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Laboratory for Atmospheric and Space Physics

June 2016 Rocket Launch Successful

June 1, 2016
Rocket Recovery Team-June 2016

The rocket recovery team waiting for the helicopter to transport the rocket back to the WSMR launch area.

After a one-week delay due to high winds, the latest SDO EVE calibration rocket successfully launched on Wednesday, June 1, from White Sands Missile Range (WSMR) in New Mexico. NASA Rocket 36.318 provided the fifth underflight calibration for solar EUV spectrographs aboard SDO, TIMED, SORCE, SOHO, GOES, PROBA2, and Hinode. The TIMED SEE instrument was launched Dec. 7, 2001 and began making daily measurements on January 22, 2002. The rocket calibration flights have occurred about once a year for the past fifteen years to accurately determine the long-term variations of the solar extreme ultraviolet irradiance. The TIMED project supported the calibration experiments from 2001 to 2008, and the SDO project has supported the calibration experiments since 2008.

The June 2016 calibration payload included rocket versions of the SDO EVE and the GOES-R XRS satellite instruments. All of the instruments got excellent measurements and will provide reference spectra for June 1, 2016 when the F10.7 was 88. The payload normally spends about 15 minutes in space with a peak altitude of about 180 miles to obtain the necessary solar EUV spectral irradiance observations. The payload then re-enters and lands via parachute and is recovered for use on future suborbital flights. For NASA Rocket 36.318, LASP and USC provided the science instruments and NASA provides all the other subsystems (launch vehicles, telemetry, attitude control, parachute / recovery, etc.). A video, courtesy of Chris Jeppesen at LASP, shows the forward and aft onboard camera feeds and is posted at It shows the forward and aft cameras side-by-side and synced in time for the full flight.

Following the recovery, the rocket payload was driven back to LASP for post flight functional tests and a more detailed inspection, as it will be re-used for future flights. TIMED/SEE PI Tom Woods and the rest of the TIMED and SDO team members are looking forward to the next rocket flight –planned for June 2018.

SEE V11 30-105nm Calibration

The degradation trend for the SEE instrument is derived with weekly on-board redundant channel and rocket underflight calibrations. The SEE Version 11 product only has degradation correction until 2012; the SEE Version 12 product will provide an updated correction that currently indicates a degradation trend of ~3%/year.

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