows us to do the ranging with much higher precision – a factor of 10 to 20 times better,” says US space agency (Nasa) deputy project scientist Felix Landerer. “So, we go from that human hair thickness down to the scale of large viruses.”

Stop and think about that for a second – measuring the distance between London and Sheffield to the accuracy of the width of a large virus.

This impressive German laser technology will form the basis of the orbiting instruments that will eventually be used to detect the cataclysmic collisions of the biggest black holes in the cosmos. Stay tuned. That mission to sense gravitational waves – it’s called Lisa – will launch in the 2030s.

Back here on Earth, the other ice project this year also involves a laser. IceSat-2 will fire six green beams of light at the Arctic floes and land ice-sheets to measure their shape.

Simple but effective: the satellite times the return of the reflected beams and converts that into a range, which in turn is converted into an elevation.

Again, the new satellite is a successor. The previous effort in the 2000s, known as IceSat-1, showed remarkable promise as an ice-sensing tool. However, its mission was blighted by fragile diode technology, and it could only use its laser for a handful of months a year.

“IceSat-2 is a micro-pulse laser,” says Nasa project scientist Thorsten Markus. “The strength of the laser pulses is much, much smaller than it was on IceSat-1, and we also have a very high pulse repetition frequency of 10kHz. Basically, the laser is always on, which makes it much less stressful on the diodes.

“We’ve had some diodes running [in test form] for seven, eight years now. So, conceptually, one laser should last a whole mission of seven years and we have two lasers onboard,” he told BBC News.

The hope is IceSat-2 will be up and operating before Europe’s ageing CryoSat mission dies.

CryoSat has been pursing very similar objectives, except its “tape measure” is a radar altimeter.

A period of overlap would allow for an inter-comparison. This is not wholly straightforward. The laser on IceSat and the radar on CryoSat don’t range to exactly the same surface.

In the former’s case, the light beams are reflected off the very top of any snow covering the ice. In the latter’s case, the radar can penetrate the snowpack for many tens of centimetres, depending on conditions, before scattering back to the spacecraft.

Scientists have to use modelled assumptions based on the regional climatology to account for any bias.

“It’s an important consideration,” says CryoSat scientist Anna Hogg from Leeds University, UK.

“If you get an extreme melt year, you can actually get a new ice layer forming in the snowpack as water trickles down from the surface and refreezes. That’s what happened during 2012 when the whole of Greenland experienced melt.

“Afterwards, CryoSat saw a step change in elevation equivalent to a 0.5m increase just because the scattering horizon had risen. It made it look like Greenland had grown ice, whereas in reality it had very probably lost mass.”

Dr Hogg has just returned from Antarctica where she has been drilling cores to try to understand better the layering in the snowpack and its influence on the radar’s return signal.

She did this as CryoSat flew overhead, in addition to an aeroplane equipped with two types of radar ranging instrument. One used the same radio frequency (Ku-band) as Cryosat; the other used a higher frequency (Ka-band) which should scatter a lot closer to the actual surface of the snowpack.

The thinking in Europe is that if CryoSat has a follow-on, it should be dual, Ku-Ka band to try to get a more direct measure of the amount of snow lying on top of the ice. This would be particularly important for sensing sea-ice thickness.

In the Arctic, CryoSat does this by measuring the height (the freeboard) of the floating ice sticking just above the ocean water and then calculating the corresponding submerged (the draft) ice. It is roughly 1/9th above and 8/9ths below.

“That becomes problematic in the Antarctic where the snow can be so heavy that it compresses the ice to the point that it’s sitting at the water-line; in other words, there is no ice freeboard,” explains Leeds colleague Rachel Tilling.

While Dr Hogg was examining snow-layering conditions on land in recent weeks, Dr Tilling was doing the same with the marine floes surrounding Antarctica.

She’s hopeful that the data gathered as she cruised across the Weddell Sea will lead to some of the first robust satellite sea-ice thickness maps for the region. And, certainly, this effort should be greatly assisted in the short-term if IceSat and the existing CryoSat can also run alongside each other for a good period of time. That’s because the differences in how each senses the surface would lead to a much improved description of snow loading, too.

“It’s a new opportunity that we haven’t had before and can only mean we will get more accurate sea-ice thickness measurements. That’s exciting,” Dr Tilling told BBC News.

