Forum for Science, Industry and Business

Sponsored by:     3M 
Search our Site:

 

NASA plans twin sounding rocket launches over Norway this winter

25.11.2015

This winter, two sounding rockets will launch through the aurora borealis over Norway to study how particles move in a region near the North Pole where Earth's magnetic field is directly connected to the solar wind. After the launch window opens on Nov. 27, 2015, the CAPER and RENU 2 rockets will have to wait for low winds and a daytime aurora before they can send their instrument payloads soaring through the Northern Lights.

Both instrument packages are studying phenomena related to the cusp aurora, a particular subset of the Northern Lights in which energetic particles are accelerated downward into the atmosphere directly from the solar wind - that is, the constant outward flow of solar material from the sun.


An aurora is seen over Greenland on April 2, 2011. Two NASA sounding rockets will launch into a particular type of aurora called a cusp aurora this winter to study different processes related to the particle acceleration that causes cusp auroras. The cusp is a region near the North Pole where Earth's magnetic field is directly connected to the solar wind, allowing daytime auroras to form.

Credits: NASA/University of Maryland, College Park/Robert Michell

Though cusp auroras are not particularly rare, they are often difficult to spot because they only happen during the day, when sunlight usually drowns out what would otherwise be a spectacular light show. However, because the magnetic North Pole is offset from the geographic North Pole, it's often possible to see cusp auroras in Northern Europe near the winter solstice.

"The magnetic pole is tilted towards North America, putting this magnetic opening--the cusp--at a higher latitude on the European side," said Jim LaBelle, principal investigator on the CAPER sounding rocket at Dartmouth College in Hanover, New Hampshire. "Combine that extra-high latitude with the winter solstice--when nights are longest, especially as you go farther north--and you can sometimes see this daytime aurora with the naked eye."

The two sounding rocket teams will also employ data from ground-based radars to detect the cusp aurora even in the case of clouds.

CAPER

CAPER, short for Cusp Alfven and Plasma Electrodynamics Rocket, will be first in the queue to launch. CAPER is investigating the electromagnetic, or EM, waves that can accelerate electrons down into Earth's atmosphere or up out to space. The electrons that are accelerated downward collide with particles in the atmosphere, releasing light and creating the cusp aurora--so spotting aurora activity at the cusp alerts the scientists that the EM wave motions they're interested in must also be present.

CAPER, flying on a four-stage Oriole IV sounding rocket, carries three instruments--one to measure low-frequency EM waves, one to measure high-frequency EM waves, and one to measure the number of particles at different energy levels. LaBelle's team will compare these observations to get a better idea of how the EM waves accelerate the particles.

"The difficulty is measuring the high-frequency waves and their associated particles," said LaBelle. "They're moving at up to a million cycles per second, so the instruments have to be able to detect changes in the waves and collect enough particles to match up."

RENU 2

The other sounding rocket to launch, a four-stage Black Brant XII-A, is the second iteration of the Rocket Experiment for Neutral Upwelling, or RENU 2, which will study the relationship between the inflow of electrons that creates the cusp aurora, electric currents flowing along magnetic field lines, and dense columns of heated neutral atoms in the upper atmosphere.

Though scientists have long known that the density of neutral atoms within the atmosphere can change throughout the day because of heating by sunlight, the original understanding was that the heating--and the extra-dense layers of neutral particles--was driven horizontally. However, some satellites have hit speed bumps as they have orbited through Earth's magnetic cusp--their acceleration briefly slowed, which indicates a small vertical slice of higher-density neutral atoms that are harder to travel through.

"When solar wind electrons collide with atmospheric electrons, they transfer some of their energy, heating the atmospheric electrons," said Marc Lessard, principal investigator for RENU 2 at the University of New Hampshire in Durham. "The higher heat means the electron populations expand upward along the magnetic field lines."

This upward flow of negatively-charged particles creates a vertical electric field, which in turn pulls up the positively-charged and neutral particles, increasing the atmospheric density in columns rather than horizontal layers. To study the phenomenon, RENU 2 will carry several instruments, including instruments to measure the electric and magnetic fields, neutral and charged particle flows, and temperatures.

