The NASA Chromospheric Layer Spectropolarimeter-2 ,or CLASP-2 sounding rocket mission, was successfully conducted on April 11 from the White Sands Missile Range in New Mexico, launched aboard a NASA Black Brant IX sounding rocket at 12:51 p.m. EDT — the CLASP-2 payload flew to an altitude of 170 miles before descending by parachute.
The payload was recovered and is reported in good condition. Good data was received and the science team is reported to be happy with the results of the mission.
CLASP-2, the acronym for Chromospheric Layer Spectropolarimeter-2, is a sounding rocket mission. Smaller, more affordable and faster to design and build than large-scale satellite missions, sounding rockets offer a way for the team to test their latest ideas and instruments — and achieve rapid science results.
The CLASP-2 instrument uses ultraviolet light to look for hidden details in a complex region of the Sun's atmosphere called the chromosphere. Scientists hope that CLASP-2 experiment will help unlock new clues about how the Sun's energy travels up through the layers of its atmosphere, and eventually out into space.
The Sun was observed for about five minutes and images were captured, as well as polarization spectra — observations that restrict incoming light to a specific direction and then record the intensity of individual wavelengths of ultraviolet light. The NASA team's focus was on obtaining polarization measurements that have never before gathered at these ultraviolet wavelengths.
CLASP-2 is a follow-on mission to the Chromospheric Lyman-Alpha Spectro-Polarimeter, which offered the first-ever polarization measurements of ultraviolet light emitted from the sun's chromosphere. Previous polarization measurements were restricted to visible and infrared light emitted from other regions of the Sun’s atmosphere.
Polarization measurements are important as they provide information on the strength and direction of the Sun's magnetic field, which plays a central role in sculpting the solar atmosphere. Understanding how the magnetic field works is vital to predicting powerful solar activity and protecting space and Earth technology from potential damage from geomagnetic storms.
On the ground, researchers will use advanced computer modeling to interpret the data collected by CLASP-2 and better understand how the energy moves through the chromosphere. And even as CLASP-2 uncovers new information, scientists working with its data will rely on data from other observatories to help put those details in context.
CLASP-2's launch and data collection will be coordinated with two satellites: NASA's Interface Region Imaging Spectrograph, or IRIS--a satellite observatory that captures non-polarized spectra and images of the Sun’s atmosphere--and the joint JAXA/NASA Hinode satellite observatory, making magnetic measurements at the Sun’s surface as well as images and spectroscopy in the much hotter atmospheric layer known as the corona. Also taking coordinated data are the Dunn Solar Telescope in Sunspot, New Mexico, and the Goode Solar Telescope in Big Bear, California.
CLASP-2 is an international collaboration led by NASA's Marshall Space Flight Center with contributions from Japan, Spain and France. CLASP-2 is supported through NASA’s Sounding Rocket Program at the agency’s Wallops Flight Facility in Virginia. NASA’s Heliophysics Division manages the sounding rocket program.