GOES-R Instruments Complete Spacecraft Integration

Two of the six instruments that will fly on NOAA's first Geostationary Operational Environmental Satellite - R (GOES-R) satellite have completed integration with the spacecraft.

The Solar Ultraviolet Imager (SUVI) and Extreme Ultraviolet and X-ray Irradiance Sensors (EXIS) were installed on the sun-pointing platform.

They will observe the sun and space weather, including coronal mass ejections, solar flares and ion fluxes that can disrupt power grids, communication and navigation systems and create radiation hazards.

"This development highlights the forward progress underway to complete the installation of the space weather instrument suite onto the GOES-R spacecraft," said Pam Sullivan, GOES-R Flight Project Manager at NASA Goddard Space Flight Center, Greenbelt, Maryland.

"It is critical we give our partners at NOAA's Space Weather Prediction Center the tools they need to improve prediction capabilities and further our knowledge of space weather."

Understanding Space Weather
The space weather mission is an important part of not only the overall GOES-R Series Program, but also NOAA's National Weather Service (NWS), which is home to the Space Weather Prediction Center.

Space weather describes the conditions in space that affect Earth and its technological systems. Space weather storms originate from the sun and occur in space near Earth or in the Earth's atmosphere.

Space weather can be difficult to understand since it is unlike the weather we experience here on Earth. For example, one type of space weather, known as coronal mass ejections, can have changing polarities, which can make it more challenging to predict the impacts of the magnetic storm.

Watch here to learn more about how space weather impacts our everyday lives. To help kids understand space weather, the GOES-R Program partnered with NASA to create materials available here for students and teachers.

Installation of the SUVI and EXIS instruments moves the program another step closer to the launch of the GOES-R satellite in early 2016.

In addition to SUVI and EXIS, the Advanced Baseline Imager (ABI) and the Space Environment In-Situ Suite (SEISS) were delivered for integration earlier this year and will be installed on the spacecraft in the coming months.

The two remaining instruments that complete the GOES-R Series Program payload are the Magnetometer and Geostationary Lightning Mapper (GLM). Both instruments are scheduled for delivery later this year.

NOAA manages the GOES-R Series Program through an integrated NOAA-NASA office, staffed with personnel from both agencies and located at NASA's Goddard Space Flight Center in Greenbelt, Maryland.

Measuring Mars Anomalies: The MAVEN Magnetometer

When you navigate with a compass you can orient yourself thanks to Earth's global magnetic field. 

But on Mars, if you were to walk around with a compass it would haphazardly point from one anomaly to another, because the Red Planet does not possess a global magnetosphere. 

Scientists think that this lack of a protective magnetic field may have allowed the solar wind to strip away the Martian atmosphere over billions of years, and now NASA's MAVEN spacecraft will study this process in detail with its pair of ring core fluxgate magnetometers. 

To download the original video please go here. Credit: NASA/Goddard/Dan Gallagher

When the Mars Atmosphere and Volatile Evolution (MAVEN) mission begins its journey to the Red Planet in 2013, it will carry a sensitive magnetic-field instrument built and tested by a team at NASA's Goddard Space Flight Center in Greenbelt, Md.

Scheduled for launch in late 2013, MAVEN will be the first mission devoted to understanding the Martian upper atmosphere.

The goal of MAVEN is to determine the history of the loss of atmospheric gases to space through time, providing answers about Mars' climate evolution.

By measuring the current rate of escape to space and gathering enough information about the relevant processes, scientists will be able to infer how the planet's atmosphere evolved.

The trip to Mars takes 10 months, and MAVEN will go into orbit around the planet in September 2014.

The Goddard-built MAVEN magnetometer will be a sensitive tool investigating what remains of the Red Planet's magnetic "shield." It will play a key role in studying the planet's atmosphere and interactions with solar wind, helping answer the question of why a planet once thought to have an abundance of liquid water became a frozen desert.

"The MAVEN magnetometer is key to unraveling the nature of the interactions between the solar wind and the planet," said MAVEN principal investigator Bruce Jakosky from University of Colorado at Boulder's Laboratory for Atmospheric and Space Physics (CU/LASP).

The magnetometer will measure the planet's magnetic field through a series of coils, each containing a magnetic ring wrapped around a metal core. The sensors, known as "flux gates," are driven in and out of saturation by applied magnetic fields.

If there is no ambient magnetic field, the sensors remain balanced. If there is an ambient field present, the sensors will go into saturation more quickly in one direction than the other. It's the imbalance that reveals the presence of an ambient field.

"A magnetometer is like an electronic compass," said Jack Connerney, mission co-investigator at Goddard. "But we measure the strength, as well as the direction, of the magnetic field."

The importance of studying the planet's magnetic field is rooted in the theory that Mars lost its global magnetic field billions of years ago, allowing the solar wind to strip the atmosphere and dry out the planet.

Unlike Earth's global magnetic field, which surrounds the entire planet, Mars only has patches of magnetic field left in its crust. This can create pockets of atmosphere that are protected against solar wind and others that are left vulnerable.

By measuring sections of the planet's magnetic field, the magnetometer could help scientists create a bigger picture of the planet's overall atmosphere.

"The magnetometer helps us see where the atmosphere is protected by mini-magnetospheres and where it's open to solar wind," Connerney said. "We can study the solar wind impact and how efficient it is at stripping the atmosphere."