  • Cryosat’s radar has the resolution to see the Arctic’s floes and leads
  • Some 8/9ths of the ice tends to sit below the waterline – the draft
  • The radar senses the height of the freeboard – the ice above the waterline
  • Knowing this 1/9th figure allows Cryosat to work out sea-ice thickness
  • The thickness multiplied by the area of ice cover produces a volume
  • IceSat-2 will do exactly the same as Cryosat but with a laser instrument

source: bbc

Design call for ‘solar sentinel’ mission

UK scientists and engineers will play a leading role in developing a satellite that can warn if Earth is about to be hit by damaging solar storms.

The European Space Agency has requested studies be undertaken to design the mission that would launch in the 2020s.

Explosive eruptions from the Sun can lead to widespread disruption on our planet – degrading communications, even knocking over power grids.

The satellite’s observations would increase the time available to prepare.

Esa has a working name for the new mission – “Lagrange”, which reflects the position the satellite would take up in space.

The plan is to go to a gravitational “sweetspot” just behind the Earth in its orbit around the Sun known as “Lagrangian Point 5”.

Spacecraft that are sited there do not have to use so much fuel to maintain station – but there is an even bigger operational rationale to use this location: it is the perfect spot to see that part of the Sun which is about to rotate into view of the Earth.

“So, not only do you get a preview of the active regions and how complicated they are, but if the Sun throws something out you also get to track it from the side,” explained British solar physicist Prof Richard Harrison.

“Imagine a fist coming directly at your face – it’s difficult to say how far away it is; but if you see that fist from the side, it’s much easier,” he told BBC News.

Esa signed four so-called Phase AB1 contracts on Friday at its mission control centre in Darmstadt, Germany.

These include two parallel industrial studies – to be led by Airbus UK and OHB System of Germany – to spec the spacecraft bus, or chassis, and the process for integrating all the satellite’s instruments.

The aerospace companies will also work out how the entire mission would be managed, from launch to the end of service life.

The actual design of the onboard instruments is the subject of the other two contracts. Both of these will be directed by British-led consortia.

RAL (Rutherford Appleton Laboratory) Space will assess the requirements of the mission’s “remote sensing package” – that is, the instruments that discern what the Sun is doing by looking at it.

The UK’s Mullard Space Science Laboratory (MSSL) will scope the “in-situ package” – those instruments that investigate the Sun’s activity by directly sensing emitted particles and magnetic fields.

Although led from Britain, these efforts will of course draw on talents from across European member states.

Presentational grey line

The different Lagrangian Points

  • These are the sweetspots in the Sun-Earth-Moon system
  • They are places where gravitational forces balance out
  • Satellites at these locations use less fuel to maintain station
  • L5 is at a 60-degree offset, and follows Earth in its orbit
  • A complementary US mission would very likely go to L1
Presentational grey line

Solar storms are a common occurrence. Our star will sometimes despatch big bursts of shortwave and longwave radiation, superfast particles and colossal volumes of charged gas (plasma) in our direction. This material is also threaded with strong magnetic fields.

When these emissions encounter Earth, they can kick-off a number of effects in modern infrastructure, from glitching electronics in aircraft avionics and in orbiting spacecraft to increasing the interference heard on radio broadcasts, such as those from the BBC.

Numerous studies have warned of the possible consequences of a major solar storm impacting Earth.

Just last year, a government report said the UK economy would lose £1bn for every day the GPS satellite-navigation service was unavailable.

“What we need is a ‘solar sentinel’, watching the Sun to tell us what is going to happen in advance,” said Dr Ralph Cordey from Airbus UK.

“This is an area where the UK’s expertise is well established. It’s also the case that the impacts of ‘space weather’ are regarded as a priority in the UK with the issue recognised in the register of civil hazards, along with pandemic flu, severe flooding and volcanic eruptions.”

The Lagrange mission concept is being overseen by the Space Situational Awareness programme at Esa to which the UK committed €22m, over 4 years, at the last gathering of Europe’s space ministers in December 2016.

When the ministers next meet, in December 2019, they will have the results of the new studies and should hopefully be in a position then to sanction the mission’s full development.

One key instrument that will have to be carried is a coronagraph.

This is a device that blocks the full glare of the Sun’s disc so that the beginnings of an eruption are more easily seen.

At the moment, space weather forecasters are relying on a coronagraph on a 20-year-old spacecraft called Soho.

“A coronagraph gives us the first warning that something really is happening,” said Prof Harrison, who is the chief scientist at RAL Space.

“A coronal mass ejection is a million times weaker in intensity than the Sun itself. It’s a contrast problem: if you didn’t block off the Sun, you wouldn’t see it.”

It is likely the Americans will launch a similar mission in the coming years that will sit directly in front of Earth in line with the Sun. Taking the two perspectives together will give solar storm forecasters the best assessment of potential impacts.

source: BBC