Though CAPER and RENU 2 will collect data for only a few minutes each, suborbital sounding rockets are a valuable way to study space and the upper atmosphere at relatively low cost.

The CAPER and RENU 2 launches are supported through NASA's Sounding Rocket Program at the Goddard Space Flight Center's Wallops Flight Facility in Virginia. NASA's Heliophysics Division manages the sounding rocket program.

Susan Hendrix | EurekAlert!

More articles from Physics and Astronomy:

nachricht Structured light and nanomaterials open new ways to tailor light at the nanoscale
23.04.2018 | Academy of Finland

nachricht On the shape of the 'petal' for the dissipation curve
23.04.2018 | Lobachevsky University

All articles from Physics and Astronomy >>>

The most recent press releases about innovation >>>

Die letzten 5 Focus-News des innovations-reports im Überblick:

Im Focus: BAM@Hannover Messe: innovative 3D printing method for space flight

At the Hannover Messe 2018, the Bundesanstalt für Materialforschung und-prüfung (BAM) will show how, in the future, astronauts could produce their own tools or spare parts in zero gravity using 3D printing. This will reduce, weight and transport costs for space missions. Visitors can experience the innovative additive manufacturing process live at the fair.

Powder-based additive manufacturing in zero gravity is the name of the project in which a component is produced by applying metallic powder layers and then...

Im Focus: Molecules Brilliantly Illuminated

Physicists at the Laboratory for Attosecond Physics, which is jointly run by Ludwig-Maximilians-Universität and the Max Planck Institute of Quantum Optics, have developed a high-power laser system that generates ultrashort pulses of light covering a large share of the mid-infrared spectrum. The researchers envisage a wide range of applications for the technology – in the early diagnosis of cancer, for instance.

Molecules are the building blocks of life. Like all other organisms, we are made of them. They control our biorhythm, and they can also reflect our state of...

Im Focus: Spider silk key to new bone-fixing composite

University of Connecticut researchers have created a biodegradable composite made of silk fibers that can be used to repair broken load-bearing bones without the complications sometimes presented by other materials.

Repairing major load-bearing bones such as those in the leg can be a long and uncomfortable process.

Im Focus: Writing and deleting magnets with lasers

Study published in the journal ACS Applied Materials & Interfaces is the outcome of an international effort that included teams from Dresden and Berlin in Germany, and the US.

Scientists at the Helmholtz-Zentrum Dresden-Rossendorf (HZDR) together with colleagues from the Helmholtz-Zentrum Berlin (HZB) and the University of Virginia...

Im Focus: Gamma-ray flashes from plasma filaments

Novel highly efficient and brilliant gamma-ray source: Based on model calculations, physicists of the Max PIanck Institute for Nuclear Physics in Heidelberg propose a novel method for an efficient high-brilliance gamma-ray source. A giant collimated gamma-ray pulse is generated from the interaction of a dense ultra-relativistic electron beam with a thin solid conductor. Energetic gamma-rays are copiously produced as the electron beam splits into filaments while propagating across the conductor. The resulting gamma-ray energy and flux enable novel experiments in nuclear and fundamental physics.

The typical wavelength of light interacting with an object of the microcosm scales with the size of this object. For atoms, this ranges from visible light to...

All Focus news of the innovation-report >>>

Anzeige

Anzeige

VideoLinks
Industry & Economy
Event News

Invitation to the upcoming "Current Topics in Bioinformatics: Big Data in Genomics and Medicine"

13.04.2018 | Event News

Unique scope of UV LED technologies and applications presented in Berlin: ICULTA-2018

12.04.2018 | Event News

IWOLIA: A conference bringing together German Industrie 4.0 and French Industrie du Futur

09.04.2018 | Event News

 
Latest News

Complete skin regeneration system of fish unraveled

24.04.2018 | Life Sciences

Scientists create innovative new 'green' concrete using graphene

24.04.2018 | Materials Sciences

BAM@Hannover Messe: innovative 3D printing method for space flight

24.04.2018 | Trade Fair News

VideoLinks
Science & Research
Overview of more VideoLinks >>>